DE05F5029

UNIVERSITÄT BONN Physikalisches Institut

Families and Degenerations of Conformal Field Theories

von Daniel Roggenkamp »DEO21241946*

In this work, moduli spaces of conformal field theories are investigated. In the first part, moduli spaces corresponding to current-current defor- mation of conformal field theories are constructed explicitly. For WZW models, they are described in detail, and sigma model realizations of the deformed WZW models are presented. The second part is devoted to the study of boundaries of moduli spaces of conformal field theories. For this purpose a notion of convergence of families of conformal field theories is introduced, which admits certain degenerated conformal field theories to occur as limits. To. such a degeneration of conformal field the- ories, a degeneration of metric spaces together with additional geometric structures can be associated, which give rise to a geometric interpreta- tion. Boundaries of moduli spaces of toroidal conformal field theories, orbifolds thereof and WZW models are analyzed. Furthermore, also the limit of the discrete family of Virasoro minimal models is investigated.

Post address: BONN-IR-2004-14 Nussallee 12 Bonn University- 53115 Bonn September 2004 Germany ISSN-0172-8741

Contents

1 Introduction 4

2 Moduli spaces of WZW models 8 2.1 Current-current deformations of CFTs 10 2.2 Some deformation theory 13 2.3 Deformations of WZW models 17 2.4 Sigma model description of deformed WZW models 20 2.4.1 Classical Action 20 2.4.2 Thedilaton 25 2.5 Explicit example: su(2)fc 31 2.6 Discussion 35

3 Limits and degenerations of CFTs 38 3.1 From geometry to CFT, and back to geometry 39 3.1.1 From Riemannian geometry to spectral triples 40 3.1.2 Spectral triples from CFTs 43 3.1.3 Commutative (sub)-geometries 47 3.2 Limits of conformal field theories: Definitions 52 3.2.1 Sequences of CFTs and their limits 52 3.2.2 Geometric interpretations 60 3.3 Limits of conformal field theories: Simple examples 64 3.3.1 Torus models 64 3.3.2 Torus orbifolds . . 69 3.3.3 WZW models 71 3.4 The m —* oo, c —> 1 limit of the unitary Virasoro minimal models M(m,m+ 1) 73 3.4.1 The unitary Virasoro minimal models A4(m, m + l)m_>oo 74 3.4.2 Geometric interpretation of M.(m,m + l)™-^ 81 3.5 Discussion 87

A Properties of conformal field theories 89

B c = 1 Representation theory 93

C Structure constants of the unitary Virasoro minimal models, and their c —> 1 limit 97

1 Introduction Moduli spaces of conformal field theories are important objects in the study of two dimensional quantum field theories because they describe critical subspaces in the space of coupling constants. In string theories, whose small coupling limits are described by conformal field theories,, these moduli spaces arise as parameter spaces of string vacua. The understanding of moduli spaces .of conformal field theories is thus a very important issue for string theory. However, although conformal field theories are quite well understood, there are only few examples of explicitly known moduli spaces at present, most of which correspond to free field theories as e.g. toroidal conformal field theories or orbifolds thereof. The reason for this is that a good conceptual understanding of deformations of conformal field theories beyond conformal perturbation theory is still lacking. Perturbation theory is usually technically involved, at least when one wants to obtain higher order contributions, and hence is only applicable to study CFT moduli spaces in small neighborhoods of explicitly known models. In particular it is in general not possible to obtain global information about the moduli spaces from perturbation theory, except in situations, where symmetry as e.g. super- symmetry is preserved by the corresponding deformations. In this work, the problem of understanding moduli spaces of conformal field theories is approached in two different ways. The first part, Sect. 2, which is based on joint work with Stefan Forste published in [39] is devoted to the study of a special class of deformations of conformal field theories, namely CURRENT- CURRENT DEFORMATIONS. All known deformations of conformal field theories are generated by per- turbations of the theory with exactly marginal fields, and it is widely believed that in fact all deformations of CFTs can be obtained in this way. Deforma- tions which are generated by perturbations with products of holomorphic and antiholomorphic currents are called current-current deformations. As was shown in [16], such deformations preserve the algebras of the cur- rents from which the perturbing fields are constructed. It turns out that this gives enough structure to determine global properties of the subspaces of mod- uli spaces corresponding to this kind of deformations. Namely we show that current-current deformations only affect the representation theory of the alge- bra generated by the currents involved in the perturbation, and not those of its commutant. In particular the coefficients of the operator product expansion of highest weight states with respect to this algebra are invariant. This allows us to explicitly construct the corresponding deformation spaces which have basis of the form O{d,d)/O{d)xO(d), where d and d are the numbers of holomorphic and antiholomorphic currents which generate the deformations. The corresponding moduli spaces are obtained by identifying isomorphic CFTs in these spaces which amounts to dividing out discrete " groups". The latter strongly depend on the structure of the CFTs under consideration. In fact, this generalizes the treatment of deformations of toroidal conformal field theories, whose moduli spaces have been constructed in [83, 15, 23], and it gives a new class of very explicitly known families of conformal field theo- ries. Namely, to each conformal field theory which possesses holomorphic and antiholomorphic currents, such families can be constructed. Important examples of non-free conformal field theories admitting current- current deformations are WZW models (see e.g. [54]). Moduli spaces of current- current deformed WZW models associated to compact semi-simple Lie groups are analyzed in detail. Furthermore a sigma model description of the deformed WZW models is derived. It is shown that like the undeformed WZW models, also the deformed ones admit representations as sigma models with Lie group target spaces. Sigma model-metric, B-field and dilaton are obtained explicitly as functions on the deformation spaces. For this, a representation of the deformed WZW models as orbifolds of products of coset- and toroidal conformal field theories is used, which is mimicked in a sigma model construction. Thus, we gain an explicit description of the moduli spaces of current-current deformed WZW models, in terms of conformal field theory as well as in terms of sigma models. The second part of this work, Sect. 3, which is based on joint work with Katrin Wendland published in [89] is devoted to the study of boundaries of CFT moduli spaces. In general, moduli spaces of conformal field theories, e.g. the moduli spaces discussed in Sect. 2 are not complete and it is an interesting question what happens to the CFT structures if one approaches the moduli space boundaries. Indeed, limits and degenerations of conformal field theories have occurred in various ways in the context of compactifications of moduli spaces of CFTs, in particular in connection with string theory. For example, zero curvature or large volume limits of CFTs that correspond to sigma models are known to give boundary points of the respective moduli spaces [3, 81]. These limits provide the connection between string theory and classical geometry which for instance is used in the study of D-branes. Also in the Strominger-Yau-Zaslow mirror construction [100, 95, 62], boundary points play a prominent role. In fact, Kontsevich and Soibelman have proposed a mirror construction on the basis of the Strominger-Yau-Zaslow conjecture which relies on the structure of the boundary of certain CFT moduli spaces [72], All the examples mentioned above feature interesting degeneration phenom- ena. Namely, subspaces of the Hubert space which are confined to be finite dimensional for a well-defined CFT achieve infinite dimensions in the limit. In fact, such degenerations are expected if the limit is formulated in terms of non- linear sigma models, where at large volume, the algebra of low energy observables is expected to yield a non-commutative deformation of an algebra ^4°° of func- tions on the target space. The algebra of observables whose energy converges to zero then reduces to A°° at infinite volume. An entire non-commutative ge- ometry can be extracted from the underlying CFT, which approaches the target space geometry in the limit [42]. By construction, this formulation should encode geometry in terms of Connes' spectral triples [19, 20, 21]. By the above, degeneration phenomena are crucial in order to single out an algebra which encodes geometry in CFTs. An intrinsic understanding of limiting processes in CFT language is therefore desirable. This will also be necessary in order to take advantage of the geometric tools mentioned before, away from those limits. Vice versa, a good understanding of such limiting processes in CFTs could allow to take advantage of the rich CFT structure in geometry. The main aim of the investigations is to establish an intrinsic notion of such limiting processes in pure CFT language and to apply it to some interesting examples. To this end, a definition of CONVERGENCE FOR SEQUENCES OF CFTs is given, such that the corresponding limit has the following structure: There is a limiting pre-Hilbert space H°° which carries the action of a Virasoro algebra, and similar to ordinary CFTs to each state in H°° we assign a tower of modes. Under an additional condition the limit even has the structure of a CFT on the sphere. This is the case in all known examples, and in particular, this notion of limiting processes is compatible with deformation theory of CFTs in the sense that limits of compact one-parameter families of CFTs are full CFTs, i.e. those defined on arbitrary surfaces. If the limit of a converging sequence of CFTs has the structure of a CFT on the sphere, but is not a full CFT, then this is due to a degeneration as mentioned above. In particular, the degeneration of the vacuum sector can be used to read off a geometry from such a degenerate limit. Namely, in our limits the algebra of zero modes assigned to those states in 7i°° with vanishing energy is commutative and can therefore be interpreted as algebra of smooth functions on some manifold M. The asymptotic behavior of the associated energy eigenvalues allows to read off a degenerating metric on M and an additional smooth function corresponding to the dilaton as well. Moreover, being a module of this commutative algebra, H00 can be interpreted as a space of sections of a sheaf over M as is explained in [72]. Simple examples which these techniques are applied to are the torus models, where the limit structure yields geometric degenerations of the corresponding target space tori ä la Cheeger-Gromov [17, 18]. In this case, Ti.°° is the space of sections of a trivial vector bundle over the respective target space torus. Similar statements are true for orbifolds of torus models, only that in this case the fiber structure of H°° over the respective torus orbifold is non-trivial. Namely, the twisted sectors contribute sections of skyscraper sheaves localized on the orbifold fixed points. Degenerations of CFTs in current-current deformation spaces constructed in Sect. 2 also give rise to geometric degenerations of tori. In this case, 7i°° correspond to spaces of sections of trivial vector bundles with fiber given by Hubert spaces of certain coset models. These coset models arise from the original CFTs in the deformation spaces by means of the coset construction with respect to certain subalgebras of the current algebras which generate the deformations. Another example, which is studied in detail and in fact was the starting point of these investigations is the family of unitary Virasoro minimal models. It strongly differs from the examples mentioned before in that it is a discrete family of CFTs, which even does not have constant central charge. This makes the construction of the sequence, the verification of convergence and the analysis of its limit much more involved. Nevertheless, it turns out that the A-series of unitary Virasoro minimal models indeed constitutes a convergent sequence of CFTs. All fields in its limit theory at infinite level can be constructed in terms of operators in thesu(2)i WZW model. The sequence degenerates, and the limit has a geometric interpretation in the above sense on the interval [0, TT] equipped 1 with constant metric 'g = dx® dx and dilaton <&(z) = In (•s/^sm~ x). A different limit for the A-series of unitary Virasoro minimal models at in- finite level was proposed in [61, 90, 91]. It is described by a well-defined non- rational CFT of central charge one, which bears some resemblance to Liouville theory. In particular, its spectrum is continuous, but degenerations do not occur. The techniques developed in Sect. 3 can also be used to describe this latter limit. The between the two different limit structures is best compared to the case of a free boson, compactified on a circle of large radius, where apart from the degenerate limit described above one can also obtain the decompactified free boson. While the degenerate limit focused on in this work has the advantage that it leads to a consistent geometric, interpretation, the one which corresponds to the decompactified free boson gives a new well-defined non-rational CFT.

Acknowledgements Ich danke meinem Doktorvater Werner Nahm und Matthias Gaberdiel, Andreas Recknagel und Katrin Wendland, die mich mit Rat und Tat unterstützt haben. Für die Zusammenarbeit an in die Arbeit eingegangen Artikeln bedanke ich mich bei Stefan Forste und Katrin Wendland. Ferner danke ich für Ihre Unterstützung dem DFG-Schwerpunktprogramm 1096, dem Marie-Curie-Trainingssite am Mathematics Department des King's College London, dem Institut für Theoretische Physik der ETH-Zürich und dem Institute for Pure and Applied Mathematics, UCLA sowie der "BIGS". 2 Moduli spaces of WZW models

In this section, special deformations of conformal field theories, namely those generated by perturbations with products of holomorphic and antiholomorphic currents are studied. As was shown in [16], such deformations preserve the alge- bras of the perturbing fields. Indeed, this allows to determine global properties of the subspaces of moduli spaces corresponding to this kind of deformations. Important examples of non-free conformal field theories admitting current- current deformations are WZW models (see e.g. [54]). The corresponding moduli spaces for WZW models associated to compact semi-simple Lie groups, will be discussed in detail. Since WZW models have descriptions as sigma models on Lie groups, it is a natural question if there are such descriptions for all conformal field theories from these moduli spaces. In fact, families of sigma models containing WZW models at special points have been discussed by many authors (e.g. in [63, 58, 94, 70, 55]). In particular one-parameter families of sigma models containing the su(2)fc-WZW models have been studied very explicitly by Giveon and Kiritsis [58], who also compared them to the families of current-current deformed su(2)fc- WZW models which were described in [101]. Ideas about a generalization of these considerations to arbitrary WZW models have also been presented in [58, 70, 71]. Here, WZW-like sigma model representations of current-current deformed WZW models will be explicitly constructed. These are sigma models with the same target space as the "undeformed" WZW model in the family, but with different (in general not bi-invariant) metrics, additional £f-fields and dilaton. The latter are constructed as functions on the deformation spaces. Thus, we obtain explicit descriptions of the moduli spaces of current-current deformed WZW models associated to compact semi-simple Lie groups in terms of conformal field theories as well as in terms of sigma models. In Sect. 2.1, exactly marginal current-current deformations of conformal field theories are discussed. We start from the facts obtained in [16], that perturba- tions of conformal field theories with products of holomorphic and antiholomor- phic currents are exactly marginal iff the holomorphic as well as the antiholo- morphic currents belong to commutative current algebras, and that in this case these holomorphic and antiholomorphic current algebras are preserved under the deformations. This can be used to reduce the problem of studying finite current- current deformations to first order deformation theory, which is carried out in Sect. 2.2, and from which it follows that the effect of these deformations on the CFT structures is completely captured by pseudo orthogonal transformations of their charge lattices with respect to the preserved commutative current algebras. The corresponding deformation spaces can thus be described by

V S 0{d, d)/O{d) x O(d). (2.1)

This generalizes the deformation results of toroidal conformal field theories [23]. The corresponding moduli spaces are obtained from the deformation spaces by taking quotients with respect to "duality groups". In Sect. 2.3 we discuss an important class of examples, namely WZW models corresponding to compact semi-simple Lie-groups. The general results from Sect. 2.1 are compared to a realization of deformed WZW models obtained from a representation of WZW models as orbifolds of products of generalized parafermionic and toroidal models given in [51]. In Sect. 2.4 various aspects of exactly marginal deformations of WZW models are analyzed from a sigma model perspective. This approach is best suited for a semiclassical treatment and in that sense less powerful than the algebraic one. However, it can illustrate the results and provide a picture for the class of deformed models. Exactly marginal deformations of WZW models from the sigma model perspective have been discussed in the past mainly for rank one groups [63, 58, 94] and for models where coordinates can be chosen such that the relevant set of chiral and anti-chiral currents follows manifestly from the equations of motion [64]. Mimicking the orbifold realization of deformed WZW models described in Sect. 2.3, we will consider an orbifold of a direct product consisting of a vectori- ally gauged WZW model and a d-dimensional torus model, where d is the rank of the group. Since a sigma model is not very well designed to accommodate orbifolds, we perform an axial-vector duality (generalized T-duality) to obtain a dual description without an additional orbifold action. To this end, we first implement the orbifold by gauging in addition an axial symmetry of the WZW model combined with shifts in the torus factor. We force the corresponding gauge connection to be flat but choose the zero modes of the corresponding La- grange multiplier such that the gauge bundle is twisted in a non-trivial way. It turns out that integrating out the gauge field instead of the Lagrange multiplier provides a sigma model without an additional orbifold action. The result is a "WZW-like" model, i.e. a sigma model with Lie group as target space, and a WZW-type action in which the bi-invariant metric is replaced by a more general bilinear form which is neither bi-invariant nor necessarily symmetric. The same sigma models can be obtained as coset models of a product of the original WZW model and d-dimensional torus models with gauge group U(l)d, embedded into both factors. All the sigma model manipulations described so far are carried out at a classical level. In full quantum field theory one has to replace the procedure of solving equations of motion by performing Gaussian functional integrals. These in general provide functional determinants, which in turn generate a non-trivial dilaton. In a pragmatic approach this can be computed by imposing conformal invariance, i.e. requiring vanishing beta functions. We will use a more elegant way consisting of a comparison of the Hamiltonian of the model and a generalized Laplacian, which depends on the dilaton [98]. Finally in Sect. 2.5, some of the results are illustrated in the example of the deformed su(2)fc-WZW model. 2.1 Current-current deformations of CFTs Although, not proven in general, it is widely believed that all deformations of con- formal field theories are generated by perturbations of the theories with marginal fields, i.e. fields Oi with conformal weights h(Oi) = 1 = h(Oi). The perturbed correlation functions on a conformal surface S of a combina- tion of operators X{p\,... ,Pk), Pi € £ are defined to be

:= (X(pu...,pk)exp fo^i/ 0iC^Ej>E, (2.2) where the integrals have to be regularized due to the appearance of singularities. If the perturbed correlation functions define a quantum field theory, which is a fixed point of the renormalization group flow, it is again a conformal field theory. This however is not the case in general. Indeed, preservation of conformal. invariance by perturbations gives non linear restrictions on the fields, which generate it (see e.g. [23]). This means that the set of exactly marginal fields, i. e. those which generate deformations of conformal field theories are not vector spaces in general. In particular the deformation spaces of conformal field theories need not necessarily be manifolds but may have singularities. (For more details on conformal deformation theory see e.g. [23, 73, 84, 85]). In the following, deformations of conformal field theories generated by a special class of marginal fields, namely products of holomorphic and antiholo- morphic currents will be discussed. These are simple enough to give a global description of the deformation spaces corresponding to them and to express the data of deformed CFTs explicitly in terms of the data of the undeformed ones. We consider conformal field theories, whose holomorphic and antiholomor- phic VF-algebras contain current algebras g^, g^ corresponding to Lie algebras g and g and k, k G N, i.e. for every j, f G g there exist holomorphic fields j{z),f(z) of conformal weight h = 1 in the theory, such that

m/ \ ., ^ j(w) dj(w) T{z)j(w) = JK ; + JK \ + reg, (z - w)z (z — w) where Kg(.,.) is a bi-invariant scalar product on g and [.,.] its Lie bracket. The holomorphic energy momentum tensor T{z) can be written as

9) aß

a with g the dual Coxeter number of g, (j )a a basis of g and TQ(Z)J(W) — reg. The same holds for the antiholomorphic current algebra replacing (g, k) by (g, k). In particular, there is a subspace of the CFT Hubert space isomorphic to g ® g of marginal fields. However, not all of these fields are exactly marginal. As was shown in [16], such fields are exactly marginal if and only if, under

10 the isomorphism above, they correspond to elements of a a, for some abelian subalgebras o C g, ö C g. Moreover deformations generated by these exactly marginal fields preserve the current algebras o, ö corresponding to a, a. Hence, every pair of abelian ü(l)d = oCg, ü(l)d = äCg gives rise to a family of conformal field theories with current algebras a, a. All these families meet in the original model, and those pairs which are identified under a CFT- automorphism give rise to equivalent deformations. We assume in the following that the conformal field theory is unitary, and its Hubert space decomposes into tensor products of irreducible highest weight representations VQ, V-Q of a, a, which are characterized by their charges Qea*, Q E a*, and whose lowest eonformal weights are given by HQ = \K{Q,Q), 1 h = \~K(Q, Q), as can be read off from (2.4) :

KQQ®VQ®VQ. (2.5)

The set of charges A C a* x ä* forms a equipped with bilinear pairing

K© (—«)• As is shown in Sect. 2.2, deformations corresponding to pairs (a, ä) only affect the representation theory of the W-algebras a, a, but not the OPE-coefncients of a © ä-highest weight vectors. More precisely, if one chooses suitable connections on the bundles of Hubert spaces over the deformation spaces [85], the effect of the deformations on the CFT structures is completely captured by transformations of the charge lattices A in the identity component O(d, d)o of the pseudo orthogonal group O(d,d), and all structures independent of the charges are parallel with respect to the chosen connection. That O(d, cQo-transformations of the charge lattice A indeed give rise to new modular invariant partition functions and also preserve locality is easy to see even without any perturbation theory. Namely, for O € O(d, d) define deformed operators L®, Lo on Ji by

: L + (Lo + Lo) lwe?i5!?<8>v<3<8>% = ( ° + (O* -

:= L (LQ-LO) I«QI3®V0®% ( 0 - + (O* - 1)(K© -S)((g,Q),

Locality is maintained because of the preservation of «©(—7c) by transformations O £ O(d,d). To show the preservation of modular invariance we consider the torus partition function depending on modular parameters r and r (q = e2mT, q = e~2mr) of the O(i)-transformed model along a smooth path O : [—1,1] —»

1From now on K = £K8|O, « =

11 O(d,d)0 with O(O) = 1, dtO(t)\t=0 = Te o{d,d)

(2.6)

and use the modular transformation properties of the unspecialized characters (see e.g. [66]):

(Z) (2-7)

27T2 —• 2irt where q = e~r~, g = e~?~. This shows that invariance under the modular trans- formation T h-> — i is preserved under O(d, (^-transformations of the charge lattices. A similar calculation proves the statement for THT + 1. Since charges (Qi Q) only characterize the o©a-modules up to automorphisms of the underlying Lie algebras, transformations of A by O(d) x O(d) C O(d,d) leave the conformal field theory invariant. Thus, the deformation spaces corre- sponding to pairs (a, a) are given by

P(o,s) = O(d, d)0/((O(d) x 0(5)) n O(d,5)0) = 0(d,5)/0(d) x 0(5). (2.8)

To get the respective moduli spaces from these deformation spaces, one has to identify points describing equivalent conformal field theories. In fact, the con- formal field theories are specified by the charge lattices marked with the Hubert spaces Hrq -Q. of a © ä-highest weight states (with all the structure they carry, as e.g. structure of modules of the Virasoro algebra etc.) and the coefficients of the operator product expansion of these highest weight states. Denoting these additional structures by S, and the automorphisms of A together with S by Aut(A, S), the components of the moduli spaces corresponding to (o,a) defor- mations can be written as

= Aut(A, S)\O(d,d)/O{d) x 0(5). (2.9)

If the action of Aut(A, S) has fixed points, M.(a$) has singularities and the Hilbert space bundle over it has non-trivial monodromies around them. More

12 precisely elements in Aut(A, 5) act on the Hubert space bundles over the defor- mation spaces, and monodromies around fixed points are given by the respective actions of the stabilizers. This gives a very explicit description of the components of moduli spaces of conformal field theories corresponding to current-current deformations. In particular conformal field theories as above come in £>(a,o) families of explicitly known CFTs, and the conformal field theory data at any point in these families can be easily reconstructed from the CFT data at one point. A well known example of this kind is the moduli space of toroidal conformal field theories. These models have holomorphic and antiholomorphic W-algebras, each of which contains a u(l)d current-algebra. They are completely character- ized by their charge lattices CHQQ are trivial for all charges), which for integer spin of the fields, locality and modular invariance of the torus partition function have to be even, integral, selfdual lattices of signature (d, d) in Rd'd [15, 83]. Hence, S is trivial and Aut(A,5) = Aut(A) = O(d,d,Z), such that the moduli spaces Md,d corresponding to the current-current deformations are isomorphic to the Narain moduli spaces [83]

^ Z)\O{d, d)/O{d) X 0{d) , (2.10) of even, integral selfdual lattices of signature (d, d) in M.d

2.2 Some deformation theory In this section, techniques from conformal deformation theory (see e.g. [23, 73, 84, 85]) are used to calculate the effect of current-current deformations on arbi- trary conformal field theories containing current algebras in their holomorphic and antiholomorphic W-algebras. In the following, a family of conformal field theories is regarded as a Hermi- tian vector bundle over a differentiate manifold2 parametrizing deformations of the conformal field theory structures in a smooth way, i.e. all CFT structures are smooth sections of corresponding vector bundles. Such families can be realized as perturbations (2.2) by exactly marginal fields. In this case, the tangent bundle of their base manifolds are subbundles of the Hermitian vector bundles. The choice of regularization method and renormaliza- tion scheme gives rise to connections on them [85]. Here connections D (called c in [85]) will be used, which restrict to the Levi-Civita connections on the tan- gent bundles of the base manifolds equipped with the respective Zamolodchikov metrics. These connections are defined by "minimal subtraction" of divergences in the regularization constant. Given a conformal field theory, it is in general quite hard to make global statements about the family of conformal field theories, generated by pertur- bation with a given set of exactly marginal fields. This is due to the fact that Singularities do not occur in our situation.

