K3 Metrics from String Theory
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M2-Branes Ending on M5-Branes
M2-branes ending on M5-branes Vasilis Niarchos Crete Center for Theoretical Physics, University of Crete 7th Crete Regional Meeting on String Theory, 27/06/2013 based on recent work with K. Siampos 1302.0854, ``The black M2-M5 ring intersection spins’‘ Proceedings Corfu Summer School, 2012 1206.2935, ``Entropy of the self-dual string soliton’’, JHEP 1207 (2012) 134 1205.1535, ``M2-M5 blackfold funnels’’, JHEP 1206 (2012) 175 and older work with R. Emparan, T. Harmark and N. A. Obers ➣ blackfold theory 1106.4428, ``Blackfolds in Supergravity and String Theory’’, JHEP 1108 (2011) 154 0912.2352, ``New Horizons for Black Holes and Branes’’, JHEP 1004 (2010) 046 0910.1601, ``Essentials of Blackfold Dynamics’’, JHEP 1003 (2010) 063 0902.0427, ``World-Volume Effective Theory for Higher-Dimensional Black Holes’’, PRL 102 (2009)191301 0708.2181, ``The Phase Structure of Higher-Dimensional Black Rings and Black Holes’‘ + M.J. Rodriguez JHEP 0710 (2007) 110 2 Important lessons about the fundamentals of string/M-theory (and QFT) are obtained by studying the low-energy theories on D-branes and M-branes. Most notably in M-theory, recent progress has clarified the low-energy QFT on N M2-brane and the N3/2 dof that it exhibits. Bagger-Lambert ’06, Gustavsson ’07, ABJM ’08 Drukker-Marino-Putrov ’10 Our understanding of the M5-brane theory is more rudimentary, but efforts to identify analogous properties, e.g. the N3 scaling of the massless dof, is underway. Douglas ’10 Lambert,Papageorgakis,Schmidt-Sommerfeld ’10 Hosomichi-Seong-Terashima ’12 Kim-Kim ’12 Kallen-Minahan-Nedelin-Zabzine ’12 .. -
JHEP05(2015)095 ) Gauge Springer N May 4, 2015 May 19, 2015 : : February 11, 2015
Published for SISSA by Springer Received: February 11, 2015 Accepted: May 4, 2015 Published: May 19, 2015 Defects and quantum Seiberg-Witten geometry JHEP05(2015)095 Mathew Bullimore,a Hee-Cheol Kimb and Peter Koroteevb aInstitute for Advanced Study, Einstein Dr., Princeton, NJ 08540, U.S.A. bPerimeter Institute for Theoretical Physics, 31 Caroline Street North, Waterloo, Ontario N2L2Y5, Canada E-mail: [email protected], [email protected], [email protected] Abstract: We study the Nekrasov partition function of the five dimensional U(N) gauge theory with maximal supersymmetry on R4 S1 in the presence of codimension two defects. × The codimension two defects can be described either as monodromy defects, or by coupling to a certain class of three dimensional quiver gauge theories on R2 S1. We explain how × these computations are connected with both classical and quantum integrable systems. We check, as an expansion in the instanton number, that the aforementioned partition functions are eigenfunctions of an elliptic integrable many-body system, which quantizes the Seiberg-Witten geometry of the five-dimensional gauge theory. Keywords: Supersymmetric gauge theory, Duality in Gauge Field Theories, Integrable Equations in Physics, Differential and Algebraic Geometry ArXiv ePrint: 1412.6081 Open Access, c The Authors. ⃝ doi:10.1007/JHEP05(2015)095 Article funded by SCOAP3. Contents 1 Introduction 1 2 Twisted chiral rings 3 2.1 The Nekrasov-Shatashvili correspondence 4 2.2 Quantum/classical duality 6 2.2.1 Electric frame -
Moduli Spaces
spaces. Moduli spaces such as the moduli of elliptic curves (which we discuss below) play a central role Moduli Spaces in a variety of areas that have no immediate link to the geometry being classified, in particular in alge- David D. Ben-Zvi braic number theory and algebraic topology. Moreover, the study of moduli spaces has benefited tremendously in recent years from interactions with Many of the most important problems in mathemat- physics (in particular with string theory). These inter- ics concern classification. One has a class of math- actions have led to a variety of new questions and new ematical objects and a notion of when two objects techniques. should count as equivalent. It may well be that two equivalent objects look superficially very different, so one wishes to describe them in such a way that equiv- 1 Warmup: The Moduli Space of Lines in