Compactifications of F-Theory on Calabi-Yau Threefolds (II)
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Umbral Moonshine and K3 Surfaces Arxiv:1406.0619V3 [Hep-Th]
SLAC-PUB-16469 Umbral Moonshine and K3 Surfaces Miranda C. N. Cheng∗1 and Sarah Harrisony2 1Institute of Physics and Korteweg-de Vries Institute for Mathematics, University of Amsterdam, Amsterdam, the Netherlandsz 2Stanford Institute for Theoretical Physics, Department of Physics, and Theory Group, SLAC, Stanford University, Stanford, CA 94305, USA Abstract Recently, 23 cases of umbral moonshine, relating mock modular forms and finite groups, have been discovered in the context of the 23 even unimodular Niemeier lattices. One of the 23 cases in fact coincides with the so-called Mathieu moonshine, discovered in the context of K3 non-linear sigma models. In this paper we establish a uniform relation between all 23 cases of umbral moonshine and K3 sigma models, and thereby take a first step in placing umbral moonshine into a geometric and physical context. This is achieved by relating the ADE root systems of the Niemeier lattices to the ADE du Val singularities that a K3 surface can develop, and the configuration of smooth rational curves in their resolutions. A geometric interpretation of our results is given in terms of the marking of K3 surfaces by Niemeier lattices. arXiv:1406.0619v3 [hep-th] 18 Mar 2015 ∗[email protected] [email protected] zOn leave from CNRS, Paris. 1 This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-76SF00515 and HEP. Umbral Moonshine and K3 Surfaces 2 Contents 1 Introduction and Summary 3 2 The Elliptic Genus of Du Val Singularities 8 3 Umbral Moonshine and Niemeier Lattices 14 4 Umbral Moonshine and the (Twined) K3 Elliptic Genus 20 5 Geometric Interpretation 27 6 Discussion 30 A Special Functions 32 B Calculations and Proofs 34 C The Twining Functions 41 References 48 Umbral Moonshine and K3 Surfaces 3 1 Introduction and Summary Mock modular forms are interesting functions playing an increasingly important role in various areas of mathematics and theoretical physics. -
$ L $-Functions of Higher Dimensional Calabi-Yau Manifolds of Borcea
L-FUNCTIONS OF HIGHER DIMENSIONAL CALABI-YAU MANIFOLDS OF BORCEA-VOISIN TYPE DOMINIK BUREK Abstract. We construct a series of examples of Calabi-Yau manifolds in arbitrary dimension and compute the main invariants. In particular, we give higher dimensional generalisation of Borcea-Voisin Calabi-Yau threefolds. We compute Hodge numbers of constructed examples using orbifold Chen-Ruan cohomology. We also give a method to compute a local zeta function using the Frobenius morphism for orbifold cohomology introduced by Rose. 1. Introduction The first examples of mirror Calabi-Yau threefolds which are neither toric or complete intersection were constructed by C. Borcea ([Bor97]) and C. Voisin ([Voi93]). This construction involves a non- symplectic involutions γS : S ! S, αE : E ! E of a K3 surface S and an elliptic curve E. The quotient (S ×E)=(γS ×αE) has a resolution of singularities which is a Calabi-Yau threefold, the mirror Calabi-Yau threefold is given by the same construction using the mirror K3 surface. C. Vafa and E. Witten studied similar constructions in [VW95] as a resolution of singularities of (E × E × E)=(Z2 ⊕ Z2) and (E × E × E)=(Z3 ⊕ Z3), where E is an elliptic curve and Z2 (resp. Z3) acts as involution (resp. automorphism of order 3). This approach leads to abstract physical models studied by L. Dixon, J. Harvey, C. Vafa, E. Witten in [Dix+85; Dix+86]. More generally, quotients of products of tori by a finite group were classified by J. Dillies, R. Donagi, A. E. Faraggi an K. Wendland in [Dil07; DF04; DW09]. In this paper we shall study Calabi-Yau manifolds constructed as a resolution of singularities of n−1 (X1 × X2 × ::: × Xn)=Zd ; where Xi denotes a variety of Calabi-Yau type with purely non-symplectic automorphism φi;d : Xi ! Xi k of order d, where d = 2; 3; 4 or 6: If Fix(φi;d) for k j d and i = 2; : : : ; n is a smooth divisor and φ1;d satisfies assumption Ad then there exists a crepant resolution Xd;n which is a Calabi-Yau manifold. -