13 information on the CFT structures in points of the family have to be more or less completely reconstructed out of the structures at one point (the point corresponding to the CFT which is being perturbed), by means of perturbation theory. Thus, one gets perturbative results only, and perturbation theory usually becomes technically difficult at higher orders. However, in the case of perturbations by products of holomorphic and an- tiholomorphic currents, there is in fact enough structure to make exact global statements about the families of CFTs generated by them using first order per- turbation theory only. In [16] it was shown that tensor products of fields of holomorphic and an- tiholomorphic currents are exactly marginal, if and only if they form abelian current algebras ä, ä respectively, and that in this case the deformations gener- ated by them preserve the corresponding current algebras a and ci. Thus these deformations give rise to families of conformal field theories with ä and ö con- tained in their holomorphic and antiholomorphic W-algebras. Moreover, the tangent vectors to the families in every point are given by products of currents, whose CFT-properties are known independently of the actual CFT. Thus the derivatives of the CFT-structures can be calculated in every point of the families and can then be integrated up. Assuming that the Hubert spaces of the conformal field theories in the fam- ilies decompose into a © ä-highest weight representations as in (2.5)

n ~ 0 ^QQ®VQ®VQ. it is shown in the following that these deformations only affect the a © ä- repre- sentations, while the OPE-coefficients of d © o-highest weight states are parallel with respect to the connection D. To be more precise, the only effect of the deformations will be O(d, ^-transformations of the charge lattices A € a* x a*. From this it follows in particular that the corresponding deformation spaces are given by (2.8)

,5) = O(d,d)o/(0(d) x O(3))0 = 0{d,d)/0{d) x O(d). (2.11) First of all, by the coset construction [60], the holomorphic W-algebra W of a conformal field theory in such a family contains the coset algebra W/d as a subalgebra, such that [W/d, a] — 0. In particular W/d is not affected by the deformation, i.e. the elements of W/d as well as their mutual OPE are covariantly constant, which implies that W/d is contained in the W-algebras of any conformal field theory in the family. Moreover, the holomorphic energy momentum tensor T of the CFT decomposes into a sum T = Ta + T", where Ta is the energy momentum tensor associated to the current algebra d and T' belongs to the coset algebra W/d and is therefore covariantly constant. Hence, the covariant derivative of T is given by the covariant derivative of Ta. The same statements hold for the antiholomorphic W-algebra. Let us now calculate the covariant derivatives of the modes of the d- and ö-currents and holomorphic and antiholomorphic energy-momentum tensors de-

14 fined by

n T(z) = ^J z -*Ln, T(z) = neZ neZ

a a where, as in Sect. 2.1 (j )a and {j )a are basis of a and ö respectively, and we denote the generators of the deformations by Oaa(z,~z) := ja(z)ja('z). By the definition of D, DOaajn can be expressed as

^ -8 ( T^ -B\ \ 1 dz _n f L 27r l ^ 'n /c(0) ^ JCP \D€{z) (2.13) where e is the regularization parameter and [X]€ means the regularization pa- rameter independent part of X3. Using the OPE (2.3) this can be expressed as

L /c.(0) ^ C(w)

l 2l = [fJce(o) ^ aß = -nkK ^5nfi. (2.14)

The same kind of arguments lead to p-.z~n f C(0) Z7rz JCPi-\Dt(z) Je (2.15) and similar expressions for the modes of ä. Altogether we find

aß Doc-sß = -iykK 5nfiJZ, Doa«Ln = -irj%j%, (2.16)

Since the zero modes j%, jfi belong to the center of a © ä, the ä © ä-PF-algebra structure is parallel with respect to D, and only the a©a-charges4 change under these deformations. Their covariant derivatives can be read off from (2.16)

0 f , (2.17)

3 a X can be written as a sum of terms proportional to e for some a. [X]e denotes the term proportional to e°. 4As noted above, we assume the zero modes of the currents to be diagonalizable on H.

15 which are transformations in o( a* © ä*, K ©(—«)). This characterizes completely the deformations of the ä 0 ä-W-algebra structures of the CFTs. Moreover the a ©a-highest weight property and the decomposition of the Hubert space (2.5) are preserved under the deformations, which means in particular that we only have to assume (2.5) for one CFT in the family. To show that this is in fact the only effect of the deformation on the CFT structures, we have to show, that the OPE of a © a-highest weight vectors is not deformed. Now, the covariant derivative of correlation functions of those vectors is given by

(2.18)

But the ln-term in the last line of (2.18) is just the logarithm of the corresponding d-, o-conformal block. Thus, the correlation functions are deformed only through the conformal blocks and the OPE-coefficients of & © ä-highest weight states are parallel. Thus, the effect of current-current deformations on the conformal field the- ory structure is completely characterized by the deformations of the charges described above. In particular from (2.17) it follows that the base manifold of the family of CFTs generated by current-current deformations is indeed given by (2.11). Let us finish with a comment on another connection D. In the discussion above, we used connections D on the Hubert space bundles over the deforma- tion spaces, which were defined by minimal subtraction. With respect to these connections operators from the W-algebras are parallel except zero modes of the current algebra. For the discussion of e.g. boundary conditions other connections D will be useful. These are defined by5

5In fact they are nothing else than the connections f from [85], which are obtained by a regularization scheme consisting of cutting out radius one disks around the punctures of the surfaces, i.e.. in (2.13) instead of taking the regularization parameter independent part [,]t one sets e = 1.

16 They satisfy & ^f^, (2-20)

ro+n >

and thus for all n G Z, the parallel transport of (j£, j^n)a,ä is given by the vector representation of O(d,d). As the connection D, also D restricts to the Levi-Civita-connection on the tan- gent bundle of the deformation space equipped with the Zamolodchikov metric.

2.3 Deformations of WZW models WZW models are conformal field theories associated to Lie groups G with bi- invariant metrics (.,.) (see e.g. [54]). For simplicity we will only consider compact semi-simple G with bi-invariant metrics corresponding to the Killing forms on the respective Lie algebras here. So, let k G N, G a semi-simple Lie-group, g its Lie-algebra of rank d with Killing form K/k, roots A, weights Q, root lattice Q(g), coroot lattice Q(g) C Q(g), and weight lattice P(g). Furthermore denote by flk the set of integrable weights of the affine Lie-algebra gk at level k. The WZW models associated to (G,K,k) have the affine Lie algebras gk as holomorphic and antiholomorphic W-algebras. Its Hubert spaces decompose into tensor products of integrable highest weight representations V^, A G Cik of Qk- For simplicity only diagonal WZW models are considered in the following, i.e. those WZW models whose Hubert spaces are given by (2.21)

Generically, the only marginal fields in WZW models are products of holomor- phic and antiholomorphic currents from the current algebras. From the general considerations in Sect. 2.1 it is clear that every pair of Cartan subalgebras f) C g, fj C g gives rise to deformations of the WZW models. However, all such pairs lead to equivalent deformations, because all maximal abelian subalgebras of a semi-simple Lie algebra are pairwise conjugated6 and inner automorphisms of g induce automorphisms of the corresponding WZW models. Thus the deforma- tion space of current-current-deformed WZW models is given by 2>wzw^O(d,d)/O(d)xO(d). (2.22) For a given Cartan subalgebra f) C g the integrable g^-highest weight represen- tations decompose into ^-highest weight modules VQ, Q G f)* as follows

^ ® V? * © V^ ® © V(ß+kS), (2.23)

6This is not true for non-semi-simple Lie algebras, where one gets more interesting moduli spaces.

17 where F^ := P(g)/fcQ(g) is a finite abelian group, V^ is a highest weight module of a generalized parafermionic W-algebra associated to the coset construction gfc/F), and V^** are highest weight modules with respect to an extended F) W- algebra [51] 7. Prom this, the charge lattice can be read off to be

•Ao = {(/i,7*)€P(g)xP(fl)|AJ-Ä*eQ(fl)}. (2.24) The "duality group" is given by the automorphisms of Ao compatible with the additional structures S^, alluded to in the last section. In the case of diagonal WZW models discussed here, all these structure are determined by representa- tion theory, and the duality group is given by the semi-direct product

Aut(A0, Sfc) S A(g) K W(g) (2.25) of the automorphism group A(g) of the root lattice Q(g) with the Weyl group W(g), where A(g) acts diagonally on Ao C P(g) x P(g), and W(g) acts on the second factor only (see [70] for a discussion of dualities of WZW models). Since A(g) = W(g) ix F(g), the "duality" groups can be written as

Aut(A0, Sk) = (W(fl) x W(fl)) K F(g), (2.26) with the Weyl groups acting separately on the two factors of Üxfi and F(g) acting diagonally. Note that these groups are finite, as opposed to the "duality groups" of d-dimensional toroidal models for d > 1. For the special case g = su(2), the group (2.26) coincide with the toroidal "duality" group 0(1,1,Z) = Z2 x Z2. Given the duality group, the moduli space of current-current deformed WZW models can now be written as (2.10)

•Mwzw = (W(g) x W(s)) x F(0)\O(d, d)/O(d) x O(d). (2.27) In fact, Ao has an even integral selfdual sublattice

Ak := {(fi, Ji) e P(g) x P(g) \ii-pe fcQ(g)} C Ao (2.28) of signature (d, d), which can be regarded as charge lattice of d-dimensional toroidal conformal field theory. Let us denote by Aut(Afc,5fc) C Aut(Ao,5fc) the subgroup of the duality group fixing Afc. This group is also a subgroup of O(d, d, Z).

7In terms of characters xx(<7>w) corresponding to the gfc-highest weight representations, this is just the string function decomposition [67]

with cji denoting the string functions.

18 Every even integral selfdual sublattice of Ao of signature (d, d), which is obtained from A& by applying a transformation of Aut(Ao,S&) gives rise to a representation of the WZW model as orbifold model

9k = (öfc/6 0 tAk)/rfc • (2.29) of a product of a coset model ßfc/f) and a toroidal conformal field theory tAA. with charge lattices A*. Such representations were presented in [51] and were actually used in [71] in the study of dualities of WZW and coset models. The torus partition function of coset and toroidal models (with the notation from footnote 7) are given by z»kl\q,q) = E EE 4

k^

where r){q) = qu rins-iC-"- ~ #n) denotes Dedekind's 77-function. acts on the Hubert spaces of the models by

giving rise to the (a, /?)-twisted torus partition functions for a, ß € Ffc

. (2-33)

2d

Prom this, one can easily read off, that the orbifold partition function of (2.29)

,9) (2.35) agrees with the torus partition function of the diagonal g^-WZW model

Q)- (2-36)

The fact that the orbifold group F^ acts trivially on the W-algebras of coset and toroidal models makes this representation of the WZW models useful for the study of current-current deformations. Namely, for given (f), h) the holomorphic and antiholomorphic W-algebras t) C gk and f)CflJt can be identified with the

19 d d ü(l) , ü(l) W-algebras of tAfc, and deformations corresponding to (F),r)) are then just deformations of the toroidal factor tAfc in (2.29). Thus, for a point O G .Mwzw the corresponding conformal field theory can be represented as8

flfc(O) = (öfe/6 ® toAk)/rfe . (2.37) This provides concrete isomorphisms between the. current-current deformation spaces of WZW- and toroidal models. Note however that in general the "duality" groups of the WZW models gfc and the toroidal models i\k do not agree. On the one hand, there might be dualities in the WZW models which do not preserve Afc and thus correspond to a change of the orbifold representation, and on the other hand dualities in the toroidal model need not lift to automorphisms of Ao together with S^. As noted above, for g = su(2), the duality group of the WZW model and the corresponding toroidal models coincide. In fact, the conformal field theories in .Mwzw have WZW-like sigma model descriptions, which will be discussed in Sect. 2.4.

2.4 Sigma model description of deformed WZW models 2.4.1 Classical Action To show that the deformed WZW models discussed above in fact have WZW-like sigma model descriptions, i.e. they are described by WZW-type actions, however with metrics different from the bi-invariant metrics and additional S-fields, we write down a sigma model action, which on the one hand defines orbifold models as in (2.37) and on the other hand describes WZW-like models. Let us start by describing the ingredients used to construct this sigma model. As above, we denote by G a compact semi-simple Lie group of rank d with Lie algebra g, Cartan subgroup H C G, corresponding Cartan subalgebra f)Cg and k € N. Furthermore, S is a 2-dimensional surface, bounding the three manifold B. Then, an ASYMMETRICALLY GAUGED WZW MODEL on E is described by the following action

9,B) (2.38)

where 9 X ~ IIB * ) is the WZW action with g : S —> G, (.,.) the Killing form on g, and x the three form on G associated to ([.,.],.) [54]. The integral over B in (2.39) is called WESS-ZUMINO TERM. (2.39) defines a quantum field theory if HziG) — 0 and G HS(G, 2?rZ), which we assume to hold. This WZW model is vectorially

8A realization of the torus partition function of the deformed su(2)fc-WZW models as a partition function of Zfc-orbifolds of tensor product of parafermionic models and free bosonic theories has already been given in [101].

20 coupled (see e.g. [49]) to an H-gauge connection A — (A, A) € Q1'0 © fiOil(E, fj) by

- (dgg-\Ä) - <(1 - Ad9) A,Ä)} , (2.40) and axially coupled (see e.g. [70, 57]) to an H-gauge connection B = {B,B) G

B,B)} . (2.41)

Adding both terms (2.40) and (2.41) to the WZW action (2.39), one obtains the general asymmetrically gauged model, provided we introduce the following coupling between the two gauge fields A and B which restores gauge invariance

c S Gtk(g,A,B) = ^ Jj{(l + Adg)B,Ä) - ((1 + Adg)A,B)} . (2.42)

This contains more terms than the interaction given in [6], where however a constraint relating the two gauge fields was imposed. We avoid such a constraint by adding a Lagrange multiplier

Sb,k(KB) = - / {-(dX,B) + (B,dX)}, (2.43) with A : £ —> V(27rQ(s)')> where Q(g)' is the image of Q(g) under the isomor- phism between \j* and F) provided by (.,.). This model will be coupled to an axially gauged H-WZW model, i.e. an axially gauged d-dimensional toroidal model

Sn,k,E (y, B) = ~^J ((y~ldy ~2B),E (y^dy - 2B)> , (2.44) where y : S —• H = U(l)d, and metric and B-field are parametrized by an invertible d x d-matrix with positive definite symmetric part E G Glps(d, R). . Below, it will be argued that the action

m ß SGtk(g,A,B,X,y) := S^k (g,A,B,X)+Sn,k,E(y^ ) (2-45) describes the current-current deformed gVWZW models discussed in Sect. 2.3. e In fact the vectorially gauged G-WZW model part S™™ + SG k of the action (2.45) describes the parafermionic factor in the orbifold representation (2.37) of the deformed models, while the H-part (2.44) describes the toroidal one. The axial gauging which couples these two parts in (2.45) amounts to the orbifold- construction in (2.37). To see this, we will make use of the local symmetries of the model (2.45) under vector transformations g -> hgh-1 (2.46) . A -* A + hdh'1 Ä -» Ä + hdh'1 X —> A + AC,

21 with h = exp (in) : £ —> H, and axial transformations

9 -> fgf, (2.47) £? -» B + f~ldf, B -> B + f-^f, y -* with / = exp(i77),T7 : S —» l)/(iQ(g)'). Let us first integrate out the Lagrange multiplier field A. Performing a partial integration in (2.43) yields ik f Ud{\B) + (\F(B))) (2.48) <£ B) + - [ (\,F(B)). (2.49) where J1" = dß is the curvature of B, 7$ represent the non-trivial one-cycles of E and n$ are the "winding numbers" of A around the dual cycles. Thus, the Lagrange multiplier forces B to be flat with logarithms of monodromies around 7i9

&i := jf Be (2ArQ(0))* S ±P(0). (2.50)

Now, axial gauge transformations can shift the bi by elements in ^Q(g). There- fore, the gauge equivalence classes of flat connections B satisfying (2.50) are com- pletely characterized by bi € (^fP(fl)) / (jQCß)) — Tfe, and the integration over the gauge field B reduces to summing over these b{. Note that Fk = P(&)/(kQ(g)) is nothing else than the orbifold group in the orbifold representation (2.37) of the deformed WZW models. Having integrated out A and B we end up with a product of an H-gauged G-WZW model, corresponding to the parafermionic coset model Qklh [49], and a d-dimensional toroidal model parametrized by E, which are coupled by F^-twists. These twists indeed correspond to the Ffc-action (2.32) on the Hilbert spaces of the conformal field theories gk/h®toEAk, and the sigma models (2.45) describe the deformed WZW models (2.37). The identification of parametrizations of deformation spaces is as usual in toroidal CFTs: O(d, d) acts on Glps(d, R) by fractional linear transformations, and we get 0(1) = E for O € O(d, d) parametrizing the orbifold models (2.37) and E G Glps(d, R) parametrizing the sigma models (2.45). Next, we construct the "T-dual" models by integrating out B first. Since B enters the action algebraically, this can be done by solving the equations of motion and plugging back the solution into the action. The calculation simplifies if we gauge fix y = 1. Solving the equations of motion for B yields

T 1 1 1 B = (PAdg + l + 2E )~ {Pdgg- -{l + PAdg)A-2A- dA} , (2.51) 1 l 1 B = (PAdff-i + 1 + 2E)' {Pg- dg + (l + PAd9-i) Ä + 2A~ 9A} , 9A similar construction was used in [88].

22 where P : g —> F) denotes the orthogonal projection on the Cartan subalgebra and A = exp (zA). This we plug back into the action (2.45). In the end, we will also integrate out A. Therefore, we gauge fix A = 1 already at this stage. Then we obtain

g,A) (2.52)

Next, we integrate out A by solving the classical equations of motion

T 1 A = (PAd9 - 1 - (1 + PAdfl) (PAd5 + 1 + 2E )~ (1 + PAd9))~*

1 T l 1 x {Pdgg- - (1 + PAd9) (PAds + 1 + 2E )~ Pdgg~ } , (2.53)

l 1 Ä = (PAdg-i - 1 - (1 + PAd^-i) {PAdg-i + 1 + 2E)~ (l + PAdfl-i))"

1 l l x {-Pflr- ^ + (1 + PAd5-0 (PAd^-i + 1 + 2E)~ Vg- dg} .

Plugging this back into the action and performing some algebra yields

So,t(s) = SgT + ^^tPAdj-JJ-^-'Pajj-'.P»-1»«) (2-54)

with the abbreviations

1 1 1 Sg := (l-P)-(PAdp-J?" )~ (PAd5 + JR- ) (2.56) 1 = (1 - P) + (RPAdg - P)- (i?PAd9 + P) .

Thus, we obtain the action of a WZW-like model with a deformed metric and additional B-field encoded in the choice of f) C g and of the matrix E. As expected from the comparison with the CFT considerations we recover the action of the original G-WZW model for E = 1. Note that in general deformed metric and B-field are not bi-invariant with respect to G. But they are bi-invariant with respect to H C G, which follows 1 from the identities £hg = Eg, Sgh = Ad^ 5sAd/l for all g € G, h € H. Moreover, as also expected from the CFT results, for generic E the model (2.45) only has a h © f) chiral symmetry algebra which is generated by

5g = ge- RTeg, (2.57)

23 with e, e : S —> fy. The corresponding chiral currents read J = kR-1 (1 - RRT) (PAdg - A"1)"1 Pdgg'1, (2.58) T l T T i 1 1 J = -k{R )- {l-R R){PAd9-1-(R y y P9- dg. Let us mention that the two degenerations of the model (2.45) E = Al, A —> 0, A —> oo correspond to the axially and the vectorially gauged WZW model respectively10 (c./. the discussion of limits of WZW models in Sect. 3.3.3). Thus, at the classical level, we achieved to construct a class of models connecting the axially gauged WZW model via the ungauged to the vectorially gauged one. Moreover, the response of our sigma model (2.54) to a variation of the de- formation parameters

6S = ^

= ~f^R(RTR-l)-1(SR-1)(l-RRT)-lRJ,j) (2.59) is bilinear in the conserved currents (2.58), suggesting that our family is indeed generated by current-current perturbations. So far, we have seen that the action of the deformed model looks like a WZW model action with deformed bilinear form, which is generically not bi-invariant anymore. This however is not the full story. When integrating out the gauge fields, one picks up Jacobians which usually give rise to a non-trivial dilaton. Hence, we expect that in addition to the deformed metric and B field, there will also be a non-trivial dilaton in the deformed model. By construction our model should be conformally invariant in the semiclassical limit. This means that the background should satisfy beta function conditions (see e.g. the review [96] and references therein). Checking these equations one will also observe that a non trivial dilaton (coupling with the power of fc° to the sigma model action) is needed. That would be one way to obtain the non-trivial dilaton. In the following subsection, we will use a different method to derive the expression for the dilaton. But before coming to that, let us comment on the relation of these deformed models to the families

GxH)/H 4 (5, B, y) := S^{g) + S%k{g, B) + Sn^(y, B) (2.60)

10This can be easily seen by comparing the sigma model actions. Alternatively, it can be deduced by the following observation. For E = 0 the additional U(l)d factor decouples and integrating over B yields the "T-dualized" orbifold of the vectorially gauged model, i.e. the axially gauged model. On the other hand in the limit A —» oo the gauge field B is frozen to zero and we are left with the vectorially gauged model. In both cases there is an additional decoupled U(l)rf factor whose torus is of vanishing size or decompactified, respectively. In our previous discussion this additional factor appears, because in the decoupling limits the gauge fixing conditions need to be altered, i.e in those limits one should gauge fixcoordinate s on G such that the metric on the coset does not degenerate.

24 of gauged WZW models of type (G x H)/H with varying embedding of the gauge group in the symmetry group of the G- and H-WZW models, parametrized by E G Glps(d, R). For the special case of symmetric E these models were described in [99]. Integrating out the gauge fields B in these models, one obtains11

(2.61)

_\ —l \ PAd5 + 1 + 2£

This in fact coincides with the action (2.54), which was obtained by integrating out B in the sigma model (2.45) we started with, if one relates the parameters

E = -E(E- I)"1 . (2.62)

Hence, for E such that E in (2.62) is well-defined and positive definite, the sigma model (2.45) we started with has a coset realization given by (2.60). This is the case e.g. for E G Glps(d, R) whose eigenvalues lie in (0,1). Note however that e.g. for E = 1, E in (2.62) is not well-defined and thus, the original G-WZW model does not have a proper coset realization as in (2.60). It only corresponds to a degeneration thereof. Nevertheless, for convenience, we will use the coset model realization in the following subsection to calculate the Hamiltonian of the model (2.45). Although the realization we use is only defined on part of the actual moduli space, we suppose that the results we obtain are actually valid on the whole moduli space. This is supported by the observation that they reproduce the correct results for the WZW model at E = 1.

2.4.2 The dilaton Next, we would like to derive the Hamiltonian of the coset models (2.60). For this, we choose E = R x S1 to be the cylinder with coordinates (r, a) and complex structure dT >-» da, da •-> — dT. In order to perform the Legendre transform, we return to Minkowskian worldsheet signature using coordinates x± :— r±a. Let us first discuss the ungauged G-WZW model (2.39). The conjugate momenta are given by

(2-63) where f2 denotes the contribution from the Wess-Zumino term. Since it contains exactly one r derivative, its final effect drops out in the Hamiltonian. The Hamiltonian is obtained by performing the Legendre transform

T l H = IdaTr(w g- dTg)- IdoL aiig-'d^g-^ + ig-'d^g-^g}), (2.64)

"The result can be read off from (2.51) by setting A = A = 0, E<-+E and A = 1.

25 where L stands for the Lagrangian belonging to (2.39). Introducing the currents

J+ = -kd+gg'1 , J_ = kg^d-g (2.65) we arrive at the classical Sugawara expression

J+) + (J-,J-)). (2.66)

For later use, we also give these currents expressed as phase space functions

T l J+ = 2irAdgzu - 2-n-kAdgÜ - ^dagg~ , (2.67)

J- = -2-nkwT + 2-Kkn - -g^d^g. (2.68)

In order to construct the Hamiltonian of the deformed G-WZW models we follow the prescription given in [10], where our starting point will be the coset model (2.60) before integrating out the gauge fields, but after gauge fixing y — 1, i.e.

B+,g-id-g) (2.69)

The additional terms as compared to the ungauged model modify the conjugate momenta according to

±-B+ + ±A4,B-. (2.70)

The corresponding Hamiltonian reads

T -2 ((l + Ad5 + 2JB )ß+, S-)), (2-71) where H denotes the Hamiltonian (2.66) of the ungauged model. Next, we modify the currents J±, such that the modified currents

J+ = J+ + kPAdgB+ + kB_, (2.72)

J- = J--kB+-kPAdg-iB-. (2.73) obey a gauge invariant Poisson algebra (see [10] for more details). In terms of the new currents the Hamiltonian of the deformed model is given by

2 2 2 2 +2k (B+,B+) + 2kk (B-,B-) - Ak (ß+, (l + 2E^B^. (2.74)

26 The additional constraints due to the vanishing of the conjugate momenta of B± can be used to eliminate the gauge fields by solving their algebraic equations of motion

+-B- = ~PJ+, (2.75)

_ - B+ = \?J- (2.76)

Since for E invertible12 these equations allow a unique solution for B±. Before giving this it is useful to employ (2.75) and (2.76) to simplify the expression (2.74) slightly. For the last term we write

and obtain

n = --^ Jda((J+,J+) + (JL,J_) + 2k{B+,J-) -2k(B-,J+)). (2.77)

Finally, we plug in the solutions

B+ = i(£ + £T + 2££T)1(j_-(l + 2E)j+), (2.78)

B- = ^{E + ET + 2ETE} "1 ( (l + 2^T) J- - 2 J+) . (2.79)

The result for the Hamiltonian of the deformed model is

T T H = --^^ JdalJdal /(l+(^E + E + 2E Ey^J+,J+\ (2.80)

E + ET + 2EETy1\ J-,J-

E + ET +2EETY1 (

T 2E) (E + E + 2

For symmetric E this expression agrees with the one given in [99]. Now, the zero mode part of the Hamiltonian restricted to a certain subspace of the Hubert space should "match" with the generalized Laplacian on the space of smooth functions on G [98]

A* := / f df,e-^^/d^(G)G^du , (2.81)

12The degeneration E = 0 for example describes the coset model G/H which is discussed in [10].

