Global Nalysis and Its a Pplications (Extended Abstract Book)
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Atiyah, M.F. 1. Geometry of Yang-Mills Fields, Lezioni Fermiani, Pisa 1979 2
BIBLIOGRAPHY Atiyah, M.F. 1. Geometry of Yang-Mills fields, Lezioni Fermiani, Pisa 1979 2. Green's functions for seH-dual four manifolds, Adv. in Math. 7 A (1981) 130-158 Atiyah, M. F., Drin'feld, V.G., Hitchin, N. J. 3. Construction of instantons, Phys. Lett. 65A (1978) 185-187 Atiyah, MF., Hitchin, N.J., Singer, I.M. 4. SeH-duality in four-dimensional Riemannian geometry, Proc. Roy. Soc. Lon don 362 (1978), 425-461 Atiyah, M. F., Jones, J. S. 5. Topological aspects of Yang-Mills theory, Comm. Math. Phys. 61 (1978), 97-118 Atiyah, M.F., Ward, R.S. 6. Instantons and algebraic geometry, Comm. Math. Phys. 55 (1977), 117-124 Barth, W. 7. Moduli of vector bundles on the projective plane, Invent. Math 42 (1977), 63-91 Barth, W., Hulek, K. 8. Monads 8.lJ.d moduli of vector bundles, manuscripta math. 25 (1978),323- 347 Beilinson, A. A. 9. Coherent sheaves on pn and problems in linear algebra, Funct. Anal. Appl. 12 (1978), 214-216 Beilinson, A. A., Gel'fand, S. I, Manin, Yu. I. 10. An instanton is determined by its complex singularlties, Funct. Anal. Appl. 14 (1980), 118-119 Belavin, A. A., Polyakov, A. M., Schwartz, A. S., Tyupkin, Yu. 11. Pseudo-particle solutions of the Yang-Mills equations, Phys. Lett. 59B (1975), 85-87 288 Bibliography Belavin, A. A., Zakharov, V. E. 12. Multidimensional method of the inverse scattering problem and duality equations for the Yang-Mills field, JETP Letters 25 (1977), 567-570 Berezin, F. A. 13. The mathematical basis of supersymmetrie field theories, Sov. -
Twistor Theory and Differential Equations
IOP PUBLISHING JOURNAL OF PHYSICS A: MATHEMATICAL AND THEORETICAL J. Phys. A: Math. Theor. 42 (2009) 404004 (19pp) doi:10.1088/1751-8113/42/40/404004 Twistor theory and differential equations Maciej Dunajski Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK E-mail: [email protected] Received 31 January 2009, in final form 17 March 2009 Published 16 September 2009 Online at stacks.iop.org/JPhysA/42/404004 Abstract This is an elementary and self-contained review of twistor theory as a geometric tool for solving nonlinear differential equations. Solutions to soliton equations such as KdV,Tzitzeica, integrable chiral model, BPS monopole or Sine–Gordon arise from holomorphic vector bundles over T CP1. A different framework is provided for the dispersionless analogues of soliton equations, such as dispersionless KP or SU(∞) Toda system in 2+1 dimensions. Their solutions correspond to deformations of (parts of) T CP1, and ultimately to Einstein– Weyl curved geometries generalizing the flat Minkowski space. A number of exercises are included and the necessary facts about vector bundles over the Riemann sphere are summarized in the appendix. PACS number: 02.30.Ik (Some figures in this article are in colour only in the electronic version) 1. Introduction Twistor theory was created by Penrose [19] in 1967. The original motivation was to unify general relativity and quantum mechanics in a non-local theory based on complex numbers. The application of twistor theory to differential equations and integrability has been an unexpected spin off from the twistor programme. -
The Language of Differential Forms
Appendix A The Language of Differential Forms This appendix—with the only exception of Sect.A.4.2—does not contain any new physical notions with respect to the previous chapters, but has the purpose of deriving and rewriting some of the previous results using a different language: the language of the so-called differential (or exterior) forms. Thanks to this language we can rewrite all equations in a more compact form, where all tensor indices referred to the diffeomorphisms of the curved space–time are “hidden” inside the variables, with great formal simplifications and benefits (especially in the context of the variational computations). The matter of this appendix is not intended to provide a complete nor a rigorous introduction to this formalism: it should be regarded only as a first, intuitive and oper- ational approach to the calculus of differential forms (also called exterior calculus, or “Cartan calculus”). The main purpose is to quickly put the reader in the position of understanding, and also independently performing, various computations typical of a geometric model of gravity. The readers interested in a more rigorous discussion of differential forms are referred, for instance, to the book [22] of the bibliography. Let us finally notice that in this appendix we will follow the conventions introduced in Chap. 12, Sect. 12.1: latin letters a, b, c,...will denote Lorentz indices in the flat tangent space, Greek letters μ, ν, α,... tensor indices in the curved manifold. For the matter fields we will always use natural units = c = 1. Also, unless otherwise stated, in the first three Sects. -