The Top Yukawa Coupling from 10D Supergravity with E8 × E8 Matter
hep-th/9804107 ITEP-98-11 The top Yukawa coupling from 10D supergravity with E E matter 8 × 8 K.Zyablyuk1 Institute of Theoretical and Experimental Physics, Moscow Abstract We consider the compactification of N=1, D=10 supergravity with E E Yang- 8 × 8 Mills matter to N=1, D=4 model with 3 generations. With help of embedding SU(5) → SO(10) E E we find the value of the top Yukawa coupling λ = 16πα =3 → 6 → 8 t GUT at the GUT scale. p 1 Introduction Although superstring theories have great success and today are the best candidates for a quantum theory unifying all interactions, they still do not predict any experimentally testable value, mostly because there is no unambiguous procedure of compactification of extra spatial dimensions. On the other hand, many phenomenological models based on the unification group SO(10) were constructed (for instance [1]). They describe quarks and leptons in representa- tions 161,162,163 and Higgses, responsible for SU(2) breaking, in 10. Basic assumption of these models is that there is only one Yukawa coupling 163 10 163 at the GUT scale, which gives masses of third generation. Masses of first two families· and· mixings are generated due to the interaction with additional superheavy ( MGUT ) states in 16 + 16, 45, 54. Such models explain generation mass hierarchy and allow∼ to express all Yukawa matrices, which well fit into experimentally observable pattern, in terms of few unknown parameters. Models of [1] are unlikely derivable from ”more fundamental” theory like supergrav- ity/string. Nevertheless, something similar can be constructed from D=10 supergravity coupled to E8 E8 matter, which is low-energy limit of heterotic string [2]. -
Basic Properties of K3 Surfaces
Basic Properties of K3 Surfaces Sam Auyeung February 5, 2020 In this note, we review some basic facts about 4-manifolds before considering K3 surfaces over C. These are compact, complex, simply connected surfaces with trivial canonical bundle. It is well known that all K3 surfaces are diffeomorphic to each other by a tough result of 4 4 2 2 Kodaira. The Fermat quartic defined as the zero locus of the polynomial z0 + z1 + z2 + z3 in CP 3 can be shown to be simply connected by the Lefschetz Hyperplane theorem because it applies to hypersurfaces as well. The main resource I used for this note is Mario Micallef and Jon Wolfson's paper Area Minimizers in a K3 Surface and Holomorphicity. In the paper, they produce an example of a strictly stable minimal 2-sphere in a non-compact hyperK¨ahlersurface that is not holomor- phic for any compactible complex structure. This is interesting because, from the Wirtinger inequality, a compact complex submanifold of a K¨ahlermanifold is a volume minimizer in its homology class and any other volume minimizer in the same class must be complex. 1 Topology Recall that we have a complete topological classification for simply connected, closed, orientable 4-manifolds. The classification depends on the intersection form of such a 4-manifold. Let Q : A × A ! Z be a symmetric unimodular bilinear form for some free abelian group A. Unimodular just means that if we have a 2 A, there exists a b 2 A such that Q(a; b) = +1. There is a classification of all such bilinear forms based on their signature, rank, and type. -
The Duality Between F-Theory and the Heterotic String in with Two Wilson