27 which takes into account the dilaton $, i.e. there is an isomorphism t between C°°{G) and a subspace of the Hubert space, such that tA^i"1 is equal to the zero mode part of the Hamilton operator restricted to this subspace. This can be explained (for more details see [98]) by the correspondence of the constraint

(Lo + L0-a) Iphysical) = 0 (2.82)

(LQ+LQ is the zero mode of the Hamiltonian and a is a normal ordering constant) with the mass shell condition, which in location space reads

~™2* • (2-83)

Here \? denotes the target space field associated to the physical state in (2.82). This will be used in the following to determine the dilaton in the deformed G-WZW models. The subspace of the Hubert space which should correspond to the space of functions on G consists of highest weight vectors only (see [42] for a discussion of this point), and thus the Hamiltonian (2.80) restricted to this subspace can be written completely in terms of zero-modes of left and right currents. Since zero-modes of left and right chiral currents are the generators of left- and inverse right- multiplication by G on itself, they can be identified with the respective sections JL and JR of TG ® g*. Choosing a basis of g*, one obtains from these sections the vector fields j£, j^, A € {1,... ,dim(G)} on G. In every point p£G, ({JL)P)A} {{3R)P)A are two basis of the tangent space TPG of G in p. Hence, A* can be written in terms of jf; or j^, <& and the target space metric G. G can be read off from the kinetic term of the action (2.54), such that we can compare A* with the Hamilton operator (2.80) to obtain 3>. This is the general strategy presented in [98]. But before applying it to the the models (2.45), let us illustrate it in the example of the "undeformed" G-WZW model. For notational convenience, we will use the sections ji and JR of TG 9* in the following computations and denote the dual Killing form on g* by (.,.). Now, the target space metric is 2i:k times the bi-invariant metric induced by the Killing form. The Laplace operator can then be written as

A = ^(JLJL) = -J^URJR) = 2J; (ULJL) + (3R,3R)) , (2.84) where the second equality reflects the bi-invariance of the metric. Observing that under the identification JQ ~ j£, J£ ~ 2R 1 °f zero-modes of the holomorphic and antiholomorphic currents with generators of the left and right multiplication the zero-mode part of the Hamiltonian (2.66) "matches" the Laplacian A, we deduce that the dilaton $ is constant. Now let us come to the discussion of the deformed models (2.45). The Hamil- tonian corresponding to the coset representation of these models has been cal- culated above (2.80). The target space metric can be obtained from (2.61) by

28 symmetrization13

GßV/2irk = {MjLß,jLv}

= (NjRß,JRU), (2.85) with

T T T M = (l+2E +PAdp)~ (l-P+2E +2E +4E &)

x (l+2£+Ad«riP)~\ (2.86)

T x (l+2£ +Ad,?p)~ . (2.87) Now, the generalized Laplacian can be written as 47rfcA* = {f-l3L, fM~lJL) + (rl3R, fN-'jn) , (2.88) where derivatives act on everything appearing to their right, and / = e-2*V/det(G)/Vdet(Go), (2.89) with Go denoting the "undeformed", i.e. the Killing metric on G. The inverses of M and iV are given by y T x (l + 2E + PAd9) (1-P) (2.90) T T T ^ + 2E + Adff-iP) (E + -E + 2E E) ^ (l + 2E + PAd5) ,

(2-91) T + E + 2EEF^ "' (l + 2E + PAds-i) ,

where we used the block diagonal structure of (1 - P + 2 (ET + E + 2ETE\\ and (\ - P + 2 (ET + E + 2EETX\ and the relations

13As noted before the actions (2.45) and (2.61) agree under the identification (2.62), and we will use the parametrization by E for the calculation of A*, because the Hamiltonian (2.80) was obtained in the coset representation. This however does not restrict the region of validity of the results.

29 Substituting (2.90) and (2.91) into (2.88) we obtain the generalized Laplacian. Employing furthermore the identities ( ** \ / **** • • • *~ "** m "* \ / ~ m *~ ** (TI ^* \ I "* /T^ \ -1 i^ O 771 I / T7>J. 1^ IT1 I f) IPJ T7> 1 I TTIJ I U1 1 O IP-i TJ1 1 I 1 I O ET'J 1 -I ~r ^-ti I i S-J ~~T i-i v ^-£> -L> ] — I JZ/ ~\~ i~t ~T~ ^-C/ ill I I JL —I— Zu J and AdpjL = -JR , Adg-iJR = -JL , the result can be brought into the form

(2.92)

jR

This expression matches with the Hamiltonian (2.80) provided that / is equal to a constant, which can be taken to one by performing a constant dilaton shift. Thus, we conclude that along the deformations there is a non trivial dilaton such that \/det(G)e~2* is independent of E. (2.93) This result does not come as a surprise however. Namely, deforming the kinetic term in the WZW action to the one in (2.54) while keeping the norm of the states in the Hubert space fixed leads to a Hamiltonian which represented on L2(G) (i.e. the space of ground states of the theory) takes the form

(2.94)

Comparison with (2.81) HQ = A* leads to

from which (2.93) follows. As a byproduct of this discussion we see from (2.93) that eigenfunctions of A* at a given E, which are also eigenfunctions with respect to the H-actions

30 induced by the left and right multiplication of H on G are also eigenfunctions of A* at all E, with different eigenvalues however. This is expected from the CFT considerations above, where the only effect of the deformations were changes of the {j, f) charges, and f)-, f)-highest weight states remained highest weight states under the deformations. To complete the discussion we should recall that the coset description we used here to construct the Hamiltonian (2.80) is only valid in the part of the parameter space of the model (2.45), where E is positive definite. In particular, it breaks down, when one of the eigenvalues of E becomes 1. Nevertheless, the Hamiltonian, we obtained, can be continued to the region where E has eigenvalues 1, as can be read off from

T 7 1 -1)[E + E )' {E + 1) J+, J_) ) , (2.96) and in fact for E = 1 it coincides with the one of the G-WZW model (2.66). This suggests that (2.96) is indeed the Hamiltonian on the whole parameter space of (2.45) and all the results from this section also apply to the entire moduli space.

2.5 Explicit example: su(2)k In this subsection we would like to illustrate our previous discussion very ex- plicitly in the simplest example, namely G = SU(2). We do not want to go through all the details, since much of the discussion for SU(2) (or SL(2, M))14 can be found in the literature (e.g. in [63, 58, 94]), but we will briefly describe the deformed CFT and compare it with the sigma model construction. For this, we will firstly derive the deformed sigma model by T-dualizing the model (SU(2)fc/U(l)xU(l)) /Zfc, and secondly compute the spectrum of the general- ized Laplacian. From the discussion of current-current deformed WZW models correspond- ing to arbitrary compact semi-simple Lie groups in Sect. 2.3, we know that the deformed su(2)fc-WZW models can be realized as orbifold models (compare (2-37))

(su(2)fc/ü(l) ® ü(l)^ß) /Zfc , (2.97) where R € (0, oo) parametrizes the u(l)-factor15. That the deformed su(2)fc- WZW model can be written in this way has first been suggested by Yang in [101], where a one-parameter family of modular invariant partition functions corresponding to such orbifold models with varying radius in the ü(l)-factor

14The discussion of deformation is often presented for the non compact version of Ai because in that case the interesting phenomenon of smooth topology change is observed. 15 As alluded to above, R H-> i is a duality.

31 was presented, noting that the partition function at R = 1 coincides with the partition function of the sti(2)fc-WZW model [53]. Let us start by describing the orbifold realization (2.97) of the deformed sii(2)fc-WZW model. First of all the model u(l)r of a free boson compactified on a circle of radius r has central charge c = 1 and the Hubert space decom- poses into irreducible highest weight modules VQ and VQ of holomorphic and antiholomorphic u(l) algebras with charges Q and Q:

where the charges and the conformal weights of the corresponding highest weight states \(p,w)) are given by Q(P;U)) = ^(^+ti)B), Q{PiW) = -^(%-wR), h{p,w) = hQlpw) and h(p,w) — \Q{p,w)- Thus, the partition function of the model can be written as . /„\ E » (2-99)

On the Hubert space there is a Zfc-action given by

The parafermionic models pffc := su(2)fc/u(l) with central charge c = j^^ — 1 have been classified in [53]. Here we only need the diagonal models, in which the Hilbert spaces decompose into highest weight representations of the holomorphic and antiholomorphic W-algebras as follows

%B)®VütB)l (2.101)

where Jk = {(j,n)\j G \Z, 0 < j < |, n € Z2fc, 2j + n = 0(mod2)}/~, (j,n) - (f — 3,n + A;), denotes the set of irreducible highest weight representations of the parafermionic W-algebra. The corresponding highest weight vectors \(j, n)) have conformal weights fy^re) = ^(j,rc) — (k+2) ~ Ik' ^or ^ — lnl — ^J- There is also a Zfc-action on this Hilbert space

Together with (2.100) this defines a Zfc-action on the product model sit(2)fc ® {1(1)/^-^, which is divided out to obtain the su(2)^(i?)-models. For r, s 6 Z& the (r, s)-twisted partition functions of the u(l)^Ä and the sit(2)fc theories are given by16

. (2-104)

16In the following we set (f1 = 0, V(j,m) = {0} for 21 - m

32 leading to the following partition function of the orbifold model

Thus the Hubert space of the orbifold theory is given by17

(2.106) The summand with r — 0 is the untwisted sector of the theory. In the following we will compare this with explicit sigma model analysis. We start with the (SU(2)/U(1) xU(l))/Zfc gauged sigma model (the parametrization is taken from [58] )18

S=Y Id2z Id+xd-x + tan2 xd+6d-9 + ^d+yd-y j , (2.107) where for the time being we omitted the dilaton term coupling to the Gauss- Bonnet density. Now, we redefine coordinates according to

9 = a + ß , y = a-ß (2.108) In these coordinates the relevant components of the target space metric can be written as

2 Gaa = Gßß = k (tan x + j^ J (2.109)

(2.110)

Now we T-dualize the a direction. The T-dual metric and f?-field follow from the Buscher fromulse [1.2]. We obtain

r l R2cos2x k (cos2 x + R2 sm^ x) G^ ksin2x 7; = ö , no • 2 (2.112) 2 2 Gaa COS^ X + R Sin" X 17The feictor | is due to the identification of parafermionic highest weight representation. 18In order to make contact with our general discussion in subsection 2.4.1 we note that in [58] an SU(2) group element is written as exp \i [6 — 0J 0-3/2 exp [ix

33 ^=0 (2.113)

C B*ß = ^ = -2 2 ^.2 +1 (2.114) 2 2 Gaa cos x + R sm^ x Now we define ä = k9, ß = 9 and drop the constant term 1 in the B-field. This amounts to

SK = -^ / d*z\ d+xd-x + :—^d+ed-9 (2.115) 2TT J I cos2 x + Rl sin x R2 cos2 x cos2 x COS2X cos2 x + R? sin2 x »)}• It remains to discuss the periodicity of 9. In order to obtain the deformed model 9 should be a 2?r periodic coordinate, i.e. ä should be a 2-7rfc periodic coordinate. If we perform the T-duality according to the prescription given in [88], the intermediate gauged sigma model on a worldsheet E will contain a term (compare (2.48)) YLf A> (2.116) where 7* are one cycles of E and rii are the winding numbers of the Lagrange multiplier ä around one cycles of S dual to 7*. As in the discussion around (2.48), summing over the fcZ valued windings of ä yields a Kronecker delta, which is non-vanishing if § A takes values in 2irZ/k. Since the original model is obtained by absorbing a pure gauge A± = d±p into a redefinition of the original coordinate, a parametrizes actually an orbifold 51/Zfe where S1 is the unit circle. Thus for the case G = SU(2) we explicitly obtained the deformed WZW action (2.54) from the orbifold representation (SU(2)fc/U(l) x U(l)) /Zk. Next, we would like to discuss the generalized Laplacian A* in this example. For notational simplicity we set k = 1 during the calculation and reinstall it in the end. After a coordinate change p = sinx (2.117) the metric of the deformed model takes the form

Up to a constant shift, the dilaton is given by the relation e~2 Vdet(G) = p. (2.119) Thus, we find explicitly „2# ^L (2.120)

34 which shows that eigenfunctions of the Laplace operator corresponding to the Killing metric on SU(2) which are also eigenfunctions of 8$, 8$ are in fact eigen- functions of the generalized Laplacian A* for all R19, however with different eigenvalues. For an eigenfunction of the Laplace operator in the irreducible SU(2) representation labelled by j 6 {0,..., |} with left and right U(l)-quantum numbers n and n, the difference of the eigenvalues of A* at R and R = 1 is given by = ^ (V - 1) "2 + Lj^»2 where we have reintroduced the level fc. Now, let us compare this with the CFT description (2.37). The difference of LQ + Lo-eigenvalues of a highest weight state in the r-twisted sector for R and R — 1 can be read off from (2.106) to be ^ = h (^(m ~r)2+{R2 ~l) r2)' (2-122) where we already identified the moduli spaces according to our general discus- sion. We observe that (2.121) and (2.122) agree, if we identify

n = m-r , n = r, (2.123)

and this identification is actually the expected one.

2.6 Discussion Having shown that the effect of current-current deformations of a conformal field theory on its structure is completely captured by deformations of a charge lattice, we obtained a description of the subspaces of CFT moduli spaces correspond- ing to these deformations as moduli spaces of certain lattices with additional structure. This generalizes the case of deformations of toroidal conformal field theories [23]. The general considerations were applied to WZW models, where they were compared with a realization of the deformed models as orbifolds of products of coset models with varying toroidal models. This realization was well suited for the construction of sigma models corresponding to the deformed WZW models. For this purpose we employed axial-vector duality to transform the orbifold of the (G/H x H)-sigma model into a WZW-like model with (in general) non-bi- invariant metric, additional B-field and non-trivial dilaton. This provides a very explicit description of the sigma models associated to deformed WZW models. It would be interesting to investigate further the geometry of metric and 5-field we obtained for the deformed models. Since the sigma models correspond to conformal field theories, they should for example satisfy some nice differential equations, namely the beta-function equations (see [96] and references therein):

19Note that at R = 1 A* = A as discussed in the previous section.

35 Apart from the general CFT considerations, we focused the discussion on the example of WZW models associated to compact, semi-simple Lie groups. There are however other interesting conformal field theories admitting current-current deformations, which deserve an analysis of their moduli spaces. These are for example WZW models corresponding to non-compact Lie-groups (see e.g. [5, 36, 4, 77]), which could provide time dependent exact string backgrounds and thus might give hints about how string theory deals with cosmological singularities (see e.g. [74, 31, 32] for a discussion of this point). But also an investigation- of moduli spaces of e.g. coset models, and in particular Kazama-Suzuki-models [69] should be of interest, because the latter would provide examples of explicitly known moduli spaces of N = 2 super confer mal field theories. A discussion of the relation between mirror symmetry and gauge symmetry in this setting has been presented in [59]. The analysis of the "behavior" of D-branes (i.e. conformal boundary condi- tions) on moduli spaces of conformal field theories is in fact a very important sub- ject in string theory. As our considerations show, current-current deformations are in fact easily tractable, and hence provide a good setup to study structural questions concerning "bulk-deformations" of boundary conformal field theories. Some semi-classical aspects of D-branes in deformed su(2)fc-WZW models were presented in [38, 37], but the general conformal field theory analysis of boundary conditions in deformed WZW models is an interesting open problem. In particu- lar, an investigation of D-branes in deformed Kazama-Suzuki models could lead to a better understanding of D-branes in moduli spaces N = 2 superconformal field theories.

36 37 3 Limits and degenerations of CFTs

In this section, techniques are developed to analyze limits and degenerations of conformal field theories, occurring e.g. at the boundaries of CFT moduli spaces. Notions of SEQUENCE OF CONFORMAL FIELD THEORIES and CONVERGENCE of such sequences are introduced. To a convergent sequence of CFTs, a LIMIT can be associated which in general is not a well-defined conformal field theory but a degeneration thereof. It possesses a pre-Hilbert space H°° carrying two commuting actions of the Virasoro algebra, and as in CFTs, to each state in "H00 can be associated a tower of modes. Under slightly stronger conditions, which are fulfilled in all examples, it even has the structure of a conformal field theory on the sphere. This notion of convergence (also the stronger one) is compatible with de- formation theory. Namely a sequence of points in a moduli space of conformal field theories, which converges in this space gives rise to a sequence of conformal field theories converging in the sense which will be defined below to the CFT specified by the limit point, i.e. in this case, the limit structure is indeed a full CFT. In general however, degeneration phenomena will occur in the limiting process, which lead_ to infinite degeneracies of certain subspaces of the Hubert space. In particular correlation functions on higher genus surfaces may diverge in the limit. These degenerations however provide new interesting structures. Namely, it turns out that the states whose conformal dimensions vanish in the limit generate a commutative *-algebra .4°°, which can be regarded as function algebra on a "target space" M. Moreover, the degenerating conformal dimensions can be used to equip the "target space" with a degenerating metric and an additional smooth function, the dilaton. Furthermore, A°° acts on the pre-Hilbert space "H°° associated to the limit, which can thus be interpreted as the space of sections of a sheaf of vector spaces on M. It even seems that the limit CFT structures are .A00-homogeneous, such that they can be localized to corresponding structures on the fibers. Thus, to a degenerate limit of conformal field theories can be associated the structure of a sheaf on M of conformal field theories defined on the sphere.. The fiber vector spaces in turn do not show any degenerations. Structures of this kind have actually already been conjectured in [72], where they were used to motivate a version of mirror symmetry which only relies on the limits of certain CFT moduli spaces. Having set up the notions of convergence of sequences of CFTs and deriv- ing the desired properties of the limit structures, some classes of examples are studied in detail. In the case of toroidal conformal field theories, degenerations give rise to trivial fibrations of torus models with smaller dimensions over de- generating subtori. Similarly orbifolds of toroidal CFTs can be analyzed. In this case we again find the respective torus orbifolds as degenerating "target space" geometries. However, the fiber structure of the limit CFT is more interesting. Namely, the twisted sectors contribute sections of skyscraper sheaves over the fixed points of the orbifold action, which gives a nice geometric interpretation to the twisted sectors. Furthermore, degenerations at the boundaries of current-

38 current deformation spaces, which were constructed in Sect. 2 are studied in the special case of WZW models. In this case degenerations give rise to fibrations of certain coset-models over degenerating tori. Moreover, also a somewhat more involved example is studied, namely the A-series of unitary Virasoro minimal models, which in contrast to the examples mentioned before is a discrete family of CFTs with varying central charge. This makes the construction of the sequence, the verification of convergence and the analysis of the limit structures more difficult. As is expected from gauged- WZW model considerations, we obtain a degenerating interval as "target space" geometry with a non-trivial dilaton. In fact, the construction of the degeneration algebra A°° can be motivated by sigma-model considerations. In large-volume sigma models, one expects the algebra of low-energy observables to be isomorphic to a non-commutative de- formation of the algebra of smooth functions on the target space, which should become commutative in the limit of infinite volume. This can be viewed as a classical limit of "quantum geometries" associated to the respective conformal field theories. In [42] a method was proposed how to extract non-commutative geometries out of CFTs. In fact, the algebra A°° can be regarded as the limit of certain subalgebras of these non-commutative geometries. This, on the one hand confirms that the construction of our limit structures is natural. On the other hand, it gives the possibility to identify "non-commutative geometric structures" in CFTs. These could be used to carry over the powerful geometric tools appli- cable to the study of sigma models in large volume limits to regions inside the CFT moduli spaces. This suggests that non-commutative geometry in terms of Connes' spectral triples [19, 20, 21] seems to be a valuable tool in the study of degenerations of conformal field theories. This chapter is organized as follows: In the first Sect. 3.1 we explain how non-commutative geometries can be extracted from CFTs, after giving a brief overview of some of the basic concepts. Sect. 3.2 contains our definitions of sequences, convergence, and limits, and is the technical heart of this part of the work. Moreover, the geometric interpretations of degenerate limits are dis- cussed. Sect. 3.3 is devoted to the study of torus models, orbifolds thereof, and degenerations of current-current deformed WZW models, where we exemplify our techniques. In Sect. 3.4 we present our results on the A-series of unitary Virasoro minimal models. We end with a discussion in Sect. 3.5. Several appen- dices contain background material and lengthy calculations.

3.1 From geometry to CFT, and back to geometry String theory establishes a natural map which associates CFTs to certain, some- times degenerate geometries. Conversely, one can associate a GEOMETRIC IN- TERPRETATION to certain CFTs, and the latter construction is made precise by using Connes' definition of spectral triples and non-commutative geometry. In Sect. 3.1.1 we very briefly remind the reader of SPECTRAL TRIPLES, ex- plaining how they encode geometric data. Somewhat relaxing the conditions on spectral triples we define SPECTRAL PRE-TRIPLES which will be used in Sect.

39 3.1.2. There, we recall the basic structure of CFTs and show how to extract spectral pre-triples from them. If the spectral pre-triple defines a spectral triple, then this will generate a non-commutative geometry from a given CFT. In Sect. 3.1.3 we explain how in favorable cases we can generate commutative geometries from CFTs. In the context of string theory, this prescription gives back the original geometric data of the compactification space. Much of this Sect. 3.1 consists of a summary of known results [20, 42, 21, 87, 72], but it also serves to introduce our notations.

3.1.1 From Riemannian geometry to spectral triples For a compact Riemannian manifold (M,g), which for simplicity we assume to be smooth and connected, the spectrum of the associated Laplace-Beltrami operator Ag:C°°(M) —> C°°(M) encodes certain geometric data of (M,g). However, in general one cannot hear the shape of a drum, and more information than the set of eigenvalues of Ag is needed in order to recover (M, g). By the Gel'fand-Naimark theorem, the point set topology of M is completely encoded in C°(M) = C°°(M): We can recover each point p G M from the of functions which vanish at p. In other words, given the structure of C°°(M) as a C*-algebra and its completion C°(M), M is homeomorphic to the set of closed points of Spec(ÖM), where OM is the sheaf of regular functions on M. Connes' dual prescription uses C*-algebra homomorphisms x: C°°(M) —• C, instead, such that pgM corresponds to Xp: C°°(M) —> C with xp(f) := f(p)'> the Gel'fand-Naimark theorem ensures that for every commutative C*-algebra A there exists a Hausdorff space M with A = C°(M). M is compact if A is unital. Example 1.1 + 1 Let /JeR , then M = §R = R / ~ with coordinate x ~ x + 2TTR has the Laplacian A = — J^. Its eigenfunctions \m)R,m € Z, obey

Z: \m)R: x -> e ; \*\m)R &\m)R; Vm,m' eZ: \m)R • \m')R = |m + m')ß, and they form a basis of C°(M) and C°°{M) with respect to the appropriate norms. Any smooth manifold is homeomorphic to §R, equipped with the Zariski topology, if its algebra of continuous functions has a basis fm, m G Z, which obeys the multiplication law fm • fm> = fm+m>. To recover the Riemannian metric g on M as well, we consider the SPECTRAL 2 TRIPLE (H :=L (M,dvolg),iI := ^A9,^:=C°°(M)), where H is viewed as self-adjoint operator which is densely defined on the Hubert space HI, and A is interpreted as algebra of bounded operators which act on elements of H by pointwise multiplication. Following [20, 42, 21], we can define a distance func- tional dg on the topological space M by considering 2 2 T:={feA I Gf:=[f,[H,f]] = -(f oH + Hof )+2foHof obeys \/heC°°{M): \Gfh\<\h\}.

40 One now sets Vx,yeM: dg{x,y):=swp\f{x)-f{y)\. (3.2)

l 2 In Ex. 1.1 with M = § R one checks that for all f,h £ C°°{M):Gfh = (f') h, and in general Gfh = g(Vf,Vf)h. In fact, by definition [8, Prop. 2.3], any second-order differential operator O satisfying [/, [|O, /]] =

V/ € A : V/ := [P, /]: H' -> HI'; V/i € A : [V/, h] = 0, (3.3) where in the above examples V/ acts on HI' by Clifford multiplication, and that A gives smooth coordinates on an "orientable geometry"; furthermore, there are fmiteness and reality conditions as well as a type of Poincare duality on the K-groups of A. If all these assumptions hold, then by (3.2) the triple (HI', V, A) defines a non-commutative geometry ä la Connes [19, 20, 21]. If the algebra A is commutative, then the triple {W,V, A) in fact defines a unique ordinary Riemannian geometry (M,g) [21, p. 162]. The claim that the differentiable and the spin structure of (M, g) can be fully recovered is detailed in21 [87]. Following [42], instead of studying SPECTRAL TRIPLES (E.',V,A), we will be less ambitious and mainly focus on triples (H, H, A), somewhat relaxing the defining conditions: Definition 1.2 We call (H, H, A) a SPECTRAL PRE-TRIPLE if H is a pre-Hilbert space over C, H is a self-adjoint positive semi-deßnite operator on M with Hop '•= ker(if) = C, and A is an algebra of operators acting on H. Since ?io,o - C 3 1, we can map A —>mbyAi-*A-l.

20In local coordinates a generalized Laplacian can thus be written as in (3.6) below. 21We thank Diarmuid Crowley for bringing this paper to our attention.

41 If additionally the eigenvalues of H have the appropriate growth behavior, i.e. for some 7 G R and V eR:

N(E) := dime 0 W € H | Hip = \

. V /, h E A: (V/, V^EndH' = 2{/, Hh)u (3.5) and such that (H', V, A) obeys the seven axioms of non-commutative geometry, then we call (H, H, A) a SPECTRAL TRIPLE or a NON-COMMUTATIVE GEOMETRY OF DIMENSION 7.