Twistor Theory 1St Edition Free Download
FREE TWISTOR THEORY 1ST EDITION PDF Stephen Huggett | 9781351406550 | | | | | String Theory and Twistor Theory - dummies This book is an introduction to twistor theory and modern geometrical approaches to space-time structure at the graduate or advanced undergraduate level. The choice of material presented has evolved from graduate lectures given in London and Oxford and the authors have aimed to retain the informal tone of those lectures. The book will provide graduate students with an introduction to the literature of twistor theory, presupposing some knowledge of special relativity and differential geometry. It would also be of use for a short course on space-time structure independently of twistor theory. The physicist could be introduced gently to some of the mathematics Twistor Theory 1st edition has proved useful in these areas, and the mathematician could be shown where sheaf cohomology and complex manifold theory can be used in physics. Previous page. Roger Penrose. Robert J. Jakob Schwichtenberg. Physics from Finance: A gentle introduction to gauge theories, fundamental interactions and fiber bundles. Next page. Burstall, Contemporary Physics. I believe that spinors and twistors are very important and that they reveal clearly profound structure that is not easily noticed using other formalisms. There can be no doubt that Sir Roger Penrose has been the leading exponent of this line of thinking for a long, long time. His book, Spinors and Spacetime is indispensable and a great classic, but it isn't Twistor Theory 1st edition the easiest book to read. In particular, I've spent a lot of time sorting through Twistor Theory 1st edition first chapter, trying to see clearly just what a Twistor Theory 1st edition "really is. -
JHEP10(2020)127 Springer July 4, 2020 : October 20, 2020 : September 22, 2020 : Boundary Action
Published for SISSA by Springer Received: July 4, 2020 Accepted: September 22, 2020 Published: October 20, 2020 Higher-spin symmetry vs. boundary locality, and a JHEP10(2020)127 rehabilitation of dS/CFT Adrian David and Yasha Neiman Okinawa Institute of Science and Technology, 1919-1 Tancha, Onna-son, Okinawa 904-0495, Japan E-mail: [email protected], [email protected] Abstract: We consider the holographic duality between 4d type-A higher-spin gravity and a 3d free vector model. It is known that the Feynman diagrams for boundary correlators can be encapsulated in an HS-algebraic twistorial expression. This expression can be evaluated not just on separate boundary insertions, but on entire finite source distributions. We do so for the first time, and find that the result ZHS disagrees with the usual CFT partition function. While such disagreement was expected due to contact corrections, it persists even in their absence. We ascribe it to a confusion between on-shell and off-shell boundary calculations. In Lorentzian boundary signature, this manifests via wrong relative signs for Feynman diagrams with different permutations of the source points. In Euclidean, the signs are instead ambiguous, spoiling would-be linear superpositions. Framing the situation as a conflict between boundary locality and HS symmetry, we sacrifice locality and choose to take ZHS seriously. We are rewarded by the dissolution of a long-standing pathology in higher-spin dS/CFT. Though we lose the connection to the local CFT, the precise form of ZHS can be recovered from first principles, by demanding a spin-local boundary action. -
The Extended Relativity Theory in Clifford Spaces