Letters in Mathematical Physics (2020) 110:3081–3104 https://doi.org/10.1007/s11005-020-01323-8 The duality between F-theory and the heterotic string in D = 8 with two Wilson lines Adrian Clingher1 · Thomas Hill2 · Andreas Malmendier2 Received: 2 June 2020 / Revised: 20 July 2020 / Accepted: 30 July 2020 / Published online: 7 August 2020 © Springer Nature B.V. 2020 Abstract We construct non-geometric string compactifications by using the F-theory dual of the heterotic string compactified on a two-torus with two Wilson line parameters, together with a close connection between modular forms and the equations for certain K3 surfaces of Picard rank 16. Weconstruct explicit Weierstrass models for all inequivalent Jacobian elliptic fibrations supported on this family of K3 surfaces and express their parameters in terms of modular forms generalizing Siegel modular forms. In this way, we find a complete list of all dual non-geometric compactifications obtained by the partial Higgsing of the heterotic string gauge algebra using two Wilson line parameters. Keywords F-theory · String duality · K3 surfaces · Jacobian elliptic fibrations Mathematics Subject Classification 14J28 · 14J81 · 81T30 1 Introduction In a standard compactification of the type IIB string theory, the axio-dilaton field τ is constant and no D7-branes are present. Vafa’s idea in proposing F-theory [51] was to simultaneously allow a variable axio-dilaton field τ and D7-brane sources, defining at a new class of models in which the string coupling is never weak. These compactifications of the type IIB string in which the axio-dilaton field varies over a base are referred to as F-theory models. -
General Introduction to K3 Surfaces
General introduction to K3 surfaces Svetlana Makarova MIT Mathematics Contents 1 Algebraic K3 surfaces 1 1.1 Definition of K3 surfaces . .1 1.2 Classical invariants . .3 2 Complex K3 surfaces 9 2.1 Complex K3 surfaces . .9 2.2 Hodge structures . 11 2.3 Period map . 12 References 16 1 Algebraic K3 surfaces 1.1 Definition of K3 surfaces Let K be an arbitrary field. Here, a variety over K will mean a separated, geometrically integral scheme of finite type over K.A surface is a variety of dimension two. If X is a variety over of dimension n, then ! will denote its canonical class, that is ! =∼ Ωn . K X X X=K For a sheaf F on a scheme X, I will write H• (F) for H• (X; F), unless that leads to ambiguity. Definition 1.1.1. A K3 surface over K is a complete non-singular surface X such that ∼ 1 !X = OX and H (X; OX ) = 0. Corollary 1.1.1. One can observe several simple facts for a K3 surface: ∼ 1.Ω X = TX ; 2 ∼ 0 2.H (OX ) = H (OX ); 3. χ(OX ) = 2 dim Γ(OX ) = 2. 1 Fact 1.1.2. Any smooth complete surface over an algebraically closed field is projective. This fact is an immediate corollary of the Zariski{Goodman theorem which states that for any open affine U in a smooth complete surface X (over an algebraically closed field), the closed subset X nU is connected and of pure codimension one in X, and moreover supports an ample effective divisor. -
K3 Surfaces and String Duality
RU-96-98 hep-th/9611137 November 1996 K3 Surfaces and String Duality Paul S. Aspinwall Dept. of Physics and Astronomy, Rutgers University, Piscataway, NJ 08855 ABSTRACT The primary purpose of these lecture notes is to explore the moduli space of type IIA, type IIB, and heterotic string compactified on a K3 surface. The main tool which is invoked is that of string duality. K3 surfaces provide a fascinating arena for string compactification as they are not trivial spaces but are sufficiently simple for one to be able to analyze most of their properties in detail. They also make an almost ubiquitous appearance in the common statements concerning string duality. We arXiv:hep-th/9611137v5 7 Sep 1999 review the necessary facts concerning the classical geometry of K3 surfaces that will be needed and then we review “old string theory” on K3 surfaces in terms of conformal field theory. The type IIA string, the type IIB string, the E E heterotic string, 8 × 8 and Spin(32)/Z2 heterotic string on a K3 surface are then each analyzed in turn. The discussion is biased in favour of purely geometric notions concerning the K3 surface itself. Contents 1 Introduction 2 2 Classical Geometry 4 2.1 Definition ..................................... 4 2.2 Holonomy ..................................... 7 2.3 Moduli space of complex structures . ..... 9 2.4 Einsteinmetrics................................. 12 2.5 AlgebraicK3Surfaces ............................. 15 2.6 Orbifoldsandblow-ups. .. 17 3 The World-Sheet Perspective 25 3.1 TheNonlinearSigmaModel . 25 3.2 TheTeichm¨ullerspace . .. 27 3.3 Thegeometricsymmetries . .. 29 3.4 Mirrorsymmetry ................................. 31 3.5 Conformalfieldtheoryonatorus . ... 33 4 Type II String Theory 37 4.1 Target space supergravity and compactification . -