Remark 1.3 Note that in the geometric setting our condition (3.5) for the operator H does 2 not imply H — \ As on L (M, dvols). In fact, H will in general be a generalized Laplacian with respect to a metric 'g = (gy) in the conformal class of g. More 2 1 precisely, we will have dvol5 = e~ *dvolö with $ G C°°(M), and with 'g~ =

2H = -e^x/detgr1^ ^e"2*Vciet|^dj (3.6) with respect to local coordinates, in accord with (3.5). We call g the DILATON CORRECTED METRIC with DILATON $. Note that

42 3.1.2 Spectral triples from CFTs We do not attempt to give a complete definition of CFTs in this section; the in- terested reader may consult, e.g. , [7, 80, 56, 78, 40, 46]. Some further properties of CFTs that are needed in the main text are collected in App. A. A UNITARY TWO-DIMENSIONAL CONFORMAL FIELD THEORY (CFT) is spec- ified by the following data: • a C-vector space H of STATES with scalar product (-|-). This scalar product is positive definite, since we restrict our discussion to unitary CFTs; • an anti-C-linear involution * on 7i, often called CHARGE CONJUGATION;

• an action of two commuting copies Virc, Virc of a Virasoro algebra (A.I) 22 23 with central charge c € R on W, with generators Ln, Ln, n 6 Z, which commutes with *. The Virasoro generators LQ and LQ are diagonalizable on 7i, such that H. decomposes into eigenspaces24

«fc,*. (3-7)

h-heZ

and we set Tih ^ := {0} if h — h $ Z. The decomposition (3.7) is orthogonal with respect to (-|-);

+ a GROWTH CONDITION for the eigenvalues H, h in (3.7): For some V G K :

+ E V£GE : OO > dim I 0 HhJi I ~°° exp (vVE^j . (3.8) \(h+h)

a unique *-invariant VACUUM Q, G Wo,o — C, as well as a dual Cl* G H* characterized by (A.2); a map C : H* ® H®2 —> C that encodes the COEFFICIENTS OF THE OPERATOR PRODUCT EXPANSION (OPE), Such that

(3-9) i.e. the induced map is the canonical pairing. The OPE-coefficients C obey (A.10) and (A.12) and can be used to define an isomorphism

!J ZZ J s. th. VXGW: 4>*(x) = C(r,n,x) = Wx)- (3.10)

22 As a matter of convenience, we always assume left and right handed central charges to agree. 23 The indexing of all modes below corresponds to energy, not to its negative. 24 In this work, we restrict our investigations to bosonic CFTs.

43 There are many properties of the map C, like the sewing relations, that have to be fulfilled for reasons of consistency, and which we will not indulge to list explicitly. Some properties of CFTs that follow from these consistency conditions should be kept in mind, however:

• ip G 7i is a lowest weight vector (lwv) with respect to the action of Virc, 25 V~Irc, i.e. a PRIMARY STATE, iff for all n € N- {0}: L-n(p = 0, ~L-n(p = 0.

For any Z-graded algebra C = ® Cn we define nSZ £ := 0£n, (3.11) ±n>0 c • H := ker£~ = {

to associate to each ip G H a tower

ular, the elements Ln, Ln, n G Z, of Virc, Virc can be interpreted as the Fourier modes of the holomorphic and antiholomorphic parts T, T of the ENERGY-MOMENTUM TENSOR. Moreover, Ctofi acts as identity on H, and all other modes of Cl act by multiplication with zero. By abuse of notation

we write T = L2ti G 7^2,0, T - ^2^ € Ho,2 for the VlRASORO STATES in H. A sextuple C = (7i, *, Cl, T, T, C) with H, *, O, T, T, C as above specifies a CFT. Two CFTs C = (H, *, SI, T, T, C) and C = (W, *', Q', T\ f, C) are EQUIVALENT, if there exists a vector space homomorphism / : V. —> W, such that I: (ft, r, T) ^ (ft', T', 7^) and *' = / o *, C = C o (/* ® J ® 7). Instead of primary states in 7^Vir, below, we will be interested in primary states with respect to a larger algebra than Vir, namely the (generic) HOLOMOR- PHIC AND ANTIHOLOMORPHIC W-ALGEBRA W*®W*', see (A.15). By (3.11) the primary states with respect to a subalgebra W of W* © W are W U - ker W" = {^ € H | Vn G N - {0}, Vw G W_n: w<^> = 0} . To TRUNCATE THE OPE TO PRIMARIES note that by (3.8) for given

w W := {

44 Let us remark that the above definition of 11 may well be too restrictive: By in- troducing appropriate (partial) completions of the relevant vector spaces one can attempt to replace our finiteness condition in (3.12) by a condition on normal- izability and thereby get rid of the restriction to Ü . Although in most of our examples we find Hw = Hw, for the orbifolds discussed in Sect. 3.3.2, Hw/Hw consists of all twisted ground states. The latter do not enter into the discussion of the zero mode algebra, which is relevant for finding geometric interpretations (see Sect. 3.2.2). Summarizing, our definition of 11, above, is well adapted to our purposes, though it may be too restrictive in general. By construction,

Let us extract a spectral pre-triple from a CFT C = (H, *, ti,T,T, C). By definition of the adjoint (see (A.5), (A.ll)), LQ acts as self-adjoint operator on H, and Li = L_i. Moreover, 2LQ = [LJ,Li] shows that LQ is positive semi- definite, and similarly for LQ. Therefore, to associate a spectral pre-triple to a CFT C, we will always use H := LQ + Lo, which by the uniqueness of Q, obeys ker(ff) = HOto = C. Following [42], we let

M:=HW = kerW" denote the space of primaries in "H with respect to an appropriate subalgebra W of the holomorphic and antiholomorphic W-algebras. Moreover, to every

AV:B. (3.13)

It is not hard to see that (H, H, A) obeys Def. 1.2 thus defining a spectral pre-triple. As a word of caution, we remark that in general for

Several other attempts to associate an algebra to a CFT can be found in the literature. Truncation of the OPE to leading terms, as suggested in [72, 2.2], gives a straight-forward algebra structure but seems not to capture enough of the algebraic information encoded in the OPE: On the one hand, if all states in "Hw are given by simple currents, e.g. for the toroidal theories focused on in [72], then truncation of the OPE to leading terms is equivalent to our truncation (3.12). On the other hand, for the example that we present in Sect. 3.4, it is not, and we show how our truncation (3.12) gives a convincing geometric interpretation. For holomorphic vertex operator algebras, ZHU'S COMMUTATIVE ALGEBRA is a commutative associative algebra which can be constructed using the normal ordered product by modding out by its associator (see [104, 11, 47]), and it is isomorphic to the zero-mode algebra [11]. Although to our knowledge Zhu's commutative algebra has not been generalized to the non-holomorphic case, it is very likely that such a generalization would yield the same geometric interpretations for degenerate CFTs that we propose below; this is related to

45 the fact that Avo Ax = Atpmx holds for the relevant states in these degenerate CFTs, see Lemma 2.10 and Prop. 2.11. Summarizing, our truncation (3.12), which goes back to [42], seems to unite the useful aspects of both the truncation of the OPE to leading terms and Zhu's algebra. The growth behavior of the dimensions of the eigenspaces of H on HI and therefore also the dimension 7 of the spectral pre-triple extracted from a CFT as described above certainly depends on the choice of the sub-W-algebra W. Thus, it is not possible to give a general formula for 7. In some examples with integral central charge c of the CFT, we find 7 = 2c as the dimension of the spectral pre-triple, see e.g. Ex. 1.5 below. So far, we have shown: Proposition 1.4 To any CFT C = (H, *, Ü, T, T, C) of central charge c, after the choice of a subalgebra W of the holomorphic and antiholomorphic W-algebras, we associate a triple

W = kerVW", H := LQ + Lo, A := {A^ \

Then (H, H, A) is a spectral pre-triple. The operator V := L\ + L\: M —> H obeys (3.5) asjwell as a Leibniz rule. However, for general CFTs we are unable to show that (H, H, A) gives a spectral triple of a specific dimension, i.e. a non-commutative geometry according to Def. 1.2. A need not, in general, act by bounded operators, and we are unable to check all seven axioms of Connes' or their reduction in [75], including the fact that A is a C*-algebra. Neither are we aware of any attempt to do so in the literature, see also [43] for a discussion of some unsolved problems that this approach poses. For toroidal CFTs, the above construction indeed gives a C*-algebra A of bounded operators [42]. We illustrate this by Example 1.5 Let CR,R 6 M+, denote the CIRCLE THEORY AT RADIUS R, i.e. the CFT with central charge c = 1 that describes a boson compactified on a circle26 of radius R. All CR possess a subalgebra. W = u(l) © u(l) of the holomorphic and an- tiholomorphic W-algebra27 (see App. B), and the pre-Hilbert space HR of CR decomposes into irreducible representations of W. The latter can be labeled by left- and right handed dimension and charge IIR, QR and JIR, QR of their lwvs, 2 where h,R = \Q R, KR = \QR. The space of primaries of CR with respect to W is

: QR = ^ (f + nR) , QR = -± (f - nR)} ,

26 Our normalizations are such that the boson compactified on a circle of radius R = 1 is described by the su(2)i WZW model. 27To clear notations, our symbol g always denotes the loop algebra associated to the Lie group G with Lie algebra g, and Qk denotes its central extension at level k.

46 see (B.4). To obtain the spectral pre-triple associated to CR by Prop. 1.4 from § := Hw we need to consider the truncated OPE (3.12). By (3.13) and (B.6), orthonormalizing the \QR; QR) as in (B.3), we have

We see that Hw = Hw and A := {A^ \

r = { (QR; QR) = (Qm,n,Qm,n) = 75 ((g + nR); (f - nR))| m,n G z} (3.15) (see (B.4)), twisted by the two-cocycle e of (B.6), yielding a non-commutative generalization of the algebra of smooth functions on §}j x S\,R. Moreover, one checks that (H, if, A) is a spectral pre-triple of dimension 2 = 2c, and we have

QR = -^(^-nR) (3.16)

in perfect agreement with (3.1).

3.1.3 Commutative (sub)-geometries By Prop. 1.4, there is a spectral pre-triple associated to every CFT. However, this construction is not very satisfactory. Namely, it depends on the choice of a W-subalgebra W, and it does not allow us to extract a non-commutative geometry ä la Connes in a straight-forward manner. Moreover, if we start e.g. with the one-dimensional Riemannian geometry (§}j,<7) discussed in Ex. 1.1, from its associated CFT we read off a spectral pre-triple (H, H, A) of di- mension 2 as discussed in Ex. 1.5. The original one-dimensional spectral pre- 2 triple (H = L (SR,dvolg),H = \&g,A = C°°(ßR)) can of course be obtained from (H, iJ, A) by restriction:

HI = spanc {|"I)Ä \rn €Z}

£ spanc {\QR;QR) € H | QR = QR = ^,m e z} = ker(Vtr,j0 - Jo>» where jo, Jo denote the zero modes of generators j,j of u(l), u(l) as in (B.I). In (3.16) we have checked that H has the correct eigenvalues on the generators of

H. Also, by (3.14), II is associative and commutative on H = ker(W~, jo — j0), and A = (Av \

47 Definition 1.6 Let C denote a CFT with central charge c, W a subalgebra of its holomor- phic and antiholomorphic W-algebras, and (H = keiW~,H, A) the associ- ated spectral pre-triple of dimension 7 as in Prop. 1.4. A spectral pre-triple (M,H,^A) of dimension c is called a GEOMETRIC INTERPRETATION OF C if H C M, A = (ApliH I ^ 6 H) is commutative, and if there are appropriate completions H, AofW, A such that (H, H, A) is a spectral triple of dimension c, 2 i.e. M — L (M,dvo\g), H — gAj, A = C°°(M) for some Riemannian manifold (M,g) of dimension c and dvol^ = e~2*dvolj, 0, e

Ao := IH I

0 as in Def. 1.7 are studied as e —> 0, where the preferred geometric in- terpretations (ME,g£), e > 0, all yield the same topological manifold M£ = M. Then (M,g£)£-+o is believed to describe a Gromov-Hausdorff limit of a metric on M, where some cycles collapse while keeping the curvature bounded. Such limits of metrics have been studied in [17, 18]. In the physics literature, the limiting geometries which arise from degenerate CFTs are sometimes referred to as LARGE VOLUME LIMITS, see [81] for a useful account.

48 Since each collapse of cycles (M, ge)s->o in [17, 18] gives a boundary point of the moduli space of Riemannian metrics on M, it is natural to use sequences (Ce)e_>o as above to construct corresponding boundary points of moduli spaces of CFTs. In a more general context, such a possibility was alluded to in [72]. It presumes the definition of topological data on the families of CFTs under consideration: Definition 1.8 A CFT-SPACE is given by the following data: A sheaf S over a topological Hausdorff space M, such that for each p € M, Cp is a CFT with associated pre-Hilbert space 7ip = Sp. Furthermore tt,T,T are global sections ofS, and all CFT-structures as e.g. OPE-coefficients, evaluated on local sections ofS, are continuous. If M. is a D-dimensional variety, then D is called the DIMENSION of the CFT-space S. If

M giving r rise to one-dimensional CFT-subspaces oo). If for i —> oo the CFT-structures of the Cp^ converge in a suitable sense, e.g. as specified in Sect. 3.2, then the limit structure gives rise to a boundary point of the CFT-space «S|p. If Iimt_toop(i) = p 6 M, then the CFT-structures converge to the corresponding structures of Cp, and the boundary point of the CFT-subspace «S|p just corresponds to this CFT. If however p € M — M, then the boundary point of the CFT-subfamily oo, then we obtain a limiting spectral pre-triple (M°°, H, A°°). The above assumption that all eigenvalues of H on Hp(t) converge with the same speed O(t~N) allows to define H°° := limt-H» tNH and should allow to read off a non-degenerate Riemannian geometry from (H°°, H00, A°°). For now, instead of considering CFTs, let us stay in the regime of function spaces and inspect limits of commutative geometries in terms of spectral triples. This serves as a motivation for Sect. 3.2 and also leads to some ambiguities which should be kept in mind. Example 1.9 We consider possible limiting procedures for the spectral triples (HR = L2(S^), H = 1&,AR = C°°(S^)) as R -> oo. By (3.1), each MR is generated by the space ©mezV^ with V^ := spanc{|m)#} an eigenspace of H with eigenvalue jgs. It is therefore natural to choose constant sections $ = {ipm | m € Z} of the

49 sheaf

with lm>°° := {lm>Ä I R

By (3.1), cpm • ipm' = ipm+m' for all m, m' G Z, so we are lead to set An|m'}oo := Im + m^oo and thus obtain a commutative algebra of bounded operators A??\ :=

(Am | m € Z) on ^m- The H-eigenvalues of all \rn)R converge to zero with the same speed as R —» oo, hence we can naturally define H9^Am)^ := ^{m}^ to obtain the commutative geometry (H^ S L2(S\), Hfö, A^ = C°°(Sj)) in the limit. Mathematically, having |m}oo represent the sequence {|m}# | R 6 R+} means that spanc {|ra)oo} is the DIRECT LIMIT (see, e.g. [27]) of the {V£, R e K+}, + where for R, R' G R , we use /R,R': SJJ/ —> SJJ with fRtR'{x) := x--^ to construct a DIRECT SYSTEM (MR, fRR,). Then, H^j is the DIRECT LIMIT of (MR,fRRI). We have used the category I\ with objects Ob (7i) = R+ the circles of radii R € R+ and morphisms the diffeomorphisms /R,R' defined above. Note that in /i there is precisely one isometry /R^RI for every pair of circles28 (§^,,S^). The limit (WfiyHfö, Afö) is the inductive limit of the functor Fi: h -> Vect which on objects maps SR i—> C°°(SJJ), and on morphisms maps /H,H' •"*• ffiR'- Instead of I\, there is another quite obvious category I2 we could have chosen, + namely with objects Ob(/2) = Ob(/i) = R+ the circles of radii i?el and morphisms the isogenies (i.e. local isometries) between circles. That is, there exists a morphism QR,RI: SR, —> §R with gRtR>(x) := x precisely if ^ G N. The inductive limit of the functor F2: I2 —* Vect which on objects maps §R 1—> C°°(S)j), and on morphisms maps gRtR' H-> g*RRi is

{\Q • 0)oo} e 0 spanc

with \fg € R/Q: |ß« 0)«, := {|0>yve I ^ e 2},

Vr € M*: Ir)«, := {|n)n/r | n € 2}. Here, M/Q denotes classes of real numbers which are commensurable over Q. ixr We have \g • 0}^ = 1 for all g 6 R/Q, and for all n G Z - {0}: |n)n/r: x H-> e . Hence we naturally define H9Z\g»0)oo := 0 for g G R/Q, and H^r)^ := ^|r)oo for r G R. This again yields a degenerate limit, but we cannot rescale H?£. as before. Namely, to interpret the |r-)oG in terms of sections-

28We use oriented circles with base points to get rid of the translations and reflections.

50 on K+. Then we can also naturally define a spectral triple (W%y H?Z, A^), with AT E A<$y r E R, acting by Ay)^ = \r + r')oo, AV • 0>«» = |r)oo iff r and r' are commensurable over Q, i.e. r = r' in R/Q, and Ay)^ = 0, J[4r|r'»0}00 = 0, otherwise. Similarly, for Q E R/Q we have AB,Q 6 ^4^ acting by Vok')oo = |r')oo, ^ok'-O)«, = \r' «0)00 iff ß = r' in R/Q and ^ok')« = 0, Ae,o\r' • 0)oo = 0, otherwise. In other words, Ae,Q acts as a projection, and {Ae»o I £ G R/Q} defines a "partition of identity", Ao := Z)ee!R/Q-^e»o- This indeed gives a commutative geometry, namely R with the flat metric and an interesting topology. Summarizing, Ex. 1.9 motivates the use of direct limits for the construction of limits of spectral pre-triples and CFTs. Moreover, as a word of caution, we have 2 found two different limiting geometries for the spectral triples (MR = L (SR), 1 H = ^A,AR — C°°(S R)) as R —»'00, depending on the choice of the constant sections of ) corresponds to a decompactification of Sjj as R —* 00 equipped with a discrete topology. Similarly, the definition of limits for CFTs that we propose in Sect. 3.2 will incorporate some ambiguity. Remark 1.10 We do not claim that direct limits yield the only sensible construction for limits of algebras or spectral triples as in Ex. 1.9. There, we have already performed a generalization from direct limits of ordered systems to direct limits of merely partially ordered systems. However, an ordered set (A%, •%, (., -)i)iel of algebras with non-degenerate bilinear forms need not be a direct system at all in order to make sense of its "limit". Since we mainly focus on the more natural direct limit construction, below, we do not give a formal definition of the more general one, here. The main idea, however, is to regard a vector space A as limit of the ordered set (A)ie/ if for every i E I there is an epimorphism /j : A —»• Ai, such that for each tp E A— {0} there exists an N G / with fi( N. If the respective limits, below, exist, then we can equip A with a limit bilinear form and algebra structure by setting

<¥>, X) ~ lim(/i(), fi{x))i, (il>,

Note that this only defines an algebra structure on A if (•, •) is non-degenerate. As an example let us discuss the limit of the algebras C°°(S}j) of Ex. 1.9, equipped with the Hermitean form L The radii R E R+ of the circles S)j constitute the ordered index set /. As limit space A we choose the space C£°(R) of compactly supported smooth functions

51 on R. Then, we define

/Ä:CC°°

which is a discrete version of a Fourier transform. Indeed, (C' fulfills all the conditions mentioned above, and the limit algebra structure on A = C£°(R), corresponding to the ordinary product of the Fourier transformed functions, is the convolution product

=

3.2 Limits of conformal field theories: Definitions As explained above, our construction is motivated by the ideas of [42, 72]. The guiding example is that of the circle theories discussed in Exs. 1.1, 3.8, 1.9, or more generally the toroidal CFTs discussed in Sect. 3.3.1, since these models as well as their large volume limits are well understood. Further motivation arises from the observation that the family of unitary Virasoro minimal models M(m, m + 1), m € N — {0,1}, can be treated by our techniques, too, as detailed in Sect. 3.4. Sect. 3.2.1 is devoted to the definition of sequences of CFTs and their limits; we propose a list of conditions which ensure that the limit possesses enough structure in order to realize some of the ideas of [42, 72]. In Sect. 3.2.2 we explain how our limits can give rise to geometric interpretations.

3.2.1 Sequences of CFTs and their limits In Ex. 1.9 we have given a motivation for our general approach to limiting processes for CFTs, which uses direct systems and direct limits29. We recall the basic definitions below but refer the reader to the literature for a more detailed exposition, see e.g. [27]. We start by defining sequences of CFTs: Definition 2.1 Let (C^jgN = {W, *\ Q,\ T\ T\ C^jgpj denote a family of CFTs with left and right central charges Ci. Given vector space homomorphisms // such that

l V», = PJ, * < 3 •• // :H 1 and (3.17) fi (rti) = a?, 1 { fl = ft (T ;) = :P, axid Vi, be:N,i

52 we call (C*,//) a SEQUENCE OF CONFORMAL FIELD THEORIES. Note that we do not demand any further CFT-structure to be preserved by the morphisms f?, which therefore are not morphisms of CFTs. Hence a sequence of CFTs cannot be regarded as a direct system of CFTs. However, (3.17) by definition gives a direct system of vector spaces (Hl,/f). It allows us to define a direct limit vector space [27]

k :=\imH = ©« spanc {^ - //V) | i, j € N, i <

where by abuse of notation for i € N we have omitted the inclusion homomor- phisms tl : Ti} <—* (BfceN^- "^-^ aDOve definition of /C°° means that for each ip € /C°° there exist k G N and ipk 6 7ik such that ip is represented by k. In the following,

ViGN: /?°: H* ^ we denote the homomorphisms given by the composition of inclusion and pro- jection, with f?° o f? = /P° for «, j € N, i < j. With the above notations,

Similarly, for t, j € N, i < j and ^ € W we define (//)*(^*) := Ul{i>)Y- This gives a direct system ((W*)*, (//)*) • Its direct limit is denoted (K.*)°°, and we have projections (/*)°° = (/f°)* as above. By (3.17), the limits /C°° and (K.*)°° possess special elements Cl, T, T and fl*, and an involution *. However, the definition of CFT-like structures on the limit vector space /C°° requires some more conditions on a sequence of CFTs, which we shall discuss now. In particular, we need a notion of convergence. In the following, let {Cz,fD denote a sequence of CFTs. Condition 1 The OPE-coefRcients C* ofC{ CONVERGE WITH RESPECT TO THE //, i.e.

The limits C of the OPE-coefficients only depend on elements of the direct limits K.°°, {JC*)°° and are trilinear. Thus a sequence of CFTs (C\/f) fulfilling Cond. 1 gives rise to a trilinear function C°° : (/C°°)* ® /C°° ® /C°° —• C. C\ *\ and the map W -> (W)*, i> "-> ip* with (3.9), (3.10) determine the Hermitean structure of Ti}. Since the homomorphisms // are compatible with this structure, if Cond. 1 holds, then the vector space IC°° inherits a limiting

53 bilinear form {-|-}oo = C°°(-*,Ct,-), which may be degenerate, though. Define M°° C /C°° to be the space of NULL VECTORS of (•I-)«, in /C°°, i.e.

'Moo:={veJC*>\Coo{v;n,v) = 0}. (3.18)

Since the Cauchy-Schwarz inequality is valid for all {-\-}i = C%(-*,0,%, •), Cond. 1 implies that C°°(-*,fi, •) defines a non-degenerate bilinear form on

nco ._ ^oo/^oo with ^oo . ^-oo _^ ^oo the projection. (3.19)

In the following, we will frequently use elements ip € /C°° to represent a class in 7i°° and by abuse of notation write ip G 7i°°. Note that 7r°° is compatible with C°° only if the following condition holds: Condition 2 All OPE-constants involving null vectors v G A/"°° as in (3.18) vanish in the limit, i.e. the following conditions hold:

Vv€N°°, V^xG/C00: C°°(x>,¥>) = 0 C°°bdp,v) = 0 = C°°{u*^x).

By (A. 10), the latter two conditions are equivalent. Cond. 2 implies that C°° descends to a well-defined map

C°° : (H00)* ® H°° ® H°° —> C.

Though short and elegant, Cond. 2 seems not to be very convenient to check in our applications. See Rem. 2.5.Ü for a simplification and note that in our Def. 2.3 we avoid this difficulty. In order to recover a CFT-like structure in the limit, we will introduce a direct limit of the decomposition (3.7) on 7^°°. To this end, we will need Condition 3 l There axe decompositions of the vector spaces Ti} into common L 0- and L0-ei- genspaces, which are preserved by the f?, i. e.

fi(a):=ß.

In fact, the induced maps f? : X\ —> Tj defined by Cond. 3 constitute a di- rect system on the index sets, whose direct limit will be called 1^ := limZj. The preservation of the decompositions by the ff guarantees the existence of a decomposition JC°°= 0 K£ . (3.20)

54 Cond. 3 even guarantees that if Cond. 1 is satisfied as well, then (3.20) imposes an analogous decomposition of A/"00 and therefore results in 0«^. (3.21) aeXoo For tpeH™ with a = [ak], ip ^ 0,

k give the (LQ,L0) eigenvalues of ip . By Conds. 1 and 2 all limits

k ha := lim h k, /ia := lim hak k—*oo A:—>oo exist. Therefore, we can define the following operators on H°°:

These give rise to a coarser decomposition of H°° than (3.21) into (Lo> £o) genspaces,

h-heZ In particular, as opposed to a well-defined CFT, it is not guaranteed that all 7i?°r are finite dimensional. Indeed, the 7Y?°r will be infinite dimensional for h,h h,h some of the examples studied in Sects. 3.3 and 3.4. In order to nevertheless allow a definition of modes analogously to (A.13), we will therefore need Condition 4 For all a e loo and all

T,rM x) ••= {ß e 1O°\H? C «£+/4IW ^ e nf-. C°°W,

is unite dimensional. Cond. 4 can also be derived from a version of uniform convergence on the Cl which we discuss in Rem. 2.5.v. To summarize, a sequence of CFTs which obeys Conds. 1-4 gives rise to a limit vector space H°° with non-degenerate bilinear form (-|-)oo = C°°(•*,£&, •) and an OPE-like structure, which assigns modes to each vector in this vector space analogously to (A. 13):

, V/i, )ü, € M, Va G 1^, VX € H~ ^ : (3.22) € Vwfax) s.th.