THE EXTENDED RELATIVITY THEORY IN CLIFFORD SPACES C. Castroa and M. Pav·si·cb May 21, 2004 aCenter for Theoretical Studies of Physical Systems, Clark Atlanta University, Atlanta bJo·zef Stefan Institute, Jamova 39, SI-1000 Ljubljana, Slovenia; Email: [email protected] Abstract A brief review of some of the most important features of the Extended Rela- tivity theory in Cli®ord-spaces (C-spaces) is presented whose " point" coordinates are noncommuting Cli®ord-valued quantities and which incorporate the lines, ar- eas, volumes,.... degrees of freedom associated with the collective particle, string, membrane,... dynamics of p-loops (closed p-branes) living in target D-dimensional spacetime backgrounds. C-space Relativity naturally incorporates the ideas of an invariant length (Planck scale), maximal acceleration, noncommuting coordinates, supersymmetry, holography, higher derivative gravity with torsion and variable di- mensions/signatures that allows to study the dynamics of all (closed) p-branes, for all values of p, on a uni¯ed footing. It resolves the ordering ambiguities in QFT and the problem of time in Cosmology. A discussion of the maximal-acceleration Rela- tivity principle in phase-spaces follows along with the study of the invariance group of symmetry transformations in phase-space that allows to show why Planck areas are invariant under acceleration-boosts transformations and which seems to suggest that a maximal-string tension principle may be operating in Nature. We continue by pointing out how the relativity of signatures of the underlying n-dimensional spacetime results from taking di®erent n-dimensional slices through C-space. The conformal group emerges as a natural subgroup of the Cli®ord group and Relativity in C-spaces involves natural scale changes in the sizes of physical objects without the introduction of forces nor Weyl's gauge ¯eld of dilations. -
Spacetime Structuralism
Philosophy and Foundations of Physics 37 The Ontology of Spacetime D. Dieks (Editor) r 2006 Elsevier B.V. All rights reserved DOI 10.1016/S1871-1774(06)01003-5 Chapter 3 Spacetime Structuralism Jonathan Bain Humanities and Social Sciences, Polytechnic University, Brooklyn, NY 11201, USA Abstract In this essay, I consider the ontological status of spacetime from the points of view of the standard tensor formalism and three alternatives: twistor theory, Einstein algebras, and geometric algebra. I briefly review how classical field theories can be formulated in each of these formalisms, and indicate how this suggests a structural realist interpre- tation of spacetime. 1. Introduction This essay is concerned with the following question: If it is possible to do classical field theory without a 4-dimensional differentiable manifold, what does this suggest about the ontological status of spacetime from the point of view of a semantic realist? In Section 2, I indicate why a semantic realist would want to do classical field theory without a manifold. In Sections 3–5, I indicate the extent to which such a feat is possible. Finally, in Section 6, I indicate the type of spacetime realism this feat suggests. 2. Manifolds and manifold substantivalism In classical field theories presented in the standard tensor formalism, spacetime is represented by a differentiable manifold M and physical fields are represented by tensor fields that quantify over the points of M. To some authors, this has 38 J. Bain suggested an ontological commitment to spacetime points (e.g., Field, 1989; Earman, 1989). This inclination might be seen as being motivated by a general semantic realist desire to take successful theories at their face value, a desire for a literal interpretation of the claims such theories make (Earman, 1993; Horwich, 1982). -
The Penrose Transform for Einstein-Weyl and Related Spaces
The Penrose Transform for Einstein-Weyl and Related Spaces Cheng-chih Tsai PhD Edinburgh University 1996 r Abstract A holomorphic Penrose transform is described for Hitchin's correspondence between complex Einstein-Weyl spaces and "minitwistor" spaces, leading to isomorphisms between the sheaf cohomologies of holomorphic line bundles on a minitwistor space and the solution spaces of some conformally invariant field equations on the corresponding Einstein-Weyl space. The Penrose transforms for complex Euclidean 3-space and complex hyperbolic 3-space, two examples which have preferred Riemannian metrics, are explicitly discussed before the treatment of the general case. The non-holomorphic Penrose transform of Bailey, Eastwood and Singer, which translates holomorphic data on a complex manifold to data on a smooth mani- fold, using the notion of involutive cohomology, is reviewed and applied to the non-holomorphic twistor correspondences of four homogeneous spaces: Euclidean 