Arxiv:1805.06347V1 [Hep-Th] 16 May 2018 Sa Rte O H Rvt Eerhfudto 08Awar 2018 Foundation Research Gravity the for Written Essay Result
Maximal supergravity and the quest for finiteness 1 2 3 Sudarshan Ananth† , Lars Brink∗ and Sucheta Majumdar† † Indian Institute of Science Education and Research Pune 411008, India ∗ Department of Physics, Chalmers University of Technology S-41296 G¨oteborg, Sweden and Division of Physics and Applied Physics, School of Physical and Mathematical Sciences Nanyang Technological University, Singapore 637371 March 28, 2018 Abstract We show that N = 8 supergravity may possess an even larger symmetry than previously believed. Such an enhanced symmetry is needed to explain why this theory of gravity exhibits ultraviolet behavior reminiscent of the finite N = 4 Yang-Mills theory. We describe a series of three steps that leads us to this result. arXiv:1805.06347v1 [hep-th] 16 May 2018 Essay written for the Gravity Research Foundation 2018 Awards for Essays on Gravitation 1Corresponding author, [email protected] [email protected] [email protected] Quantum Field Theory describes three of the four fundamental forces in Nature with great precision. However, when attempts have been made to use it to describe the force of gravity, the resulting field theories, are without exception, ultraviolet divergent and non- renormalizable. One striking aspect of supersymmetry is that it greatly reduces the diver- gent nature of quantum field theories. Accordingly, supergravity theories have less severe ultraviolet divergences. Maximal supergravity in four dimensions, N = 8 supergravity [1], has the best ultraviolet properties of any field theory of gravity with two derivative couplings. Much of this can be traced back to its three symmetries: Poincar´esymmetry, maximal supersymmetry and an exceptional E7(7) symmetry. -
Introduction to String Theory A.N
Introduction to String Theory A.N. Schellekens Based on lectures given at the Radboud Universiteit, Nijmegen Last update 6 July 2016 [Word cloud by www.worldle.net] Contents 1 Current Problems in Particle Physics7 1.1 Problems of Quantum Gravity.........................9 1.2 String Diagrams................................. 11 2 Bosonic String Action 15 2.1 The Relativistic Point Particle......................... 15 2.2 The Nambu-Goto action............................ 16 2.3 The Free Boson Action............................. 16 2.4 World sheet versus Space-time......................... 18 2.5 Symmetries................................... 19 2.6 Conformal Gauge................................ 20 2.7 The Equations of Motion............................ 21 2.8 Conformal Invariance.............................. 22 3 String Spectra 24 3.1 Mode Expansion................................ 24 3.1.1 Closed Strings.............................. 24 3.1.2 Open String Boundary Conditions................... 25 3.1.3 Open String Mode Expansion..................... 26 3.1.4 Open versus Closed........................... 26 3.2 Quantization.................................. 26 3.3 Negative Norm States............................. 27 3.4 Constraints................................... 28 3.5 Mode Expansion of the Constraints...................... 28 3.6 The Virasoro Constraints............................ 29 3.7 Operator Ordering............................... 30 3.8 Commutators of Constraints.......................... 31 3.9 Computation of the Central Charge..................... -
S-Duality-And-M5-Mit