55 Recall that for a well-defined CFT, the modes of specific subsectors form closed algebras, like the holomorphic and antiholomorphic W-algebras. However, we need additional conditions which ensure that this algebra structure is preserved in (3.22). We first specify Definition 2.2 ___ For a sequence {C\fl) of CFTs, let Wl denote a sequence of unite subsets of r4 with T\ T 6 W and //(VV*) = Wj, which generate subalgebras

of the holomorphic and antiholomorphic W-algebras. Assume that the Wl are all of the same type^. e. they differ only by their structure constants with respect to the elements ofW\ Then the family W* D VirCi © VirCi is called the STABLE W-ALGEBRA, and the elements ofW1 are called W-STATES. By definition, the Virasoro algebra is stable in every sequence of CFTs, and we denote

To guarantee that (3.22) induces the action of a W-algebra on 7i°°, the stable W-algebras have to obey the following two conditions: Condition 5 The ff preserve the primaries of the W1, which never become null:

V»,3 € N: // ((^)W') C {W)W\ and f°° ([H1)™* - {0}) nAf°° = 0.

Condition 6 For every holomorphic W-state w and x £ ^°°J n € Z, the sequence CONVERGES WEAKLY TO wn,oX as defined by (3.22), that is: /C00, Vw,w G VV°°, Vn € Z : ^X.oX*), (3-23) and analogously for antiholomorphic W-states w. Indeed, a sequence of CFTs with stable W-algebras W* which obeys Conds. 1 - 6 featuresji W-algebra action of W°° on H°°, generated by the modes of all W- states in W°°, and with structure constants obtained as limits of the structure l constants of the W>\ The stable W-algebras W are nonTtrivial by definition, since at least Vir^ and VirCi are stable. Hence, for example

co (3 3) c := 2 C (n*,T,L2n) = 2 lim &{{<&)*,T, L\W) = lim a i—>oo i—»oo gives the central charge of the limiting Virasoro algebras Virc, Virc C W°°. Analogously, as expected, for (p g H?0^,

h = IC^^^L^/^W h = \C°°{v\TMv)/\v\2- (3-24)

56 Finally, in order to introduce a limit of the truncated OPE (3.12) for all states that are relevant for our geometric interpretations in Sect. 3.2.2, we will need Condition 7 For alla,ße Too and all

,H) G K2 | 3V G fr as in (3.12). IfH™ C WgJ, then \I(

Definition 2.3 Let (Cl, //) denote a sequence of CFTs with stable W-algebras Wz, whose four- point functions on IP1 converge with respect to the f? as real analytic functions outside the partial diagonals, with the standard behavior near the singularities (see App. A). In other words, for alii eN, ,w £ Wl,

exists as real analytic function ofz,l G C\{0,1} = P^-fO, 1, oo} with expansions (A.4) around the points 0,1, oo. If the sequence moreover fulfills Conds. 3-7, then it is called FULLY CONVERGENT. As a word of caution we remark that in general due to additional null vectors, the limits of four-point functions do not descend to well-defined objects on (ft00)®4.

57 Proposition 2.4 Let (C*, fl) denote a fully convergent sequence of CFTs with stable W-algebras Wl. Then this sequence obeys Conds. 1-7. Proof: We need to show that Conds. 1 and 2 follow from the convergence of four-point functions on the sphere and Conds. 3-7. Indeed, Cond. 1 is an immediate consequence, since for

(=8)

To see that Cond. 2 is satisfied, first assume that there are vectors v 6 A/^, V? € £?j, X € K,™c such that C°°(v*,(p, x) ¥= 0, and choose a sequence {V'Hj of orthogonal bases of the Hl,tä 6W'._j, which converges weakly to an orthogonal J h),hj basis of JC°°. Using (A.10), we can expand the following four-point function around z = 0 as in (A.9):

In particular, we can choose i/4 := v% and obtain a contradiction to the conver- gence of four-point functions. By (A.10), this also contradicts the existence of u,

58 Remark 2.5 i. Since for ip € Hl -r in a convergent sequence of CFTs (ft*|f2*(l, l)ip(z,~z)\ip)i x % 2h 2h = C ((ti )*,xp, ip)z~ J~ , the convergence of the (LQ,LO) eigenvalues for states with non-vanishing norm follows independently from the arguments given after Cond. 3.

ii. The crucial step in the proof of Prop. 2.4 is the observation that each coefficient in (3.25) remains bounded in the limit. The latter is equivalent to the following condition:

For x,i> e IC°° set f/ := h^ - hxi, Jf := h^i - Hxi; (3.26) then y

Hence (3.26) implies Cond. 2 and is equivalent to the convergence of four- point functions (x'K^Cl, !)¥>*(*, *)lx%

iii. In general, null vectors of a representation of the Virasoro algebras Virc, Virc are defined to be states that descend from a lowest weight vector but vanish under the action of each Ln, Ln with n < 0. Although our definition (3.18) of null vectors is different, a fully convergent sequence of CFTs has stable Virasoro algebras and allows us to define the action of Vire, Virc on 7i°° such that null vectors in this conventional sense are not present, either.

iv. Our definition of a fully convergent sequence of CFTs with stable W- l algebras W simplifies greatly if JV°° as in (3.18) reduces to {0}. Then Cond. 2 is void. Moreover, Cond. 6 follows from the convergence of four- point functions, since the limiting four-point functions are well-defined on 7i°° and the factorization properties (A.9), (A.17) - (A.18) of four-point functions remain valid in the limit. As in ordinary CFTs, this also implies associativity of the OPE in the limit, and the existence of all n-point functions on P1.

v. It is not hard to show that Cond. 4 is equivalent to a version of uniform convergence of the OPE-constants:

e H°°, Vx 6 ?C, OL 6 Too, Vji,j5 € R,Ve> 0 3/ € N : Vz > 7, V € V^itp, x) with C°°(r, V, X) ^ 0 :

The above notion of full convergence turns out to be too restrictive for our purposes. In fact, we would like to allow for diverging conformal weights and other structure constants in decoupled sectors of the CFTs. This happens for example in the large radius limit of the free boson on the circle, where the winding modes get infinitely massive as R —>• oo, see (3.16). As motivated by

59 Def. 1.7, in these cases we should restrict our considerations to the closed sectors with converging conformal weights: Definition 2.6 We call a sequence (C\ /?') of CFTs Cl = (W, *\ Cl\ T\ T\ C{) CONVERGENT, if the following holds: For every i € N, the subspace W C W consisting of those vectors whose conformal weights converge under the f( is closed under the OPE. Moreover,

Vt, j en, i

, *°°, Ü, T, T, C°°) is called LIMIT OF THE SEQUENCE (C\f?) OF CFTS. The stable W-algebras are called PRESERVED W-ALGEBRAS.

Remark 2.7 The discussion of convergence of sequences of CFTs generalizes to one-dimensio- nal CFT-spaces

3.2.2 Geometric interpretations As mentioned above, our notion of convergence admits the occurrence of de- generation phenomena. One of them is the VACUUM DEGENERACY, i.e. the degeneration of the subspace of states with vanishing conformal weights. While this subspace is one-dimensional in a well-defined CFT, it may become higher- dimensional, and even infinite-dimensional, in the limit of CFTs. In Def. 1.7 we have introduced PREFERRED GEOMETRIC INTERPRETATIONS of CFTs; in this section we will argue that limits of CFTs with an appropriate vacuum degener- acy can be expected to allow such geometric interpretations. Similar approaches 30In fact, CFT-spaces of toroidal models, more generally of WZW- and coset-models (see [39]) or of orbifolds thereof, and discrete sequences of CFTs are the only well known examples of CFT-spaces. Although the moduli space M of N = (4,4) SCFTs on K3 is known [2], the corresponding CFT-space S over M has not yet been constructed.

60 have been proposed in [78, §6] as well as [42, 72], but with no general definitions of sequences and limits of CFTs at hand. In the following, let (0%^ = (H\ *\ Sl\ T\ T1, C*)^ denote a conver- gent sequence of CFTs. As in Def. 2.6, its limit is denoted C°° = (H°° := /CTO/Af°°, *°°, SI, T, T, C°°). By Cond. 5 we can set

JJOO .=

Note that H°° C H°°, since descendants cannot have vanishing dimensions. To every

co V^GH°°: Av:m —> H°°, AV(X) := *(

M£°_ := M°° D H™v for all h,heWLwe und A^ (w™-A C H^. In particular, A°° acts on H°°. Proof: Fix ip € H°°. Note that L\

= 0,

which by definition (3.18) proves Li

£.,> X € W~x.: (h4> ~ hx) C°°(ip*,

Hence C°°(ip*,ip,x) = ^(A^x) ¥" 0 only if hx — h^, and similarly hx = h^. This proves the claim. D By the above, the only non-trivial mode of each ip G H°° is <£>o,o- This motivates

Definition 2.9 In the limit C°° of a converging sequence of CFTs we set H°° := 7^0 and call 00 A°° := {Av\ (p G H ) the ZERO MODE ALGEBRA. To fix notations, we now choose an orthonormal basis {^jK-g^ of H°° such that

61 *(ipj) = ipj for all jeN and ipj€.Hl.-i where as always ^»*- is a representative of ty, i.e. ipj = /£°($) in H°°. We set

c (A } (A 2) Vo, 6, c e N: Ca 6 := C°°(V*, V«, V*) =° <& i <&. (3.27) Following [42], we expect the zero mode algebra of a limit of CFTs to give rise to a spectral triple which defines a commutative geometry. In fact, Lemma 2.10 The zero mode algebra A°° of the limit of a sequence of CFTs is commutative if and only if

Proof: t With respect to the orthonormal basis {' Pj}j€^ chosen before (3.27), we have

One therefore checks:

Va, b € N: A^o A^,b = A^h o A^a ^ E E^Ä VcdeN (3.28) j i (3.27) <=> AoA = A D

Proposition 2.11 The zero mode algebra A°° of the limit of a convergent sequence of CFTs is commutative. Proof: By the proof of Lemma 2.10, the claim is equivalent to (3.28). This equation follows from the relations imposed on the OPE-constants by crossing symmetry. Namely, for all o, b, c, d€ N, both sides of

converge to real analytic functions on C — {0,1} = IP1 — {0, l,oo} with power series expansions in z, 2; z~l, IP1, respectively. Since by Cond. 5 the sum over primaries in (A. 16) does not contain contributions from null vectors, we can use (A.16) - (A.18) to analyze the structure of (3.29): Both sides converge to formal power series in z, z~l, z~, ~z~l, respectively, with non-negative integer exponents, only, which by Lemma 2.8 are regular. Hence both sides must be constant, receiving only contributions from the leading terms in the conformal blocks31. 31Indeed for the proof of the Proposition, it is actually enough to argue that the constant parts of the limits of both sides of (3.29) have to agree, which gives the required identity (3.28).

62 Then (A.18) shows J^j cLCcj = Ej CLCcj whidl bY (3-27) is equivalent to (3.28). D

Remark 2.12 i. Similarly to Rem. 2.5.iv, the proof of Prop. 2.11 simplifies considerably if null vectors are not present in JC°°. Then the proof of Lemma 2.10 00 shows L\tpa—0 as an element of /C°° for all tpa e H , such that for all

o = {^1^(11)^^(^)1^}

In other words, all conformal blocks are constant, and crossing symmetry can be used directly to show Prop. 2.11. ii. Our definitions easily generalize to the case where the central charges of the left and right handed Virasoro algebras do not coincide. Then the situation greatly simplifies if all CFTs under consideration are chiral: One immediately identifies Av(x), f,X€ M°°, with the normal ordered product of

By Prop. 2.11, limits of CFTs are naturally expected to possess preferred geo- metric interpretations: Definition 2.13 Let C°° denote the limit of a convergent sequence of CFTs with limiting central charge c and zero mode algebra A°°. Let e : N —» M, limi_>0Oe(2) = 0 be a function of maximal asymptotic decay for i —> oo such that for all

\\, ~ hm —-r— < oo, H°°ip := \e

Then the linear extension of H°° is a self-adjoint operator H°°: H°° —> H°°. If there exist completions E°°, Ä°° ofH°°, A°° such that (M°°;H°° ,Ä°°} is a spectral triple of dimension c, then the latter is called a GEOMETRIC INTER- PRETATION OF C°°.

Remark 2.14 Note that the condition on e in Def. 2.13 only fixes the asymptotic behavior of e up to a multiplicative constant. Thus, also H°° is only defined up to this

63 multiplicative constant, which in the geometric interpretation just rescales the metric. A limit C°° therefore only determines a spectral (pre-)triple up to an overall scale. In the following we will usually fix this constant, and it will be understood implicitly that the spectral (pre-)triple is only defined up to a rescal- ing.

Remark 2.15 Indeed in all examples we know, the operator H°° satisfies the following 7-term identity: V/, g, h £ A°°

[H°°,fgh] - [H°°,fg}h-[H°°>gh}f-[H°°,hf}g (3.30) + [H°°, f] gh + [H°°, g] hf + [H°°, h] fg = 0, which means that in the geometric interpretation H°° can be regarded as a second order differential operator without zeroth-order term, i.e. as a, generalized Laplacian. This is expected from sigma model considerations (see e.g. [98]). In fact, M. Kontsevich explained us an argument proving (3.30) in the general setting of degenerations of CFTs discussed above. We refrain from spelling this out here. Instead, we content ourselves with noting that (3.30) is obviously fulfilled in all the examples discussed below. The fact that H°° is a generalized Laplace operator in the geometric inter- pretation, which thus can be written in the form (3.6) then allows us to read off a metric g and a dilaton $ from the triple (H, H°°,A°°) obtained from a degeneration of CFTs. The above definition may seem artificial, since we cannot prove a general result allowing to give geometric interpretations for arbitrary limits of CFTs. How- ever, below we will see that there are interesting examples which do allow such geometric interpretations, in particular a non-standard one which we present in Sect. 3.4. Moreover, from the viewpoint of non-linear sigma model constructions and large volume limits of their underlying geometries, Def. 2.13 formalizes the expected encoding of geometry in CFTs, see [78, 42, 72], which justifies our definition.

3.3 Limits of conformal field theories: Simple examples This section consists in a collection of known examples, where we discuss limits of CFTs and their geometric interpretations in the language introduced in Sect. 3.2. Sects. 3.3.1 and 3.3.2 deal with toroidal CFTs and orbifolds thereof, respectively, in Sect. 3.3.3 the boundaries of moduli spaces of WZW models are discussed. We confirm that our techniques apply to these cases and that they yield the expected results. In particular, the discussion of toroidal CFTs fits our approach into the picture drawn in [42, 72].

3.3.1 Torus models As a first set of examples, let us discuss bosonic toroidal CFTs. These are u(l)d- WZW models, whose W-algebras contain u(l)d © u(l) -subalgebras generated

64 by the modes of the respective u(l)d = Revalued currents. That is, (B.I) generalizes to /(*) = 5>^-\ f{z) = neZ a a kl l [ n> Ü =m5 öm+nfi, [än,ä m] = Holomorphic and antiholomorphic energy-momentum tensors can be obtained as T = \ Y^k '-3k3\ T — \Hk '•3k~3k'-- Their modes give rise to holomorphic and antiholomorphic Virasoro algebras with central charges c = d. The pre-Hilbert space Hv of a toroidal CFT Cr decomposes into irreducible lowest weight representations of u(l)d©u(l) , which are completely characterized by their holomorphic and antiholomorphic u(l)d © u(l) -charges (Q; Q) € F C

The corresponding norm-1 lwvs \Q; Q) have conformal weights32

2 h 1^2 T - — in n\Q;Q) - 2^ » n\Q;Q) ~ 2^ ' see and, by definition, the corresponding fields V\Q-Q\(ZI'Z) ( (A-.7)) obey

,^) +reg.; (3.31) Q J^W*'*) = (w - 2)

The n-point functions of the VXQ.-QX (Z, Z) reduce to products of the respective holomorphic and antiholomorphic conformal blocks

(3.32) Recall that the right hand side gives a well-defined function for Z{, ~z~i € C away from the partial diagonals, iff all QiQj — QiQj £ Z. Indeed, the charges (Q; Q) of lwvs in a toroidal CFT constitute an even integral selfdual Lorentzian lattice r C Md)d of signature (d, d), where the quadratic form is given by the double spin 2(h — h) of the respective state, and addition corresponds to fusion. We denote by Ud the unique even integral selfdual Lorentzian lattice of signature (d,d) and regard F as image of an embedding33 i : Ud ^ F C Rd'd of Ud into Rd>d. Making use of the OPE (3.31) and contour integration, the n-point functions of descendants can also be extracted from (3.32). This procedure only involves , p. derivation and multiplication by charges Q , Q . 32 For Q e Rd, Q2 denotes the standard quadratic form on Rd. 33 The embedding is only specified up to automorphisms of U .

65 To determine the OPE-constants of lwvs from (3.32) note that the overall sign on the right hand side of this equation depends on the ordering of the fields VIQ..Q Aziy'zi). This is due to the COCYCLE FACTORS which for d = 1 have the simple form (B.6). To state a general formula, we first have to generalize (B.4). Given a toroidal CFT with charge lattice t{Ud) = F c Rd'd, one can always find a lattice A C Rd of rank d and a linear map B:Rd —> (Rd)*, such that with respect to appropriate coordinates on M.d>d the following holds: Denote by A* C (Rrf)* the Z-dual of A and identify {Rd)* with Rd by means of the standard scalar product on Rd. Then B is skew-symmetric and

r = {(Q; Q) = ^ {ß - BX + A; M - BX - A) | (/*, A) € A* x A} . (3.33)

Moreover,

(/) for (QW;Q ) = ^ (/*« _ SAW + A(0 ; ß(>) _ ßAW _ A(')) e F: (3.34)

with all other OPE-constants vanishing. Note that for d = 1, Eq. (3.34) simplifies to (B.4) - (B.5) due to the absence of the ß-field. By the above, a toroidal CFT C = Cr is completely characterized by its charge lattice F, and thus the moduli space of these models is the NARAIN MODULI SPACE

•A^Narain = O(d,d,Z)\O(d,d)/O(d) X 0{d) of even integral selfdual Lorentzian lattices in Rd'd [15, 83]. 1 1 We will discuss sequences (C := Cr4,//) of toroidal CFTs in A^arain witi stable W-algebra u(l)d © u(l) and fixed n:Ud -»• Ti such that

V», j, € N, A G f/d, P, P £ C[x{, ...,xixl...,xi...}: (3.35)

ti •• P (K)m) ? ((*&) |*i(A)>i ^ P ((o*)*,) P ((S*

This choice of sequence is natural from the point of view of deformation theory and completion of A^Narain' see R-em- 2.7. Indeed, the OPE of lwvs is constant under the // defined in (3.35), and OPE as well as all correlation functions of such sequences converge if and only if the lattices F^ = ti(Ud) converge in Rd>d. In this case, (3.35) is fully convergent in the sense of Def. 2.3. Furthermore Af°° = {0}, which implies that the limiting n-point functions have the usual factorization properties (c.f. Rem. 2.5.iv). In fact, the lattices F; converge within A^arain' such that no degeneration phenomena occur. All n-point functions on surfaces with positive genus converge as well, and the limit of such a sequence is again a toroidal CFT with charge lattice Too = limi-^ooFj. / On the other hand, A f^arain is not complete, and a sequence of lattices F^ may degenerate but still give a convergent sequence in the sense of Def. 2.6. Namely, given any primitive null-sublattice AT c Ud of rank 5 € N, one can construct

66 convergent sequences such that the images L{(N ) converge with tj(iV) collapsing to {0}, while the images of lattice points in Ud — iV-1 diverge. In fact, we can split34 Ud = N* © NL = N* © N © M, (3.36) such that N* is null with N* © N = C/5. Then the lattice in the limit, FQO := lim ti(N±) = lim tj(M), i—KX> i—+00 is again an even integral selfdual Lorentzian lattice in M.d'd, however with smaller rank: r«, = Ud's. Every sequence (3.35) showing this kind of degeneration is convergent in the sense of Def. 2.6. The limiting pre-Hilbert space is a u(l)d © u(l) -module

As before, we have TV00 = {0} and therefore the usual factorization properties of the limiting n-point functions on the sphere. However, the degeneration of the lattice results in a diverging torus partition function, and the limit only has the structure of a CFT on surfaces of genus 0 with an infinitely degenerate vacuum sector. In the spirit of Rem. 2.7, we regard these degenerate limits as boundary points of the CFT-space S over O(d,d)/O(d) x O(d) of toroidal CFTs. The underlying Hausdorff space of such boundary points has a stratification

ddes{O(d,d)/O(d) xO(d)) ^ (J O(d- 5,d - 6)/O(d - 5) x O(cZ- 5). l

AT = Q[r], e: ((Q; Q), {Q1^')) —• (-1)^', (3.38)

i.e. \Q; Q) ffl \Q'; Q1) = (-I)"*' \Q + Q1; Q + Q1) with notations as in (3.34). For any N as above, the lwvs corresponding to elements in N generate a commutative subalgebra AN — C[N] C ^4r- Similarly to the one-dimensional case discussed in Sect. 3.1.3, restriction to AN gives a commutative geometry. In fact, AN is isomorphic to the algebra of smooth functions on a J-dimensional torus T^N) = R5/2TTAS, where A$ is a lattice of

Here, © denotes the direct sum, not the orthogonal direct sum.

67 rank 6 such that i(N) C F in (3.33) is described by restricting to lattice vectors () J The zero mode algebra A°° associated to the degenerate vacuum sector of (3.37) (see Sect. 3.2.2) is isomorphic to AN — C[iV], whose closure is the algebra of smooth functions on a topological torus TN- More precisely, each /j, € A| corresponds to a function T^N) 3 x h^ etß^ € C. It is an eigenfunction of the Laplacian on T^jv)» equipped with the standard metric inherited from Rs, with eigenvalue /it2. The latter goes to zero as i —> oo. Since 7V"°° = {0}, .4°° also acts on the entire limiting pre-Hilbert space H°°, which is a projective module of finite type over .4°° and can therefore be regarded as the space of sections of a vector bundle over TJV — Spec(^4°°). Thus, in the limit we find a CFT-fibration over the moduli space TN of ground states of the limit theory as described in [72]. In fact, with a suitable choice of coordinates as in (3.33), the limiting structure of such degenerating sequences of toroidal CFTs can be regarded as LARGE VOLUME LIMIT, where TH(N) is the sequence of subtori obtaining infinite radii, while their duals collapse. It is a geometric interpretation in the sense of Def. 2.13, if N is a maximal null sublattice, i.e. if 6 = d. Otherwise, it can be viewed as geometric interpretation of an appropriate subtheory with central charge d = S. Remark 3.1 As described in Ex. 1.9 for the case of spectral triples of circles, we can also use partially ordered systems to obtain limits of toroidal CFTs different from the ones discussed above. For instance, in the case of circle models CR, R G R+ (see Ex. 1.5, App. B), we can define a partially ordered system analogously to the construction given in Ex. 1.9. In the latter case, the limit spectral triple for functions on circles corresponds to R with a complicated topology. Similarly, the limit of the partially ordered system of circle theories decomposes into subsectors which only couple through the vacuum. However, as explained in Rem. 1.10, one does not have to use the direct limit construction to define limits of spectral triples, and the same is true for limits of CFTs. Let us briefly discuss this in the case of the INFINITE RADIUS LIMIT OF CIRCLE MODELS. To define a limit of the ordered set (CR)Ä€R+ of CFTs without a given direct system, we have to find an appropriate Hermitean limit vector space H°° and epimorphisms /# : 7i°° —* HR, R ER+, by hand. In fact, using notations as in (3.15), o 2 H°°:=C2 (R)®C[x1,X2,...]® (3.39) together with A (3-40) satisfy conditions similar to those stated in Rem. 1.10. Since the respective limits exist, we can define limit correlation functions by

z!,zi)... (pn(zn,zn)\0) := lim {0\fR((pi)(zi,zi).

68 and similarly obtain limit OPE-constants. The notion of convergence of sequences of CFTs introduced in Defs. 2.3, 2.6 can be generalized to such a limit construction of ordered sets of CFTs.

Indeed, the system (CR, /K).R€R+ denned by (3.39) - (3.40) is convergent in this generalized sense. Its limit is a full CFT, namely the UNCOMPACTIFIBD FREE BOSONIC THEORY with pre-Hilbert space35

and in particular does not show any degeneration phenomena. We emphasize that H00 and the /# had to be constructed by hand and are not compatible with CFT-deformation theory, which is our reason for preferring the direct limit construction of Sect. 3.2.