3-space, hyperbolic 3-space, Euclidean 5-space (considered as the space of trace- free symmetric 3 x 3 matrices) and the space of non-degenerate real conics in complex projective plane. The complexified holomorphic twistor correspondences of the last two cases turn out to be examples of a more general correspondence between complex surfaces with rational curves of self-intersection number 4 and their moduli spaces. Declaration I hereby declare that the thesis is composed by me and is my own work. 111 Acknowledgments I would like to thank my supervisor Dr. T. N. Bailey for his guidance, encourage- ment and comments throughout the period of my study at Edinburgh University. Thanks are also due to the Department of Mathematics and Statistics for provid- ing such a nice environment in which to work, and to the ORS Awards Scheme for partial financial support. -
Ellectromagnetism and Gravitation
Ellectromagnetism and Gravitation MARIO sc HONBERG* A formulation of the electromagnetic theory in a differentiable manifold devoid of any metric and afine structure is discussed. It is shown that the Maxwell equations in such a manifold in,u.olve a tensor describing the properties of the dielectricity and magnetic permeability of space because of the anisotropy of such a general space. It is also shown that this tensor is es:;entially equivalent to the metric of the angles on the manifold. Thus the necessity of having equations for the determination of this tensor in order to determine the electromagnetic field shows that the Maxwell equations are not a complete set of differential electromagnetic equa- tions. The Einstein gravitational equation appears as complementing the Maxwell set of equations allowing the determination of the dielectricity tensor. Thus a natural fusion of the electromagnetic and gravitationai theories is obtained with an electromagnetic foundation for the geometry of the world-manifold. Discute-se uma formulação da teoria eletromagnética numa variedade diferenciável des- provida de quaisquer métrica e estrutura afim. Mostra-se que as equações de Maxwell em tal variedade envolvem um tensor que descreve as propriedades da dieletricidade e da per- meabilidade magnética do espaço devido ?i anisotropia de tal espaço geral. Mostra-se tam- bem que êsse tensor é essencialmente equivalente h métrica dos ângulos na variedade. Assim a necessidade de se ter equações para a determinação dêsse tensor, a fim de se determinar o campo eletro-magnético, mostra que as equações de Maxwell não são um conjunto completo di: equações diferenciais eletromagnéticas. -
From Spinor Geometry to Complex General Relativity 3
February 1, 2008 20:37 WSPC/INSTRUCTION FILE esposito International Journal of Geometric Methods in Modern Physics c World Scientific Publishing Company FROM SPINOR GEOMETRY TO COMPLEX GENERAL RELATIVITY∗ GIAMPIERO ESPOSITO INFN, Sezione di Napoli, and Dipartimento di Scienze Fisiche, Universit`aFederico II, Complesso Universitario di Monte S. Angelo, Via Cintia, Edificio N’ 80126 Napoli, Italy [email protected] Received (1 April 2005) An attempt is made of giving a self-contained introduction to holomorphic ideas in gen- eral relativity, following work over the last thirty years by several authors. The main top- ics are complex manifolds, two-component spinor calculus, conformal gravity, α-planes in Minkowski space-time, α-surfaces and twistor geometry, anti-self-dual space-times and Penrose transform, spin-3/2 potentials, heaven spaces and heavenly equations. Keywords: Two-component spinors; twistors; Penrose transform. 1. Introduction to Complex Space-Time The physical and mathematical motivations for studying complex space-times or arXiv:hep-th/0504089v2 23 May 2005 real Riemannian four-manifolds in gravitational physics are first described. They originate from algebraic geometry, Euclidean quantum field theory, the path- integral approach to quantum gravity, and the theory of conformal gravity. The theory of complex manifolds is then briefly outlined. Here, one deals with para- compact Hausdorff spaces where local coordinates transform by complex-analytic transformations. Examples are given such as complex projective space Pm, non- singular sub-manifolds of Pm, and orientable surfaces. The plan of the whole paper is eventually presented, with emphasis on two-component spinor calculus, Penrose 3 transform and Penrose formalism for spin- 2 potentials. -
Algebraic Geometry in Cosmology?