N . More on = 2 S-dualities and M5-branes .. Yuji Tachikawa based on works in collaboration with L. F. Alday, B. Wecht, F. Benini, S. Benvenuti, D. Gaiotto November 2009 Yuji Tachikawa (IAS) November 2009 1 / 47 Contents 1. Introduction 2. S-dualities 3. A few words on TN 4. 4d CFT vs 2d CFT Yuji Tachikawa (IAS) November 2009 2 / 47 Montonen-Olive duality • N = 4 SU(N) SYM at coupling τ = θ=(2π) + (4πi)=g2 equivalent to the same theory coupling τ 0 = −1/τ • One way to ‘understand’ it: start from 6d N = (2; 0) theory, i.e. the theory on N M5-branes, put on a torus −1/τ τ 0 1 0 1 • Low energy physics depends only on the complex structure S-duality! Yuji Tachikawa (IAS) November 2009 3 / 47 S-dualities in N = 2 theories • You can wrap N M5-branes on a more general Riemann surface, possibly with punctures, to get N = 2 superconformal field theories • Different limits of the shape of the Riemann surface gives different weakly-coupled descriptions, giving S-dualities among them • Anticipated by [Witten,9703166], but not well-appreciated until [Gaiotto,0904.2715] Yuji Tachikawa (IAS) November 2009 4 / 47 Contents 1. Introduction 2. S-dualities 3. A few words on TN 4. 4d CFT vs 2d CFT Yuji Tachikawa (IAS) November 2009 5 / 47 Contents 1. Introduction 2. S-dualities 3. A few words on TN 4. 4d CFT vs 2d CFT Yuji Tachikawa (IAS) November 2009 6 / 47 S-duality in N = 2 . SU(2) with Nf = 4 . -
Is String Theory Holographic? 1 Introduction
Holography and large-N Dualities Is String Theory Holographic? Lukas Hahn 1 Introduction1 2 Classical Strings and Black Holes2 3 The Strominger-Vafa Construction3 3.1 AdS/CFT for the D1/D5 System......................3 3.2 The Instanton Moduli Space.........................6 3.3 The Elliptic Genus.............................. 10 1 Introduction The holographic principle [1] is based on the idea that there is a limit on information content of spacetime regions. For a given volume V bounded by an area A, the state of maximal entropy corresponds to the largest black hole that can fit inside V . This entropy bound is specified by the Bekenstein-Hawking entropy A S ≤ S = (1.1) BH 4G and the goings-on in the relevant spacetime region are encoded on "holographic screens". The aim of these notes is to discuss one of the many aspects of the question in the title, namely: "Is this feature of the holographic principle realized in string theory (and if so, how)?". In order to adress this question we start with an heuristic account of how string like objects are related to black holes and how to compare their entropies. This second section is exclusively based on [2] and will lead to a key insight, the need to consider BPS states, which allows for a more precise treatment. The most fully understood example is 1 a bound state of D-branes that appeared in the original article on the topic [3]. The third section is an attempt to review this construction from a point of view that highlights the role of AdS/CFT [4,5]. -
A Survey of Calabi-Yau Manifolds
Surveys in Differential Geometry XIII A survey of Calabi-Yau manifolds Shing-Tung Yau Contents 1. Introduction 278 2. General constructions of complete Ricci-flat metrics in K¨ahler geometry 278 2.1. The Ricci tensor of Calabi-Yau manifolds 278 2.2. The Calabi conjecture 279 2.3. Yau’s theorem 279 2.4. Calabi-Yau manifolds and Calabi-Yau metrics 280 2.5. Examples of compact Calabi-Yau manifolds 281 2.6. Noncompact Calabi-Yau manifolds 282 2.7. Calabi-Yau cones: Sasaki-Einstein manifolds 283 2.8. The balanced condition on Calabi-Yau metrics 284 3. Moduli and arithmetic of Calabi-Yau manifolds 285 3.1. Moduli of K3 surfaces 285 3.2. Moduli of high dimensional Calabi-Yau manifolds 286 3.3. The modularity of Calabi–Yau threefolds over Q 287 4. Calabi-Yau manifolds in physics 288 4.1. Calabi-Yau manifolds in string theory 288 4.2. Calabi-Yau manifolds and mirror symmetry 289 4.3. Mathematics inspired by mirror symmetry 291 5. Invariants of Calabi-Yau manifolds 291 5.1. Gromov-Witten invariants 291 5.2. Counting formulas 292 5.3. Proofs of counting formulas for Calabi-Yau threefolds 293 5.4. Integrability of mirror map and arithmetic applications 293 5.5. Donaldson-Thomas invariants 294 5.6. Stable bundles and sheaves 296 5.7. Yau-Zaslow formula for K3 surfaces 296 5.8. Chern-Simons knot invariants, open strings and string dualities 297 c 2009 International Press 277 278 S.-T. YAU 6. Homological mirror symmetry 299 7. SYZ geometric interpretation of mirror symmetry 300 7.1.