3.3.2 Torus orbifolds If a given CFT allows an appropriate action of a finite symmetry group36, then one can construct a new model from these data by ORBIFOLDING, see e.g. [22]. Since from our point of view the main ideas are apparent already in the simplest 1 examples of torus orbifold models, namely the S /Z2-orbifold theories CR, R G R+, that is the Z2-orbifolds of the circle models CR described in Ex. 1.5 and App. B, we will restrict our discussion to this family. On the pre-Hilbert space HR of the circle theory CR, the non-trivial element of Z2 acts by

• P(an)P(än)\QR; QR) .—> P(-an)P(-an)\ - QR; -QR) for P,P€ C[xi, X2,...]. The pre-Hilbert space of the resulting orbifold model CR consists of the ^-invariant part of 7iR and additional twisted sectors. Each sector decomposes into lowest-weight representations of the generic orbifold W- algebra W = W(2,4) ©W(2,4) C u(l)©u(l) as detailed in [82]: In the untwisted sector, there are norm-1 lwvs •^[QR'IQR)1'2 = 4j| — QR'I—QR)1'2 of conformal weights h = \QR, h = \QR for each Z2-equivalence class of charges (B.4) appearing in the original circle theory. An additional norm-1 lwv \QR) of con- formal weights h — h = 1 occurs in the basic u(l) © u(l) representation with = l QR QR — 0- Furthermore, in the twisted sector, there are four lwvs \cr R), 1 \T R), I e {0,1}, with h = h= ^ h = h = -jg, respectively. The OPE in the circle theories is invariant under the Z2-action, and the OPE in the orbifold models respects the Z2-grading on the pre-Hilbert spaces. Hence the correlation functions and OPE of states in the invariant sectors of the orbifold models coincide with the respective data in the circle theories. Correlation functions containing states in the twisted sectors have been discussed in [25, 24], and the OPE between lwvs can be extracted from them. 35This pre-Hilbert space is a closure of H°° defined in (3.39). 36 That is, the group acts as group of automorphisms on the pre-Hilbert space of our theory leaving the n-point functions invariant, and the level matching conditions [26] are obeyed.

69 Given a sequence {Ri)i€N in R+, we consider the sequence (C^, f?) of S1/^- 22 z orbifold models such that on lwvs //(IQ/^Q^) ) = \QRj; QRj) \ ff (I©*,)) = T r This definition |ÖÄ,-)» //d<4» = Wk,)* //(l k)) = l k)- naturally extends to the descendants as in (3.35). Then, as in the case of toroidal models, all correlation functions and the OPE converge with respect to the // if and only if (Aj)igN converges in R+, limj-tooRi = i?oo > 0. In this case, {Cj?,fD is a fully convergent sequence of CFTs in the sense of Def. 2.3, and J\f°° = {0}, implying the existence of correlation functions on P1 (see Rem. 2.5.iv). No degeneration occurs, which means that correlation functions on surfaces of positive genus converge, too. Thus, in the limit we obtain a full CFT, namely the S1/Z2-model at radius ÄQQ. If Ri —> 0 or Ri —> oo, our sequence of CFTs is convergent in the sense of Def. 2.6. Indeed, all correlation functions between states with convergent weights converge, 7V°° = {0}, and in the limit we obtain a well-defined CFT on the sphere with degenerate vacuum sector. In the language of Sect. 3.3.1, for Ri -* oo we can use (3.36) with M = {0} and N = lA^(m;m) \ m € z|, N* = {^(n; -n) \ n € z}, and N <-• N* if Ri -> 0.

By Prop. 1.4 we can associate a spectral pre-triple (M, HhA) to each orbifold model CR2. AS mentioned after (3.12), here we find Hw ^ VT. By [25, 24] the OPE-constants including twisted ground states are given by

a a Ä) >\Qm,n,Qm,n) A^R)) = & \{.\Qm,n;Qm,n} ) , \ R.) > \ RJ)

l with notations as in (3.15). Hence the /vv(o"^, a R) used in (3.12) are infinite. On the other hand, A contains a subalgebra given by the Z2-invariant part A' := 2 oo, the zero mode algebra .4°° = C[Z]Z2 is generated by the lwvs rep- resented by | -2*—; -^—)Z2, m € Z. It is the algebra of Z2-symmetric functions on the circle, i.e. the functions on S1/^- In fact, the |m)^ := /f° ( ) are characterized by the recursion relation which agrees with the recursion relation for the (rescaled) CHEBYSHEV POLY- NOMIALS OF THE FIRST KIND, see e.g. [65]:

Tm(cosx) := 2cos(m:c), for m G N, x G [0,TT].

Hence \m)%g should be identified with the function x i-> Tm(cos;c). This is not surprising, since the lwvs |m)^ are Z2-symmetric combinations of lwvs in the underlying circle theories, which in turn correspond to exponential functions.

70 2 Indeed, {To/\/2, TI, T2, ...} is an orthonormal basis of L ([0, TT], dvols) with 1 dvol9 = cte/27r, i.e. with the flat standard metric g on [0, TT] = S /^- Hence the 2 00 methods of Sect. 3.1.1 yield !°° = L (SVZ2,rfa;/27r), A°° = C ^/!^), which according to Def. 2.13 for the limit gives the expected geometric interpretation on S2/Z2 with the flat metric g induced from the standard metric on S1 and 1 a trivial dilaton <&. Note also that the m™ Chebyshev polynomial Tm is an 2 eigenfunction of the Laplacian ^Afl = —5^2 with eigenvalue ^rri , as expected from

with Al =

As for the toroidal CFTs discussed in Sect. 3.3.1, A™ acts on the entire pre- Hilbert space H°° which can be regarded as the space of sections of a sheaf over Sx/Z2. Let us restrict the discussion to the states |cr')oo := /?° (|<7^)). The action of ^4°° on them can be extracted from the OPE-coefficients (3.41):

ml Z2 -1) \Qm,n ; Qm,n) H WR) = ~~~ \ l\ oo-

l It follows that the sections corresponding to \a R) are peaked around the respec- tive Z2-fixed points, i.e. the endpoints of the interval [0, IT]. In the limit their support in fact shrinks to these points. The same holds true for all other states in the twisted sectors. They are sections of skyscraper sheaves over the fixed points of the orbifold action. As expected, in the limit the OPE of two states in the twisted sectors vanishes, unless the corresponding sections have common support. This gives a nice geometric interpretation of the twisted sectors.

3.3.3 WZW models As was shown in Sect. 2.2 current-current deformations of general CFTs can be understood in terms of pseudo-orthogonal transformations of certain charge lattices. Namely, current-current deformations only affect the representation theory of the f) © f)-W-algebra generated by the deformation currents, while the OPE of the lwvs with respect to this W-algebra are unchanged. This is a generalization of the situation in toroidal CFTs, which are com- pletely characterized by their charge lattices (c.f. Sect. 3.3.1). In particular, current-current deformation spaces are given by (2.8) and degenerations of CFTs at the boundaries of these spaces can be analyzed in a similar fashion as was done in Sect. 3.3.1 for toroidal CFTs. Let us illustrate this in the case of WZW models whose current-current deformations were discussed in detail in Sect. 2.3. As explained in Sect. 2.3, a point in the current-current deformation space (2.22) of a jjfc-WZW model is specified by an isometric embedding 1 — (Q, Q) : c d d Ao -> R ' of the even Lorentzian charge lattice (2.24) of the WZW model

71 into Rd'd, where Q,Q denote the projections on Rd>° and R°>d respectively. We set P := t(Ao). Then the Hubert space of the deformed WZW-model can be decomposed as follows (c.f. (2.23))

where [n] denotes the equivalence class of JX 6 P(g) in P(g)/fcQ(g). The corre- sponding lwvs are denoted by |(A,}j,,~ß))u. Now, let us consider a sequence of CFTs in X\vzw specified by ii and37

(3-43) Vi,j,G N, A G fife, (A*,M) G Ao and P,P e C[x\,... ,xf,x\,... ,x$,...]. For the same reasons as in the torus case, such a sequence is fully convergent iff i\ converges on the entire lattice Ao. In this case, the sequence (3.43) converges to the full CFT in the WZW deformation space which is characterized by the limit too := limi-Kjof-i. However, also as in the torus case, the space £*wzw is not compact and degenerations of the charge lattices may occur at its boundaries. Indeed, since current-current deformations of WZW models only affect the rep- resentation theory of the respective current algebras, (3.43) is convergent iff the sequence tj is convergent on the sublattice of Ao where <,$ is non-divergent. The limit structure then only depends on the limit of the sequence of tj restricted to this sublattice and furthermore M°° = {0}. Let us discuss such degenerations in slightly more detail. For simplicity we restrict our attention to the following maximal degenerations. For w G W(g) d d d choose Nw := Ao fl {(x, wx)\x G R } C R ' as the null-sublattice of Ao which collapses to {0} in the limit. Since Nw is of maximal rank, the charges of all vectors in AQ\NW simultaneously diverge in this degeneration. Thus, the limiting pre-Hilbert space is given by

V V V Ä.fal ® Ä.F7il ® <3=o ® Vs=0 • (3-44)

As alluded to above, the sequence is convergent. In fact, all correlation functions on the sphere converge. Thus the limit carries the structure of a CFT on the sphere. The vectors in fi°° with vanishing conformal weights have to come from coset-factors which are isomorphic to the vaccum representation. Thus, as a vector space .A00 is generated by the vectors

\(u, k(y + //), kw{v + ^))oo , z> simple current, \x € Q(g). (3.45)

The OPE of the simple currents38 reduces to addition of charges and one finds

A°° <* C[D(g)], (3.46)

37 As in Sect. 2 the modes of the deformation currents axe denoted by fn, ~fn respectively. 38Simple currents and field identifications of coset models are discussed e.g. in [52, 92].

72 where D(g) is the lattice generated by the roots of g together with those weights of g which give rise to simple currents39. The spectrum of this algebra is a d-dimensional topological torus Td and, as for the toroidal CFTs, from the degeneration of the conformal weights one can deduce a degenerating sequence of metrics on Td. As in the torus case, the dilaton is trivial. Furthermore because we have convergence with M°° = {0}, H°° is an „4°°- module and can thus be interpreted as the space of sections of a sheaf of vector spaces over Td. In fact H°° is a projective ^4°°-module and corresponds to a trivial vector bundle over Td. Its fiber is isomorphic to the tensor product of the state space of the tu-twisted g^/fy-coset model and vacuum modules from the current-algebras

W(S*/8)» o vQ=0 ® VQ=0 . (3.47) Note, that the field identifications of the coset models arise quite naturally here through the presence of simple current states in A°°. A simple example is the su(2)fc-WZW model. Its current-current deformation space is given by 0(1,1)/O(l) x 0(1) = R>0. There are two possible degenera- tions corresponding to the points 0, co. These correspond to degenerations of the sublattices 7V"i, Nw C Ao, where 1, w are the two elements of W(su(2)) = Z2. The corresponding CFT-limits have the structure of fibrations of the 1-, w-twisted 40 st*(2)fc/u(l)-WZW models on the circle. In the same way other in general non-maximal degenerations can be ana- lyzed. Collapsing rank-J sublattices of Ao leads to fibrations of gfc/u(l)l5-coset models over ^-dimensional tori Ts. In view of the results of Sect. 3.3.1 this is expected from the orbifold representation (2.37) of deformed WZW-models and the completion of the deformation spaces is in fact the same as the one for toroidal CFTs. In fact, the arguments given above do not restrict to WZW models but gener- alize to current-current deformations of arbitrary compact CFTs. Degenerations in this general setup also give rise to fibrations of the respective coset models over topological tori.

3.4 The m —> 00, c —»• 1 limit of the unitary Virasoro minimal models A4(m,m + 1) In Sect. 3.4.1 we show that the techniques introduced in Sect. 3.2 for the study of limits and degeneration phenomena also apply to the family of diagonal unitary Virasoro minimal models M(m,m + 1), m G N — {0,1}, which gives a fully convergent sequence of CFTs. In Sect. 3.4.2 we determine and study a geometric interpretation of its limit .Moo as m —> 00, and we discuss the inherent D-brane geometry.

39 For simply laced Lie algebras all weights can be obtained as sums of roots and simple current-weights, i.e. in this case D(g) = P(g). 40 These correspond to the axially and the vectorially gauged WZW model respectively.

73 3.4.1 The unitary Virasoro minimal models M(m, m + l)m_).oci Both outset and favorite example for our investigation are the unitary Virasoro minimal models Mm := M.(m,m + 1), m € N — {0,1} [7], which correspond to the (A, A) (left-right symmetric) modular invariant partition functions in the CIZ classification [13, 14]. In this section, we explain how a fully convergent m m sequence (C , /4) with C = Mm for m e N — {0,1} can be defined according to Def. 2.3. To our knowledge, such a construction was first alluded to in [28, §6 and App. B] as well as in [78, §6]. Our approach also allows us to determine a geometric interpretation of the limit of this sequence a^m^oo, according to Def. il3.

Let us start by recalling some of the main properties of the CFT M.m. Since this model is diagonal, we can restrict our discussion to the action of the holomor- phic Virasoro algebra. The pre-Hilbert space of Mm decomposes into a finite sum of irreducible representations of the Virasoro algebra Vir^ with central charge e--1-;$rnr (3'48) These irreducible representations are labeled by Mm.= {(r, s)\r, s € N, 1 < r < m, 1 < s < m + l}/~ with (r, s) ~ (m — r, m + 1 — s), i.e. r + s ~ 2m + l — r — s, such that by choosing appropriate representatives we can write

Mm = {(r, s)|l

Each irreducible Virasoro module V(?s\, (r,s) € Mm, has an lwv \r,s)m of con- formal dimension (r{m + 1) - sm)2 - 1 m^oo (r - s)2 r2 - s2 s2 - 1 (r, s). We will extend these embeddings to vector space homomorphisms f%+l between the corresponding irreducible Virasoro modules. To meet Cond. 5 of Sect. 3.2.1, we must map lwvs to lwvs:

r, s) 41Our choice of embeddings is quite natural and has been used already in [103] in the context of slightly relevant perturbations of Mm- However, there are other choices, leading to different limits of CFTs.

74 similarly to (3.35). Here, P, P are elements of the same degree in the weighted polynomial ring C[a;i,:E2, • ••] with degrcn = n, and we substitute xn = L™ or +1 xn = L™ in lexicographical order (see Def. 4.1). To construct consistent maps of type (3.51), recall from [7] that the char- acteristic feature of the representation Vr?s\ is the fact that the Verma mod- ule built by the action of the Virasoro algebra Vir^ on \r, s)m with character q^&n (^ an(j ^,gen ^ m (g 7) contains a proper non-trivial submodule of SINGULAR VECTORS, that is of lwvs of Vir^ at positive level. The occurrence of these singular vectors, which have been quotiented out to obtain VP .,, makes \T,S) our construction slightly delicate. However, the very properties of direct lim- its allow us to solve this problem. For later convenience, we give the following technical Definition 4.1 Let m G N - {0,1} and (r, s) G Mm. For each N G N choose a set VJ^sj(N) of monomials with weighted degree N, such that

{p(L™)|r, s)m | P € r%s)(N), Ne N} (3.52)

n is a basis ofV%s), where for P G P^AN), P(xn) = n< ™th a, G N and

P(L™) := [L?)ai o (L£T2 o • • • .

IfB™s) G N obeys

1 VN,N' G N: N + N' < B^s) =• V^s)(N) • V£s)(N ) c

A then B^s) G N is called an ENERGY BOUND ofV^s) = (P(?s)(A0);v6N. system •R™ x with maximal energy bound among all systems giving bases (3.52) is called a BASIC MONOMIAL SYSTEM OF WEIGHT Wfi. sy A sequence (P^s of monomial systems is called SPECIAL if for all m> M and for all N < Pjjf^JV) = V^^HN), where BP ^ are the respective energy bounds, andahnost all VVl, are basic. [T,SJ Note that the relations which arise from the existence of singular vectors in the

Verma module over \r, s)m, up to a global pre-factor (m(m +1))""^ with K G N, are linear with respect to all monomials P(L™) of a given weighted degree iV, with coefficients ap G R[m] of degree at most 27V". Moreover, as follows from the explicit character formula (C.I), the singular vectors which under the action of T r Vi- cm generate the submodules of singular vectors have weights h P+m _s+m+l-, and /ijy _s+2(TO+i))> i-e. levels rs and (m—r)(m+l — s), respectively. We conclude that for fixed r, s G N — {0}, the energy bound of basic monomial systems ~PJ^S) of weights hfr * is monotonic increasing in m. Moreover, Lemma 4.2 For every pair r, s G N — {0} with (r, s) G MM (M minimal), we can choose a special sequence (VV£s\)m>M of monomial systems according to Def. 4.1, and the respective energy bounds approach infinity as m —> oo.

75 m In the following, (P s\)m>M will always denote a fixed special sequence of mono- mial systems of weights h^s, as in Lemma 4.2. Note that we can depict these monomial systems in terms of a convex polyhedron, as is customary in toric geometry. We then define

+1 ViV € N, VP e P%s)(N) : C [P{L%)\r, s)m] := P(L^)\r, s)m+1. (3.53)

Finally, we linearly extend the /™+1 to vector space homomorphisms fm :J . fm+1. -iim ^^ i;m+l. fj fj frn+1. -i;m c—^ ">;J ld V V V fm — V£3)> Jm • V(r,s) ^ (r,s) ' /m — Jj-l °-°/m • (r,s) ^ (r,s)- Then by construction, Lemma 4.3 Tie sequence (Aim, fm) -is a sequence of CFTs with stable Virasoro algebra ac- cording to Defs. 2.1 and 2.2.

In the following, we show that the sequence (M.my fm) is fully convergent ac- cording to Def. 2.3. Although above we have made a lot of choices, we will argue that our limit is independent of all choices, including the use of monomials and lexicographical order for their interpretation. First note that by (3.48) and (3.50),

2 m—>oo 1 , m m—>oo , (r—s) /Q r-A\ L jL cm —• c = 1, h{rs) —> h(TjS) = ? -, (3.54) i. e. all structure constants of the stable Virasoro algebras Vir^ converge. More- over, setting C Cm $$),(s>s) ••= (ilMmT, K, n)m, |S', ,>m) (3.55) with respect to orthonormal \r,s)m as in [30], the calculations (C.3)-(C8) imply

with A € R and E for t

76 oo. It will therefore suffice to prove convergence of those n-point functions which only contain primaries |r, s)m, since all others can be obtained from them by application of differential operators with coefficients depending polynomially on the structure constants of the Virasoro algebra. Let V(™s\(z>^) denote the field which creates \r, s)m as in (A.7). By [28, 30], an n-point function

on P1 is a bilinear combination of a finite (m-independent) number of specific conformal blocks (see (3.57)) with coefficients given by OPE-constants. Since by Lemma 4.4 all OPE-constants converge asm-* oo, it remains to prove that the conformal blocks converge. To this end we use their Feigin-Puks integral representations for Mm. In particular, we employ the Coulomb-gas formalism, i.e. a BRST construction of the VP ^ (see [34]), which is adequate since the OPE-constants in Mm have been calculated by this technique in the first place [29]. In fact, the correction [35] to [34, (3.14)] ensures that the BRST charges remain well-defined operators as m —» oo, yielding the Coulomb-gas description valid in our limit. Recall (see, e.g. , [34, 1]) that in the Coulomb-gas formalism the VfJ?^ are obtained by a BRST construction from CHARGED FoCK SPACES, built by the action of the Heisenberg algebra on \r, s)m. In particular, primary fields of Mm are given by BRST invariant operators with screening charges, such that f/(l) representation theory can be used to calculate the n-point functions. That is, in an n-point function the field V^Jz, ~z) can be represented in terms of products of holomorphic SCREENED VERTEX OPERATORS

} :== r ^Ul " ' f dui Y dvi •••<£> dvj (3.56)

and their antiholomorphic counter-parts. Here, each Va denotes the holomorphic part of a vertex operator of charge a as in Sect. 3.3.1: V\Q-Q\{Z, and

Each conformal block is proportional to some I f I f

Vctm\U\) * * ' V

77 way that the minimal distance between them as well as the minimal distance between the contours and the Zi is bounded away from zero by a constant. Since the integrand of (3.57) is the well-known n-point function of vertex operators for the free bosonic theory, see (3.32), it therefore converges uniformly on the integration domain implying that limit and integration can be interchanged. Hence the integral of the limit function is well-defined because the integration domain is compact and does not hit singularities of the integrand. D Combining the above results, we find Proposition 4.6 The sequence {Mm, fm) of unitary Virasoro minimal models converges fully to a limit A^oo according to Def. 2.3. Proof- In view of Lemmas 4.4 and 4.5 and by Def. 2.3 it only remains to be shown that Cond. 7 of Sect. 3.2.1 holds. We set

Vr,s€N-{0}: Ir.s)«, := f£{\r,s)m). By (3.54) we have {\r, r)«, | r 6 N - {0}} . (3.58)

Then by Lemma 2.8 for all r,s',s€N- {0} and h = h = (s'~ s)2/4, the OPE- constant C°° (ip*\ |r,r)oo, |s', s)oo) must vanish for every primary ip € H°° with ip 0 Mf3,-. This is directly confirmed by Lemma C.I. Moreover, (C.2) implies m / thatC ((|p',p)m)*,|r,r)m,|s ,s)m) vanishes for all m unless \r-s^\ + l < pW < (/) w w min{r + s - 1,2m - 1 - r - s } and pW + r + s = 1(2). This restricts p and p' to a finite number of possibilities as m —> oo, implying Cond. 7 of Sect. 3.2.1. In fact, a straightforward calculation using (C.4)-(C8) shows

^pl for \r-s\ + lP)°°- ( - ) p=|r-s|+l, p+r+s=l(2) D Note that although we have made many choices in our construction above, the actual structure of the limit M«, is independent of those choices. This is largely due to the fact that Conds. 1 - 7 of Sect. 3.2.1 are rather restrictive. For exam- ple, recall the two basic singular vectors of levels rs and (m — r)(m+l — s) in the Verma module built on the primary |r, s)m. The latter state does not play a role in the limit, since its level becomes infinite asm-» oo. In the language of our basic monomial systems of Def. 4.1 it always lies above the energy bound. On the other hand, the singular vector at level rs has dimension \{r + s)2 and implies

78 that there also is a polynomial Prs of degree rs such that Prs{Ln)\r, s)oo = 0. Since up to normalization, Prs is uniquely determined by r, s, and by the struc- ture constants of Virc=i, the dependence on the choice of the basic monomial r system ('P^s)(^))A eN drops out in the limit. Remark 4.7

In contrast to the examples discussed in Sect. 3.3, for the limit of (M.m, fm) we obtain additional null vectors, i.e. N°° ^ {0}. This is due to the fact that the 2 conformal weights of lwvs \r, s)m converge to (r — s) /4, while the central charge converges to 1 (see (3.54)). By the above discussion of singular vectors, the characters of the limit Virasoro modules before quotienting out the null vectors are given by J

But at c = 1 there are null vectors (B.8) in the Fock spaces built on lwvs with conformal weight h, 2\/7i € N, and the limit characters decompose into characters (B.9) of irreducible representations of the Virasoro algebra of central charge c = 1,

min{T-,s} —1 _ V"^ ~~ 2-~i "*-|(k-s|+2fc)2 ' fc=O Those submodules of JC°°, where /C°° jM°° = H°° as in (3.19), which correspond to lwvs at positive levels consist of limit-null vectors, whose norms converge to r zero for m —» oo. For instance, the norm of fm(LT\ i r)m), r > 1, is given by the limit of

r-2 — 1 \Tm\r r\ I2 — rm((Tm\r r\ YOm Tm\r r\ \ — 0hm m7Z°° - (1 fifVt \^i\r,r)m\ —o {{l^i \r,r)m) ,iZ ,Lx \r,r)m) — IK, •, ~ . {6.W) Thus this vector and all its descendants are elements of As alluded to in Rem. 2.5.iv, the quotienting out by additional null vectors in (3.19) spoils the factorization properties of the limit-correlation functions on P1. However, as pointed out in [61, Sect. 3.1.1] it is possible to modify the definition of the fit in such a way that M°° = {0}. This is achieved by SCALING UP THE ADDITIONAL NULL VECTORS. For example, we can set m „ \r x \r r\lml I Jm\P 1J(LTWl \'i'/mj r)™) •=•— ' .m\)\ _•' PJml-^ (UP-\rl \'i' r) Im)-)

Indeed, homomorphisms fm can be constructed in such a way that (Mm, fm) is a sequence of CFTs with stable Virasoro algebras according to Defs. 2.1, 2.2, which does not lead to additional null vectors asm -» oo. However, the modification fm t-+ fm could destroy the convergence of correlation functions. That this is not the case, and that in fact the sequence (Mm, fm) of CFTs is fully convergent follows from the Coulomb-gas formalism. In the propf of Lemma 4.5 we have already pointed out that the expressions obtained from the

79 Coulomb-gas formalism remain well-defined as m -» oo. Recall that the Fock space representation of elements of Wf i in the Coulomb-gas representation is formally obtained from an action of the positive modes of the Heisenberg algebra on \r, s)m. Hence singular vectors with respect to the action of Vir^ on \r, s)m are automatically zero, see Ex. 4.8 for an illustration. Namely, each singular m m m m vector v 6 /C°° is of the form u = f™(v ) with u = Q \r, s)m, where Q is an operator on Hm which can formally be written as polynomial in the positive modes of the Heisenberg algebra, with each coefficient converging to zero as 77i —> co. In fact, each coefficient is a power series in ^ with vanishing constant term. Therefore, our rescaling yields v = /^D(^'m) = Q\r, s)oo with an operator Q on 7i°° which again can formally be obtained as polynomial in the positive modes of the Heisenberg algebra. Hence all correlation functions involving Q\r, s)^ also converge. This way, we can obtain a limit of the A-series of Virasoro minimal models whose correlation functions on Fl have the usual factorization properties. As a model case, in Lemma C.2 we also show by direct calculation that no diver- gences are introduced in Cd^p)^,Li\r,r)oo, \s',s)) when the singular vectors Li\r,r)oo are scaled up.