Symmetry, Integrability and Geometry: Methods and Applications SIGMA 10 (2014), 073, 20 pages Big Bang, Blowup, and Modular Curves: Algebraic Geometry in Cosmology? Yuri I. MANIN y and Matilde MARCOLLI z y Max-Planck-Institut f¨urMathematik, Bonn, Germany E-mail: [email protected] z California Institute of Technology, Pasadena, USA E-mail: [email protected] Received March 01, 2014, in final form June 27, 2014; Published online July 09, 2014 http://dx.doi.org/10.3842/SIGMA.2014.073 Abstract. We introduce some algebraic geometric models in cosmology related to the \boundaries" of space-time: Big Bang, Mixmaster Universe, Penrose's crossovers between aeons. We suggest to model the kinematics of Big Bang using the algebraic geometric (or analytic) blow up of a point x. This creates a boundary which consists of the projective space of tangent directions to x and possibly of the light cone of x. We argue that time on the boundary undergoes the Wick rotation and becomes purely imaginary. The Mixmaster (Bianchi IX) model of the early history of the universe is neatly explained in this picture by postulating that the reverse Wick rotation follows a hyperbolic geodesic connecting imag- inary time axis to the real one. Penrose's idea to see the Big Bang as a sign of crossover from \the end of previous aeon" of the expanding and cooling Universe to the \beginning of the next aeon" is interpreted as an identification of a natural boundary of Minkowski space at infinity with the Big Bang boundary. Key words: Big Bang cosmology; algebro-geometric blow-ups; cyclic cosmology; Mixmaster cosmologies; modular curves 2010 Mathematics Subject Classification: 85A40; 14N05; 14G35 1 Introduction 1.1 Future and past boundaries of space-times The current observable domain of our expanding Universe is almost flat. -
Background Geometry in Gauge Gravitation Theory
BACKGROUND GEOMETRY IN GAUGE GRAVITATION THEORY Gennadi Sardanashvily Department of Theoretical Physics, Moscow State University, 117234 Moscow, Russia E-mail: [email protected] Abstract Dirac fermion fields are responsible for spontaneous symmetry breaking in gauge grav- itation theory because the spin structure associated with a tetrad field is not preserved under general covariant transformations. Two solutions of this problem can be suggested. (i) There exists the universal spin structure S → X such that any spin structure Sh → X associated with a tetrad field h is a subbundle of the bundle S → X. In this model, gravitational fields correspond to different tetrad (or metric) fields. (ii) A background tetrad field h and the associated spin structure Sh are fixed, while gravitational fields are λ λ λ µ identified with additional tensor fields q µ describing deviations ha = q µha of h. One can think of h as being effective tetrad fields. We show that theree exist gauge trans- formations whiche keep the background tetrad field h and act on the effective fields by the general covariant transformation law. We come to Logunov’s Relativistic Theory of Gravity generalized to dynamic connections and fermion fields. arXiv:gr-qc/9709054v1 21 Sep 1997 1 Introduction Existence of Dirac fermion fields implies that, if a world manifold X is non-compact in order to satisfy causility conditions, it is parallelizable, that is, the tangent bundle TX is trivial and the principal bundle LX of oriented frames in TX admits a global section [1]. Dirac spinors are defined as follows [2, 3]. Let M be the Minkowski space with the metric η = diag(1, −1, −1, −1), a written with respect to a basis {e }.