Example 4.8 As in Ex. 1.5 let C^, i € N, denote the CFT with central charge c = 1 that describes a boson compactified on a circle of radius Ru here with Ri := 1 + ^. See in particular (3.15) for notations. According to (B.7) - (B.9) the Verma l m n e module built on each \Q m,ni~$mtn)ii i ^> by the action of the Virasoro algebra is irreducible if (m, n) ^ (0,0) because all our R% are irrational. We can therefore define a direct system (Hz,fl) by

V(m,n)^ (0,0): j? where P denotes a polynomial in the Lk, £jr, k, k > 0. In the vacuum sector we use as in (3.35), where as usual a\, o^ denote the modes of the generators j, j of u(l) © u(l) in Cfy. One checks that this gives a convergent sequence CHl,f!-) of CFTs, but the direct limit /C°° possesses null vectors in W°°, where H°° = JC^/tf00. For example, i/i:=(4-(Li)2)|Qi,o;Öi,o>i. (3-61)

1 where for \Q\>o]Q\,o)i we have Q\o = Q ^ = ^7 ™ _^, and h{ = hi = •j-,1 -.a l^+ j, which gives a null vector v = /f0^*)- On the other hand, in Sect. 3.3.1 we have already constructed a fully con- vergent sequence (W, //) of CFTs via

80 with P as above. Now the limit is the su(2)i WZW model, i.e. a full fledged well-defined CFT. Note that in terms of the latter Fock space representation, v% in (3.61) is given by

Hence /f°(z/) ^ 0 in W°° = K°°. The direct system (H*, //) yields the vectors 2 (ai) |^; ^5)00, «217^; 7^5)00 as linearly independent elements of H™+i 1, where the combination ( -^ITT??; ^)°° differ by the null vector u and are thus identified in 7i°°i 1. However, the above directly implies how the ^+4'4 fl can be redefined by scaling up the additional null vectors, and then both limits give the same well-defined CFT. To approach the full limit structure obtained on the pre-Hilbert space Ti.°°, re- call that in the proof of Lemma 4.5 and in Rem. 4.7 we have argued that the correlation functions in Moo are adequately described in terms of the Coulomb- gas formalism. A closer study of this formalism also shows that it should be possible to represent the operator product algebra of the limit within the su(2)i WZW model42. Namely, as follows from performing the limit in (3.56), the operator corresponding to |r, s)^ in a given correlation function should be represented by a combination of the left-right symmetric u(l) vertex operator Vio__r^3..Q_r-s<.(z,~z) of the circle model CR~\ and the zero modes Q± of the 'w 1/2iW ~7T' holomorphic fields J±(z) which create \Q;Q) = | ± \/2;0) as in (B.10), along with their antiholomorphic counterparts.

3.4.2 Geometric interpretation of M(m, m + l)TO_s.0O Note that by (3.54) the limit .Moo of the sequence of unitary Virasoro minimal models has an infinite degeneracy of every energy level. This means that we cannot interpret .Moo as part of a well-defined CFT. However, the degeneration of the vacuum sector allows us to apply the techniques introduced in Sect. 3.2.2 and to find a geometric interpretation of the limit. Indeed, in Prop. 4.10 below we identify the algebra .A00 obtained from H°° by (3.59) with the algebra generated by the CHEBYSHEV POLYNOMIALS OF THE SECOND KIND, i.e. with the algebra of continuous functions on an interval: Lemma 4.9 th For every r € N — {0}, let Ur denote the r CHEBYSHEV POLYNOMIAL OF THE SECOND KIND; S Ur (cos x) := ^E!1} x e [0, TT] . (3.62) sin Ou 42This is in accord with [24, p. 655], where it is stated that the su(2)i WZW model "in some sense can be regarded as the limit c —> 1 of the discrete unitary series".

81 Then Ur(t = cos a:) is a polynomial of degree r — 1 in t G [—1,1], and the J7r(t) form an orthonormal system of polynomials with respect to the scalar product

(f,9)U~ f f(t)g(t)u,(t)dt, u,(t) := IVX^.. (3.63) J —1 Moreover, the Chebyshev polynomials of the second kind obey the recursion relation r+s-l U 3 64 Vr,seN-{O},Vte[-l,l]: Ur{t)Us(t) = Y, PW- ( - ) p=|r-s|+l, p+r+s=l(2)

The proof of Lemma 4.9 is a straightforward calculation, see e.g. [65, Problems 3.1.10(a)]. Note in particular that this lemma implies

oo

Vt e [-1,1], Vx € [0, TT]: Scosxit) = J2 Up{t)Up(cosx) f sinz. (3.65)

P'=i We are now in the position to give a geometric interpretation for our limit according to Def. 2.13: Proposition 4.10 The limit Mco of the sequence (Mm, fm) of unitary Virasoro minimal models has a geometric interpretation on the interval [0, TT] equipped with the dilaton- corrected metric g = 4y sin4a; dx dx and dilaton $ such that e"2*^ = ^ sin2a; for x € [0, TT]. Proof- As a first step, we need to construct a spectral pre-triple (M°°, H°°, A°°) from our limit M^ according to Def. 2.13. In fact, by Def. 2.9, M°° is given in (3.58), and .A00 is the associated zero-mode algebra specified in (3.59). Moreover, (3.50) shows that on H°°, according to Def. 2.13, we need to set

2 VreN-{0}: A? :=_lim_m (h£rt+ fc£rl) = ^, (3.66)

Comparison of (3.59) with (3.64) shows that .4°° agrees with the algebra gen- erated by the Chebyshev polynomials of the second kind. Here, similarly to the discussion of Chebyshev polynomials of the first kind at the end of Sect. 3.3.2, we view the Ur as functions x t—> Ur(cosx) with x € [0, ir\. There- fore, A°° can be identified with the algebra of smooth functions on [O,TT], and (3.63) shows that [0, re] is equipped with the dilaton-corrected metric g with 2 dvols = yjg{x)dx = ^s\n xdx as claimed. By the discussion in Sect. 3.1.1 it therefore remains to identify H°° in (3.66) with the generalized Laplacian H as

82 defined in (3.6) and to read off the dilaton #. To this end we use the characteri-

zation (3.5), that is, for all f,he C°°([0,7r]) we must have (/, 2Hh)u = (/', h')u. Since

(3 3) (f,2Hh)ul(f',h% = Jo

= "Jo r we deduce that 2H = — sin~2a;^ sin2x^, and thus g~ = dx® dx and e"2*^ = 2 2L ^ sin x. With (3.62) one now checks that HUr (cos x) = ^- Ur(cos x), in perfect agreement with (3.66). D

Remark 4.11 Metric and dilaton can also be obtained more directly from the action of H°° on .A00 as follows. As discussed above, as a topological space, M is determined by A°°, which by means of t : \r, r)^ »-» ([0, IT] 3 x H-+ Ur(cosx)) is isomorphic to C°°([0,7r]). Using the form

of the generalized Laplace operator (3.6) on [0, IT], from iH°°i * = A* one obtains the following differential equations

r2-1„ , , , &„ , , 1 /r2- 1. -Ur(cosx) = A®Ur(cosx) = -—- I UJcosx) det g \ 2 (rcosrx ,cosa:\ /cosa; „ _ 9 deto\\ I —: TT(7 (cos x)— — h 0 9 + ——x —— I \ SIM r sin x) \sina; X 4 det g ) ) for all r G N. Solving these equations for det "g and $ one easily obtains det 7j = 1 and e~2* = csin2 x, where the integration constant c = ^ can be determined by comparing the scalar products on H°° and C°°([0, TT]).

Remark 4.12 The distance functional, which is associated to the dilaton-corrected metric g = •^s sin4a; dx ® dx on the interval [0, IT] determined in Prop. 4.10, is

Vo,b€[0,7r]: d(a,&) = £|£(a)-£(&)| with &T) ~ 2r - sin(2r).

Here, ^(r/2) is the rc-coordinate of a regular cycloid in Cartesian coordinates. That is, if we consider a unit wheel which roles horizontally at unit speed, then 2nd(0,r/2) measures the distance that the point (2,0) on the wheel travels horizontally within the time r.

Remark 4.13 On the level of topological manifolds, our geometric interpretation of Moo on

83 an interval could have been predicted from the discussion in [42, §3.3]. Namely, the unitary Virasoro minimal model Mm can be obtained by an su(2)-coset construction: kA su(2)m-2esu(2)i su(2)m_i

In this language, the labels r and s in \r, s)m refer to the relevant representations of su(2)m_2 and su(2)m_i, respectively. Loosely speaking,'since only states with r = s enter in our zero-mode algebra, our geometric interpretation can be ex- pected to yield a semiclassical limit of the coset WZW model su(2)m/su(2)m as m —» oo. That is, by [42, (3.25)-(3.26)] the limit should have a geometric inter- pretation on the space SU(2)/Ad(SU(2)) = T/W with T the Cartan subgroup and W the Weyl group of SU(2). Indeed, with T = 17(1), W = Z2 we obtain T/W = [0, TT]. An analogous observation was already made in [91]. There, it was also pointed out that43 the geometric interpretation of M.^ on the interval fits nicely with an analysis of the qualitative Landau-Ginzburg description for the minimal models Mm [102]: As m —»• oo, the Landau-Ginzburg potential approaches a square well with walls at X = ±1, forcing the scalar field X of the Landau-Ginzburg theory to take values on the interval [—1,1]. Furthermore also metric and dilaton agree with the sigma model data pro- posed for general coset models in [42, Sects. 3.2, 3.3]. Namely, the metric g on the interval comes from the Killing metric on SU(2), and e~2* is the function on T/W which assigns to every point the volume of the respective SU(2)-conjugacy class. The sigma model metric and the dilaton, can also be obtained by a gauged WZW model construction as was done in [76] in the case of su(2)fc/u(l). Let us very briefly describe the steps and results of the calculations. As alluded to above the sigma model data of the Virasoro minimal models in the large level regime can be obtained from an SU(2)/Ad(SU(2))-gauged WZW model. The action of gauged WZW models after integrating out the gauge fields is given in [50, Eq. (2.8)]. After gauge fixing to T/W the action becomes the free action of the scalar field x parametrizing the interval T/W. In particular, we obtain a constant sigma model metric for this field. As explained e.g. in [97, Sect. 4.2] the dilaton is given by — ^ times the logarithm of the coefficient of the term quadratic in the gauge fields in the gauged WZW action [50, Eq. (2.3)]. The coefficient is easily calculated after gauge fixing to be proportional to sin2(:r), leading to e~2* ~ sin2(a:). Thus, the sigma model calculations confirm the results we obtained from the CFT-degeneration.

Remark 4.14 Apart from the direct limit construction studied above, one can introduce other sensible limits for the family Mm as m —» oo, similarly to Rem. 3.1. In partic- m ular, if there is a system of epimorphisms fm: H°° —> H such that all limits

(O\tpi{zi,Zi)...tpn(zn,Zn)\Q) := lim (0\fm(

according to J. Cardy

84 of n-point functions exist, then H°° can be interpreted as pre-Hilbert space of a limit theory M^. We believe that this is the structure underlying the ideas of [61, 90, 91]. Indeed, there the authors find a limiting pre-Hilbert space of the form ^ © H?;4,

where for h € E+ with 2y/h $ N, V^en denotes the generic representation of the Virasoro algebra Virc=i with character (B.7). Analogously to the situation in Rem. 3.1, no degeneration phenomena occur in this procedure, and the limit M» is conjectured to be part of a well-defined non-rational CFT with central charge c = 1, which has an interesting resemblance to Liouville theory. Evidence for this conjecture is given in [90], where in particular crossing symmetry is proven in some model cases. It seems that the two limits .Moo and Moo are complementary in many re- spects: For instance, the representation content of TC°° is complementary to the one we have found in 1i°°, see (3.54). Moreover, while the limit M^ seems to be a well-defined CFT, .Moo shows the degeneration phenomena discussed above, which allow to extract a geometric interpretation from the limit structures. A third approach to limiting processes is taken in [44]. There, limits of WZW models at infinite level are introduced by means of INVERSE LIMITS instead of direct limits. While our direct limit construction takes advantage of those structures which the pre-Hilbert spaces of minimal models Mm share at m ^> 0 and for sufficiently low conformal dimensions, the inverse limit construction of [44] allows to interpret the collection of fusion rings of g—WZW models as a category and to identify a projective system in it. Clearly, as mentioned above, we cannot view the family (.Mm)mGpj-{o,i} of minimal models as direct system of CFTs with the natural ordering induced by N. The same is true already on the level of g—WZW models; however, in [44] a suitable non-standard partial / ordering is found for the latter. Whether geometric interpretations of (A fm)m_>Oo with the expected properties arise from this construction remains to be seen. We have not worked out the details of an application of our techniques to g- WZW models at infinite level. However, we expect that the results of [42] should tie. in naturally thus leading to a direct limit construction with the expected geometric interpretation on the group manifold G. In fact this conjecture from a slightly different viewpoint has been discussed in [79]. The results of Prop. 4.10 and Rem. 4.13 imply that under the coordinate change t = cos a;, our limit .Moo has a geometric interpretation on the unit interval. By the ideas of [42] this also means that each unitary Virasoro minimal model Aim with m 3> 0 can be regarded as sigma model on the unit interval. We therefore expect to gain some insight44 into the shape of the D-branes in this bulk-geometry by considering the bulk-boundary couplings for m » 0. Recall that for each Mm we use the diagonal, that is the charge conjugation invariant partition function. Hence the Ishibashi states \p',p))m are labeled by 44 strictly speaking, after extending our constructions of Sect. 3.2 to the boundary sector

85 {p\ P) £ -A/m with Nm as in (3.49). Moreover, each (r, s) £ A/"m labels a boundary- condition. Its bulk-boundary coupling with respect to \p',p))m is given by

S _ (r,s)(p',P) {r's)

In order to investigate the geometry of the D-branes, we can restrict to the cou- plings of the bulk-fields (p', p1) which by Prop. 4.10 correspond to the Chebyshev polynomials Up> of the second kind. This means that we will focus on the bulk- boundary couplings Bfof) and the bulk-boundary coupling support functions m—X /("<)(*):- I (

In the above definition of fj£s\ we have introduced the appropriate pre-factor corresponding to the rescaling in (3.66) by hand. In order to analyze fJ^s\{t) for m ^> 0, we use t — cos x as before, and divide the domain of definition of x, the interval [O,TT], equidistantly. That is, we set

V(r,s)eAfm: xr:=^ % : Note the following useful reformulation of (3.62) for all p, r € N — {0}:

C/,-(cos(rCp))sin(a;p) = sin(rxp) = sin(pav) = J7p(cos(xr))sin(a;r), (3.68) and analogously for xp, xr. Using xr « xr for m ~^> 0, we therefore find:

^ sin(ray) sm(sxpi)

p'=l m— 1 (3^8) 2 V^ 7T / ^ Us(cos(xp>)) Jsm(xp>) si P'=I oo

y)) J7s(cos(xp'))

r+s—1 oo

p=|r-s|+l, () r+r+s—s 1 = E IE p=|r-a|+l, () r+s-1 (3.65)

p=|7—st+1, p+r+s=l(2)

86 We interpret this calculation in form of Remark 4.15 For the unitary Virasoro minimal models Mm at m > 0, the D-branes corre- sponding to stable boundary states labeled by (r, 1) which are elementary in the sense of [86] and the D-branes corresponding to the unstable boundary states (1, s) can be interpreted as being localized in the points t = cos(a;r) = cos(^) and t = cos(xs) = cos (^+j ) on the interval [—1,1], respectively. On the other hand, D-branes corresponding to the unstable boundary states (r, s) with r ^ 1, s/1 are supported on a union of these points. In view of Rem. 4.13 this is in accord with the general shape of D-branes in coset models [48, 41].

3.5 Discussion To conclude, let us address some open questions arising from our investigations. Of course, there are several interesting unsolved problems concerning the degen- erating limit .Moo of the A-series of unitary Virasoro minimal models of Sect. 3.4. For example, it would be interesting to gain more insight into the rep- resentation of this limit within the su(2)i WZW model, as mentioned at the end of Sect. 3.4.1. In particular, there are two fusion closed subsectors in .Moo, corresponding to the states |r, l)oo, r G N — {0}, and |1, .s)ooj s € N — {0}, re- spectively. We expect them to have a comparatively simple description in terms of the su(2)i WZW model, because no additional null vectors occur in the cor- responding Verma modules. Moreover, by acting with the zero mode algebra «4°° on one of these subsectors, one can generate the entire limit pre-Hilbert space H°°. Thus an understanding of these subsectors should also allow some insight into the geometry of the entire .A00 module H°°, for instance the fiber structure of the corresponding sheaf. Finally, one could try to extract the non- commutative geometries from the Virasoro minimal models at finite level which at infinite level reduce to the limit geometry on the interval determined in Prop. 4.10. Next, a generalization of our discussion in Sect. 3.4 to WZW models and their cosets in general would be nice, e.g. to the families of unitary super-Virasoro minimal models. More generally, for all limits of degenerating sequences of CFTs, it would be interesting to understand the compatibility of the limit structures with the action of the zero mode algebra .4°°. In particular, the limit OPE-constants are .4.°° homogeneous and therefore should be induced by a corresponding fiberwise structure on the sheaf with H°° as space of sections. It is likely that the entire limit can be understood in terms of such fiberwise structures together with the A°° action. This is in accord with the results of [72]. In fact, the zero mode algebra would be an interesting object to study in its own right, not least because there seems to be a relation to Zhu's algebra as mentioned in Sect. 3.1.2. Finally, it would be natural to extend our constructions to the boundary

87 sector. This could allow a more conceptual understanding of geometric interpre- tations of D-branes, for example in terms of the K-theory of .4°°.

88 A Properties of conformal field theories

In this Appendix, we collect some properties of CFTs that are used in the main text. Recall the Virasoro algebra Virc at central charge c, with generators

Ln, n G Z, •

3 Vm, n€Z: [Lm,Ln] = (n- m)Lm+n + ^(n - n)5m+nfi. (A.I)

In a given CFT C = (H, *, ft, T, T, C), the vacuum fl € H and its dual ft* G H* are characterized by

= l; Vn i-+ ip* of (3.10) can be explained by the relation between our OPE-coefficients C and the n-POINT FUNCTIONS

H®n9^i®---®^n H-» {0\Mzi>Zl)-~M*n,Zn)\0te (A-3) of a CFT. Here, E is a conformal surface, and the right hand side of (A.3) denotes a real analytic function En\Z) -* C outside the partial diagonals D = UijDij n with Dij :— {(zi,..., zn) G S | z\ = Zj}. Moreover, the right hand side of (A.3) possesses expansions around the partial diagonals Dij:

r T i+r,...;zn,zn) (zi-Zj) (zi-Zj) . (A.4)

Here, Rij C M? is countable without accumulation points, and only finitely many arr are non-zero for r + r < 0. Furthermore, the arr themselves are linear combinations of (n — l)-point functions with OPE-coemcients as linear factors. Finally, the right hand side of (A.3) is invariant under permutation of the tpi(zi, ~z,i). One says that the correlation functions constitute a REPRESENTATION OF THE OPE. It is a basic feature of CFTs that each state ip G "H possesses an ADJOINT ift G Ti.[x] such that two-point functions on the sphere E = CU{oo} = P1 encode the metric onTi.:

1 1 = lim n(0|^(«7- ,w- )x(C,C)|0>pi. (A.5)

Using conformal invariance one can determine ^(z,!:) as the image of *ip(z,~z) under the transformation /:ZH l/z, ~z i-» \j"z. In particular, if tp G H^ is real and QUASI-PRIMARY {e.g.

^(z-1,z-1) = v{z,z)z2hz2li. (A.6)

As an abbreviation, one defines IN- AND OUT-STATES by setting

6K: (VI == Em w—»0

\X) := limX(C,C)|0)Pi. (A.7)

89 Now the OPE-coefficients C can be recovered as

(A.8)

Similarly, with

They have the following expansion around z = 0:

«,?)|Vd) (A.9)

where {V'jjj denotes a suitable orthonormal basis of 7i. Using the above characterization of ip^, conformal invariance, and (A.6), one finds if

*^ = ^ are always real. Moreover, using (A.6) one shows

VnGZ: 4 = i-n; Vx^S«: (LnV)*X = V*(^-nX). (A.ll) Since up to possible phases, n-point functions (A.3) are invariant under per- mutations of the (Pi(zi,~Zi), the second and third arguments in C(-, •, •) can be interchanged, up to a phase and contributions of descendants to the OPE. How- ever, the characterization (3.11) of primaries together with (A.ll) ensures that every primary state is orthogonal to each descendant. Hence,

€n with tpew^.xe«^.s^€H^HnHV": , if, X) = (-ifx

To define MODES associated to each 9? G H, note that for all h, h, /j,, /I, the space *s nn^e dimensional by (3.8), so we can set

^p s- th-

If 9? 6 ^/T) then ^7^ obeys

90 In general, all three-point functions in a CFT can be obtained as linear combina- tions of three-point functions of the primaries, acted on by differential operators. For example, if tp G W^^, X € H^, V G H^, then and analogously for L\. On the other hand, analogously to (A.9), all n-point functions of a CFT can be recovered from its OPE-constants. This imposes many consistency conditions on the latter. An important example for this is CROSSING SYMMETRY (A.18) of four-point functions on the sphere. Before discussing crossing symmetry, let us introduce W-ALGEBRAS, since we will use them to rewrite (A.9) in a slightly different way. Namely, for ip G ker(Lo) and x € %hh' VßißX ^ ® implies (/i,/Z) = (n,0) with n G Z, and similarly for elements of ker(Lo) with /x, ß interchanged. The modes associated to states in ker(Lo), ker(L0) generate a HOLOMORPHIC or ANTIHOLOMORPHIC W-ALGEBRA W* D Virc, W D Vire defined by

W* := spanc {

and analogously for W or any subalgebra W of W* © W*. We suppose that H decomposes into a sum of tensor products of irreducible lowest weight represen- tations V^1*, Vß of the holomorphic and antiholomorphic W-algebras,

(a,ö)€X Moreover, the OPE determines the commutative associative product on the rep- resentation ring of W* W* which is known as FUSION:

for conformal families [pa] with f^}k&K^eK with K, ~K C ©pN denote a basis of the descendants of ißj, which is (Lo)-^o)-homogeneous, with bi-degree of ^k'k} given by (hj + \k\,hj + \k\), \k\, \k\ G N for all k G K, k G K. For a, b,j€N we set

Then, there are constants Pii^,]?^ } £ K, such that Vj EN,Vk€K,k<=K : (A.16) i ^ ?/> c

91 ()} Here, /?^ = ß^' := 1. Now, for all a,b,c,d,j € N the CONFORMAL BLOCKS axe given by r a ~\ 4 c A*) ==

Up to factors zhi~ha~hh ^zh)-hv-ht>^ the conformal blocks are (anti-)meromor- phic functions on C with poles at 0, 1, oo. They encode the four-point functions of primaries by

and CROSSING SYMMETRY reads: for all a, b, c, d € N

92 B c = 1 Representation theory

In this Appendix, let C = (H, *, fi, T, T, C) denote a unitary conformal field theory with c = 1. We recall some basic facts about its representation content; see also [45]. Since all known unitary conformal field theories at c = 1 can be constructed with energy momentum tensor T = \:jy. and j a u(l) current (which not necessarily is a field of the theory), it is convenient to use the Heisenberg algebra oo z n l K ) = Y] a>nz ~ , where [an,am] = m8n+mfi. (B.I)

Then all states in the pre-Hilbert space of every known theory C with central charge c = 1 are obtained from the Fock space that we construct from appropri- ate polynomials in the an,n > 0, acting on an appropriate subset of all lwvs of the Virasoro algebra. To build the latter it suffices to take states

\h, Q), such that LQ \h, Q) = h \h, Q), with h=^-, ao\h,Q) = Q\h,Q), (B.2) *(\h,Q)) = \h,-Q), as well as so-called twisted ground states with h = h < 1/16, which we will not make use of in the following, however. We will always normalize the \h, Q) such that C(\h,Q)\Cl, \h,Q» (3=0) (h, -Q \h, Q) = 1. (B.3) In a consistent theory, all left and right charges (Q; Q) are contained in a charge lattice. Namely, for every theory C there is a fixed R 6 R+ such that all (Q; Q) that may occur are given by

(Q;Ö) = 75(mÄ+E;mÄ-5s), m,n GZ. (B.4)

In a so-called CIRCLE THEORY AT RADIUS R, the pre-Hilbert space is just the entire Fock space built on the set of vacua \Q; Q) := %-,Q/ ® %-, Qj with all allowed values of (Q; Q). The su(2)i WZW-model is the circle theory at radius R = 1. All \Q; Q) are simple currents, and the leading terms in the OPE are given by

f r Q )*,\Q;Q)AQ ;Q')) = (-I^XQ'-Q')^ (B.5) with all other OPE-constants vanishing. Equivalently,

\Q;Q)m\Q';Q'} = e((Q;Q),(Q';Q')) \Q + Q';Q + Q')

iQ®iQ'Q')/2 ' (B.6) with notations as in (3.12). The COCYCLE FACTOR e introduces the appropriate phases.

93 For central charge c = 1, the character of a Virasoro irreducible representa- tion with lowest weight vector of dimension h generically is *r(9) = ^

n2\._ T/— 2-, T/ ' sn Pi>l, Ft (Pi+-+Pt)(n+1-Pi Pi) Pi+-+Pk=n+1 l~1

2 2 where l2^-) denotes the lowest weight vector of conformal weight ft= j,n6ff. Hence the character reduces to fcna/*-«(B+a)a/4)- (B.9) In the following, we restrict attention to the holomorphic side only. The generic W-algebra W of circle theories is generated by the u(l) current j. The %-,Q) are just the lowest weight vectors of irreducible representations VQ of W with characters X = x 3r regardless of the value of Q. In particular, if y/2Q = n 6 Z, by (B-9)

oo

fc=O and the Fock space built on ^-, Q) contains infinitely many Virasoro irreducible representations with lowest weight vectors \h,Q) ,h — ^- + N,N = k(\/2\Q\ + k), k

and let V[n)m] denote the space of states in the irreducible representation of the Virasoro algebra with lwv \[n, m]} of norm 1. Note that e.g. for the circle theory at R = 1 (the su(2)i WZW model) each positive eigenvalue of LQ is highly degenerate since this theory has an enhanced su(2)i Kac-Moody algebra the zero modes of whose generators commute with LQ. More precisely,

m——n,m=n{2)

All the representations V[nm] with \m\ < n, m = n(2) have the same character Xin2 as m (B-9)- Let J±(z) denote the holomorphic fields creating \Q;Q) = 4

| ±-\/2;0) as in (A.7). Then we define

Q± '•= / dzJ±(z), i.e. [Q+,<5-] = \/2ao =: 2Jo5 [JQ,Q±\ = 94 the zero modes of J±, J in the enhanced su(2)i Kac-Moody algebra of the circle model at radius R = 1. Since [Ln,Q±] = 0 for all n € Z, from (B.10) to- gether with (B.2) it follows that \h,Q) = KQ^ \h,Q± \ß) for some K € C* if \h, Q ± y/2} exists. More precisely, (B.10) inductively shows

if the left hand side does not vanish. Prom our normalization (B.3) it now follows that for m, I € N, ' |[n = m + 2/,m]> = \f^-Ql--|[n,n]>, and Q± |[n,±n]) = 0.

In particular, Q'_ |[n,n]) = 0 for I > n.

95 C Structure constants of the unitary Virasoro mini- mal models, and their c —> 1 limit

The unitary diagonal Virasoro minimal model M.m := M.(m,m + 1) with m € N — {0,1} has central charge Cm given by (3.48). Its irreducible representation (r, s) of the Virasoro algebra has an lwv \r, s}m with weight (3.50), and character

_£m. oo urn

h _ q ™,2k(m+l) + s) |1 < (C.I) Fusion reads

min{n'+s'— l,2m+1 —n'—s'} min{n+s—1,2m— 1 —n—s}

S',S) \JP Vyjy (p'lP)' (C.2) p'=|n'-s1+l, p=|n-s|+l, p'+n'+s's 1(2) p+n+s=1(2) The structure constants as in (3.55) are given by [30]

£r(p'p)

J'-2 r(s rs-s-t+y 8-l-i Tn-n-i+y n-l-i T -p- - +l+t) i=0 t yp

._a/_1_i+,i_w(s_l_j))r(„-n'-l-j+I'-»(»-l-i))r(p'-p-1-i+J'+yö»-

a a l n',n s',s Q(P',P) (C.3) with FT- 3/:-£> Zr-i^ + n-p + l), i':- \tf+n'-p

I'—l l-i I'—l l-l y\4(l'-l)(l-l) FT FT 1 TT r(i+iyO TT T(j-jy) i=lj=l i=l j=l i'—l I—1 / ' { V) 11 r(j.--j_jy') 11 r(^'—j+jy) > t=l j=l 1 1 1 "ry (*-J+V(I+J) Y "TT1 r(i+iyor(i-i-j/'(i+i)) "y^ ro'-jy)r(i-j+ j=l ^ ' i=l j=l y(i+3))

i=l r(l-i-ij/Or(t+j/'(l+ij) .^ T{n'-j+yj)T{j-n>+\-y{l+j)) •

r Note that fiiy, an/>n and C ^,'^ws/s^ are products of expressions G(N,M,e) := ffiff-ffi = (-1)^^(1 + AT - Me) ^ 7V + Me) !™1^

97 where N,M G Z and e G {y, ?/}. We also have the following expansions for m —> oo, to lowest order in y = y'+ 0(y2):

G(N,M,e) y~° ((- T(N+Me) V^O ( $ ifiV<0 ~ | if iV > 0 ' where sign(TV) = 1 for N > 0, sign(AT) = -1 for N < 0. Hence we obtain the lowest order expansions

^^

(C4)

max{n',n}' where

j-j/,l'-2,l-2), (C.5)

k(x, a, b) := d(x,a) + d(—x, b) — 2g(x, a, b), d(x,a) := max{min{a + l,a + 1 — 2x},— (a + 1)}

g(x,a,b) := (min{a - f ,6 + f } - ^ x), so A;(a;, a, 6) = \a — fe — x\ — \x\ fora, 6>—1. (C6) Moreover,

V— 2

= ^S^) n^-''+M'-l-«)e(n-n'+tln'-l-i)

e(p'_ p + ^ -p'- 1 - »}

e(n'- n + 1 + j - Z' -n + 1 + j) e(p - p'+ 1 + j - l',p + 1 + j)}

Thus in the limit m —+ oo we have

98 with

_ / min{n',n) min{s',s> max{p',p} \l'2 - 7(p',p) ',s) ~ \ max{n',n} max{s',s} min{p',p}) W-^n'.nXs'.s) ' p(p'>P) _ 17 ;/| , p(p'p) //-i o\ E{n',n)(s',s) ~ l'-'l + V,n)W ^C<8^

Note that ^j^'n)(s's) never vanishes in the allowed regime p'+ n'+ s' = p+n+s =

1(2), |nW - SW| < pW < nC) + 5W. These constants obey Lemma C.I 1 Given (p',p), (n\ n), (s , s) such that A^){s,s) + 0, we have E^){s,s) > 0. More precisely, with v := n'—n,cr := s'— s,TT := p'— p,

Proof- Since I'- l = l(a + u- TT), from (C.5), (C.6), (C.8) we find

-\cr\ - \v\ - |TT| = max{|cr + z/|, |TT|} + max{|<7 — v\, |TT|} — \a\ — \u\ — \K\.

Therefore,

if |7r| < min{| 0, if |TT| > max{|cr + v\, \a — v\}, which proves the lemma. D In Rem. 4.7 we explain how additional null vectors in the limit .Moo of unitary Virasoro minimal models can be scaled up without introducing divergences in three-point functions. In fact, Lemma C.I can be used in order to extend the example of scaling up null vectors given in [61, Sect. 3.1.1] by a direct calculation:

Lemma C.2 All vectors L\\r,r)^, r > 1, can be scaled up to non-vanishing norm without / introducing divergences in the OPE-constants C(|p ,p)Jo,Li|r)r)oo, \s\ s)^). Proof: By (3.60), a normalization of L>i\r,r)oo to non-vanishing but finite norm is given by jD™rl:= lim (m + 1) Li|r,r)m, 771—»OO

99 i.e. we set 75 (nm ,) •= Dj , Note that for finite m, (C.2) shows that w^L^ is only non-vanishing if \{r + sW — 1 — pW) G {0,..., min{r, sW} — 1}, hence we restrict to such p, p'. By (A. 14) we find

(hm hm hm \ ^(p'p) ^ r

~ (171 •

Therefore, if E,'p), , >, > 1, the assertion follows directly from the convergence \r,r)(S,s) ^ of each term in the latter expression. On the other hand, for p', p in the range given above, by Lemma C.I we have Ef'K, , s = 0 iff \p'— p\ = \s'— s\. Hence in this case

(

remains finite, too.

100 References

[1] L. ALVAREZ-GAU ME, G. SIERRA, AND C. GOMEZ, Topics in conformal field theory, in Physics and mathematics of strings, World Sei. Publishing, Teaneck, NJ, 1990, pp. 16-184. [2] P. ASPINWALL AND D. MORRISON, String theory on K3 surfaces, in Mir- ror symmetry, B. Greene and S. Yau, eds., vol. II, 1994, pp. 703-716, hep-th/9404151.

[3] P. S. ASPINWALL, B. R. GREENE, AND D. R. MORRISON, Calabi-Yau moduli space, mirror manifolds and spacetime topology change in string theory, Nucl. Phys., B416 (1994), pp. 414-480, hep-th/9309097.

[4] I. BARS, Ghost - free spectrum of a quantum string in SL(2, R) curved space-time, Phys. Rev., D53 (1996), pp. 3308-3323, hep-th/9503205.

[5] I. BARS AND D. NEMESCHANSKY, String propagation in backgrounds with curved space-time, Nucl. Phys., B348 (1991), pp. 89-107.

[6] I. BARS AND K. SFETSOS, Generalized duality and singular strings in higher dimensions, Mod. Phys. Lett., A7 (1992), pp. 1091-1104, hep-th/9110054.

[7] A. A. BELAVIN, A. M. POLYAKOV, AND A. B. ZAMOLODCHIKOV, Infinite conformal symmetry in two-dimensional quantum field theory, Nucl. Phys., B241 (1984), pp. 333-380.

[8] N. BERLINE, E. GETZLER, AND M. VERGNE, Heat kernels and Dirac operators, Springer-Verlag, Berlin Heidelberg New York, 1992. [9] N. BOURBAKI, Elements de mathematique. Theorie des ensembles, Her- mann, Paris, 1970. [10] P. BOWCOCK, Canonical quantization of the gauged Wess-Zumino model, Nucl. Phys., B316 (1989), p. 80.

[11] D. BRUNGS AND W. NAHM, The associative algebras of conformal field theory, Lett. Math. Phys., 47 (1999), pp. 379-383, hep-th/9811239. [12] T. H. BUSCHER, A symmetry of the string background field equations, Phys. Lett., B194 (1987), p. 59.

[13] A. CAPPELLI, C. ITZYKSON, AND J. B. ZUBER, Modular invariant parti- tion functions in two dimensions, Nucl. Phys., B280 (1987), pp. 445-465. [14] , The ADE classification of minimal and A\ ' conformal invariant theories, Commun. Math. Phys., 113 (1987), pp. 1-26.

[15] A. CASHER, F. ENGLERT, H. NICOLAI, AND A. TAORMINA, Consistent superstrings as solutions of the d = 26 bosonic string theory, Phys. Lett., B162 (1985), p. 121.

101 [16] S. CHAUDHURI AND J. A. SCHWARTZ, A criterion for integrably marginal operators, Phys. Lett., B219 (1989), p. 291.

[17] J. CHEEGER AND M. GROMOV, Collapsing Riemannian manifolds while keeping their curvature bounded. I, J. of Diff. Geometry, 23 (1986), pp. 309-364.

[18] , Collapsing Riemannian manifolds while keeping their curvature bounded. II, J. of Diff. Geometry, 32 (1990), pp. 269-298.

[19] A. CONNES, Noncommutative differential geometry, Inst. Hautes Etudes Sei. Publ. Math., (1985), pp. 257-360.

[20] , Geometrie non commutative, InterEditions, 1990.

[21] A. CONNES, Gravity coupled with matter and the foundation of non- commutative geometry, Commun. Math. Phys., 182 (1996), pp. 155-176, hep-th/9603053.

[22] R. DlJKGRAAF, C. VAPA, E. VERLINDE, AND H. VERLINDE, The operator algebra of orbifold models, Commun. Math. Phys., 123 (1989), p. 485.

[23] R. DIJKGRAAF, E. VERLINDE, AND H. VERLINDE, On moduli spaces of conformal field theories with C > 1, In Copenhagen 1987, Proceedings, Perspectives in String Theory 117-137.

[24] R. DIJKGRAAF, E. VERLINDE, AND H. VERLINDE, c = 1 conformal field theories on Riemann surfaces, Commun. Math. Phys., 115 (1988), pp. 649-690.

[25] L. J. DIXON, D. FRIEDAN, E. J. MARTINEC, AND S. H. SHENKER, The conformal field theory of orbifolds, Nucl. Phys., B282 (1987), pp. 13-73.

[26] L. J. DIXON, J. A. HARVEY, C. VAFA, AND E. WITTEN, Strings on orbifolds. 2, Nucl. Phys., B274 (1986), pp. 285-314.

[27] A. DOLD, Lectures on algebraic topology, vol. 200 of Die Grundlehren der mathematischen Wissenschaften, Berlin-Heidelberg-New York: Springer- Verlag, 1972.

[28] V. S. DOTSENKO AND V. A. FATEEV, Conformal algebra and multipoint correlation functions in 2d statistical models, Nucl. Phys., B240 (1984), p. 312.

[29] , Four point correlation functions and the operator algebra in the two dimensional conformal invariant theories with the central charge C < 1, Nucl. Phys., B251 (1985), p. 691.

[30] , Operator algebra of two-dimensional conformal theories with central charge c < 1, Phys. Lett., B154 (1985), pp. 291-295.

102 [31] S. ELITZUR, A. GIVBON, D. KUTASOV, AND E. RABINOVICI, From big bang to big crunch and beyond, JHEP, 06 (2002), p. 017, hep-th/0204189.

[32] S. ELITZUR, A. GIVEON, AND E. RABINOVICI, Removing singularities, JHEP, 01 (2003), p. 017, hep-th/0212242.

[33] B. FEIGIN AND D. FUKS, MOSCOW preprint, (1983).

[34] G. FELDER, BRST approach to minimal models, Nucl. Phys., B317 (1989), p. 215. [35] , Erratum: BRST approach to minimal models, Nucl. Phys., B317 (1989), p. 548. [36] S. FORSTE, A truly marginal deformation ofSL(2,R) in a null direction, Phys. Lett., B338 (1994), pp. 36-39, nep-th/9407198. [37] , D-branes in a marginally deformed WZW model, in Proceedings of the 35th International Symposium Ahrenshoop on the theory of Ele- mentary Particles: Recent Developments in String / M Theory and Field Theory, Berlin, Germany, 26-30 Aug 2002, 2002, hep-th/0212199. [38] , D-branes on a deformation of SU(2), JHEP, 02 (2002), p. 022, hep-th/0112193.

[39] S. FORSTE AND D. ROGGENKAMP, Current current deformations of conformal field theories, and WZW models, JHEP, 05 (2003), p. 071, hep-tn/0304234.

[40] P. D. FRANCESCO, P. MATHIEU, AND D. SENECHAL, Conformal field theory, Graduate Texts in Contemporary Physics, Springer-Verlag, New York Berlin Heidelberg Barcelona Hong Kong London Milan Paris Singa- pore Tokyo, 1996.

[41] S. FREDENHAGEN AND V. SCHOMERUS, D-branes in coset models, JHEP, 02 (2002), p. 005, hep-th/0111189.

[42] J. FRÖHLICH AND K. GAWEDZKI, Conformal field theory and geometry of strings, in Mathematical quantum theory. I. Field theory and many-body theory (Vancouver, BC, 1993), Amer. Math. Soc, Providence, RI, 1994, pp. 57-97, hep-th/9310187.

[43] J. FRÖHLICH, O. GRANDJEAN, AND A. RECKNAGEL, Supersymme- tric quantum theory, non-commutative geometry, and gravitation, in Symetries quantiques (Les Houches, 1995), North-Holland, Amsterdam, 1998, pp. 221-385, hep-th/9706132.

[44] J. FUCHS AND C. SCHWEIGERT, WZW fusion rings in the limit of infinite level, Commun. Math. Phys., 185 (1997), pp. 641-670, hep-th/9609124.

103 [45] M. GABERDIEL, D-branes from conformal field theory, in Proceedings of the Workshop on the Quantum Structure of Spacetime and the Geometric Nature of Fundamental Interactions, Corfu, Greece, 13-20 September 2001, hep-th/0108044.

[46] M. R. GABERDIEL AND P. GODDARD, Axiomatic conformal field theory, Commun. Math. Phys., 209 (2000), pp. 549-594, hep-th/9810019.

[47] M. R. GABERDIEL AND A. NEITZKE, Rationality, quasirationality and finite W-algebras, Commun. Math. Phys., 238 (2003), pp. 305-331, hep-th/0009235. [48] K. GAWEDZKI, Boundary WZW, G/H, G/G and CS theories, Annales Henri Poincare, 3 (2002), pp. 847-881, hep-th/0108044.

[49] K. GAWEDZKI AND A. KUPIAINEN, Coset construction from functional integrals, Nucl. Phys., B320 (1989), p. 625. [50] , Coset construction from functional integrals, Nucl. Phys., B320 (1989), p. 625.

[51] D. GEPNER, New conformal field theories associated with Lie algebras and their partition functions, Nucl. Phys., B290 (1987), p. 10. [52] , Field identification in coset conformal field theories, Phys. Lett., B222 (1989), p. 207.

[53] D. GEPNER AND Z. A. QiU, Modular invariant partition functions for parafermionic field theories, Nucl. Phys., B285 (1987), p. 423.

[54] D. GEPNER AND E. WITTEN, String theory on group manifolds, Nucl. Phys., B278 (1986), p. 493. [55] D. GERSHON, Exact 0{d,d) transformations in WZW models, Phys. Rev., D50 (1994), pp. 6481-6489, hep-th/9312154. [56] P. GlNSPARG, Applied conformal field theory, in Lectures given at the Les Houches Summer School in Theoretical Physics 1988 (Les Houches, France), pp. 1-168, hep-th/9108028.

[57] P. H. GINSPARG AND F. QUEVEDO, Strings on curved space-times: Black holes, torsion, and duality, Nucl. Phys., B385 (1992), pp. 527-557, hep-th/9202092.

[58] A. GIVEON AND E. KlRITSIS, Axial vector duality as a gauge symmetry and topology change in string theory, Nucl. Phys., B411 (1994), pp. 487- 508, hep-th/9303016.

[59] A. GIVEON AND E. WITTEN, Mirror symmetry as a gauge symmetry, Phys. Lett., B332 (1994), pp. 44-50, hep-th/9404184.

104 [60] P. GODDARD, A. KENT, AND D. I. OLIVE, Virasoro algebras and coset space models, Phys. Lett., B152 (1985), p. 88.

[61] K. GRAHAM, I. RUNKEL, AND G. M. T. WATTS, Minimal model boundary flows and c = 1 eft, Nucl. Phys., B608 (2001), pp. 527-556, hep-th/0101187.

[62] M. GROSS, Topological mirror symmetry, Invent. Math., 144 (2001), pp. 75-137, math.ag/9909015.

[63] S. F. HASSAN AND A. SEN, Marginal deformations of WZNW and coset models from 0{d,d) transformation, Nucl. Phys., B405 (1993), pp. 143- 165, hep-th/9210121.

[64] M. HENNINGSON AND C. R. NAPPI, Duality, marginal perturbations and gauging, Phys. Rev., D48 (1993), pp. 861-868, hep-th/9301005. [65] P. HENRIci, Essentials of numerical analysis with pocket calculator demonstrations, John Wiley & Sons Inc., New York, 1982. [66] V. G. KAC, Infinite dimensional Lie algebras. Cambridge, UK: Univ. Pr. (1990) 400 p. [67] V. G. KAC AND D. H. PETERSON, Infinite dimensional Lie algebras, theta functions and modular forms, Adv. Math., 53 (1984), pp. 125-264.

[68] L. KADANOFF, Multicritical behaviour at the Kosterlitz-Thouless critical point, Ann. Physics, 120 (1979), pp. 39-71.

[69] Y. KAZAMA AND H. SUZUKI, Bosonic construction of conformal field the- ories with extended super symmetry, Mod. Phys. Lett., A4 (1989), p. 235. [70] E. KlRITSIS, Exact duality symmetries in CFT and string theory, Nucl. Phys., B405 (1993), pp. 109-142, hep-th/9302033. [71] E. B. KlRITSlS, Duality in gauged WZW models, Mod. Phys. Lett., A6 (1991), pp. 2871-2880. [72] M. KONTSEVICH AND Y. SoiBELMAN, Homological mirror symmetry and torus fibrations, in Symplectic geometry and mirror symmetry (Seoul, 2000), World Sei. Publishing, River Edge, NJ, 2001, pp. 203-263, math.SG/0011041.

[73] D. KUTASOV, Geometry on the space of conformal field theories and con- tact terms, Phys. Lett., B220 (1989), p. 153. [74] H. Liu, G. MOORE, AND N. SEIBERG, Strings in a time-dependent orb- ifold, JHEP, 06 (2002), p. 045, hep-th/0204168. [75] S. LORD, Riemannian geometries, (2000), math-ph/0010037.

105 [76] J. M. MALDACENA, G. W. MOORE, AND N. SEIBERG, Geometrical in- terpretation ofD-branes in gauged WZW models, JHEP, 07 (2001), p. 046, hep-tn/0105038. [77] R. MANVELYAN, On marginal deformation of wznw model and PP-wave limit of deformed AdS(3) x S(3) string geometry, Mod. Phys. Lett., A18 (2003), pp. 1531-1538, hep-th/0206218.

[78] G. W. MOORE AND N. SEIBERG, Classical and quantum conformal field theory, Commun. Math. Phys., 123 (1989), p. 177. [79] , Classical and quantum conformal field theory, Commun. Math. Phys., 123 (1989), p. 177. [80] , Naturality in conformal field theory, Nucl. Phys., B313 (1989), p. 16. [81] D. MORRISON, Where is the large radius limit?, in Proceedings of Strings '93, Berkeley, CA, USA, May 24-29, 1993, M. H. et al., ed., Singapore: World Scientific, pp. 311-315, hep-th/9311049.

[82] W. NAHM, On quasi-rational conformal field theories, Nucl. Phys. Proc. Suppl., 49 (1996), pp. 107-114.

[83] K. S. NARAIN, New heterotic string theories in uncompactified dimensions < 10, Phys. Lett., B169 (1986), p. 41.

[84] K. RANGANATHAN, Nearby CFTs in the operator formalism: The role of a connection, Nucl. Phys., B408 (1993), pp. 180-206, hep-th/9210090.

[85] K. RANGANATHAN, H. SONODA, AND B. ZWIEBACH, Connections on the state space over conformal field theories, Nucl. Phys., B414 (1994), pp.405-460, hep-th/9304053.

[86] A. RECKNAGEL, D. ROGGENKAMP, AND V. SCHOMERUS, On relevant boundary perturbations of unitary minimal models, Nucl. Phys., B588 (2000), pp. 552-564, hep-th/0003110.

[87] A. RENNIE, Commutative geometries are spin manifolds, Rev. Math. Phys., 13 (2001), pp. 409-464.

[88] M. ROCEK AND E. VERLINDE, Duality, quotients, and currents, Nucl. Phys., B373 (1992), pp. 630-646, hep-th/9110053.

[89] D. ROGGENKAMP AND K. WENDLAND, Limits and degenerations of unitary conformal field theories, (2003), hep-th/0308143, to appear in Comm. Math. Phys.

[90] I. RUNKEL AND G. M. T. WATTS, A non-rational CFT with c = 1 as a limit of minimal models, JHEP, 09 (2001), p. 006, hep-th/0107118. [91] , A non-rational CFT with central charge 1, Fortsch. Phys., 50 (2002), pp. 959-965, hep-th/0201231.

106 [92] A. N. SCHELLEKENS AND S. YANKIELOWICZ, Simple currents, modular invariants and fixed points, Int. J. Mod. Phys., A5 (1990), pp. 2903-2952.

[93] J. SCHWINGER, The theory of quantized fields. II, in Selected papers on quantum electrodynamics, J. Schwinger, ed., Dover publications Inc., 1958, pp. 356-371.

[94] K. SFETSOS AND A. A. TSEYTLIN, Antisymmetric tensor coupling and conformal invariance in sigma models corresponding to gauged WZNW theories, Phys. Rev., D49 (1994), pp. 2933-2956, nep-th/9310159.

[95] A. STROMINGER, S.-T. YAU, AND E. ZASLOW, Mirror symmetry is T- duality, Nucl. Phys., B479 (1996), pp. 243-259, hep-th/9606040.

[96] A. A. TSEYTLIN, Sigma models and renormalization of string loops, Lec- tures given at 1989 Trieste Spring School on Superstrings, Trieste, Italy, Apr 3-14, 1989. [97] , Effective action of gauged wzw model and exact string solutions, Nucl. Phys., B399 (1993), pp. 601-622, hep-th/9301015. [98] , Conformal sigma models corresponding to gauged Wess-Zumino- Witten theories, Nucl. Phys., B411 (1994), pp. 509-558, hep-th/9302083. [99] , On a 'universal' class of WZW type conformal models, Nucl. Phys., B418 (1994), pp. 173-194, hep-th/9311062.

[100] C. VAFA AND E. WlTTEN, On orbifolds with discrete torsion, J. Geom. Phys., 15 (1995), pp. 189-214, hep-th/9409188. [101] S.-K. YANG, Marginal deformation of minimal N = 2 superconformal field theories and the Wüten index, Phys. Lett., B209 (1988), p. 242. [102] A. B. ZAMOLODCHIKOV, Conformal symmetry and multicritical points in two- dimensional quantum field theory. (In Russian), Sov. J. Nucl. Phys., 44 (1986), pp. 529-533. [103] , Renormalization group and perturbation theory near fixed points in two-dimensional field theory, Sov. J. Nucl. Phys., 46 (1987), p. 1090. [104] Y. ZHU, Modular invariance of characters of vertex operator algebras, J. Amer. Math. Soc, 9 (1996), pp. 237-302.

107