alent objects have the same description and inequiva- the Plane lent objects have different descriptions. Moduli spaces can be thought of as geometric solu- Let us begin with a problem that looks rather simple, tions to geometric classification problems. In this arti- but that nevertheless illustrates many of the impor- cle we shall illustrate some of the key features of mod- tant ideas of moduli spaces. uli spaces, with an emphasis on the moduli spaces Problem. Describe the collection of all lines in the of Riemann surfaces. (Readers unfamiliar with Rie- real plane R2 that pass through the origin. mann surfaces may find it helpful to begin by reading about them in Part III.) In broad terms, a moduli To save writing, we are using the word “line” to mean problem consists of three ingredients. -
Bosonization and Mirror Symmetry Arxiv:1608.05077V1 [Hep-Th]
Bosonization and Mirror Symmetry Shamit Kachru1, Michael Mulligan2,1, Gonzalo Torroba3, and Huajia Wang4 1Stanford Institute for Theoretical Physics, Stanford University, Stanford, CA 94305, USA 2Department of Physics and Astronomy, University of California, Riverside, CA 92511, USA 3Centro At´omico Bariloche and CONICET, R8402AGP Bariloche, ARG 4Department of Physics, University of Illinois, Urbana-Champaign, IL 61801, USA Abstract We study bosonization in 2+1 dimensions using mirror symmetry, a duality that relates pairs of supersymmetric theories. Upon breaking supersymmetry in a controlled way, we dynamically obtain the bosonization duality that equates the theory of a free Dirac fermion to QED3 with a single scalar boson. This duality may be used to demonstrate the bosonization duality relating an O(2)-symmetric Wilson-Fisher fixed point to QED3 with a single Dirac fermion, Peskin-Dasgupta-Halperin duality, and the recently conjectured duality relating the theory of a free Dirac fermion to fermionic QED3 with a single flavor. Chern-Simons and BF couplings for both dynamical and background gauge fields play a central role in our approach. In the course of our study, we describe a \chiral" mirror pair that may be viewed as the minimal supersymmetric generalization of the two bosonization dualities. arXiv:1608.05077v1 [hep-th] 17 Aug 2016 Contents 1 Introduction 1 2 Mirror symmetry and its deformations 4 2.1 Superfields and lagrangians . .5 2.2 = 4 mirror symmetry . .7 N 2.3 Deformations by U(1)A and U(1)R backgrounds . 10 2.4 General mirror duality . 11 3 Chiral mirror symmetry 12 3.1 Chiral theory A . -
Jhep05(2019)105
Published for SISSA by Springer Received: March 21, 2019 Accepted: May 7, 2019 Published: May 20, 2019 Modular symmetries and the swampland conjectures JHEP05(2019)105 E. Gonzalo,a;b L.E. Ib´a~neza;b and A.M. Urangaa aInstituto de F´ısica Te´orica IFT-UAM/CSIC, C/ Nicol´as Cabrera 13-15, Campus de Cantoblanco, 28049 Madrid, Spain bDepartamento de F´ısica Te´orica, Facultad de Ciencias, Universidad Aut´onomade Madrid, 28049 Madrid, Spain E-mail: [email protected], [email protected], [email protected] Abstract: Recent string theory tests of swampland ideas like the distance or the dS conjectures have been performed at weak coupling. Testing these ideas beyond the weak coupling regime remains challenging. We propose to exploit the modular symmetries of the moduli effective action to check swampland constraints beyond perturbation theory. As an example we study the case of heterotic 4d N = 1 compactifications, whose non-perturbative effective action is known to be invariant under modular symmetries acting on the K¨ahler and complex structure moduli, in particular SL(2; Z) T-dualities (or subgroups thereof) for 4d heterotic or orbifold compactifications. Remarkably, in models with non-perturbative superpotentials, the corresponding duality invariant potentials diverge at points at infinite distance in moduli space. The divergence relates to towers of states becoming light, in agreement with the distance conjecture. We discuss specific examples of this behavior based on gaugino condensation in heterotic orbifolds. We show that these examples are dual to compactifications of type I' or Horava-Witten theory, in which the SL(2; Z) acts on the complex structure of an underlying 2-torus, and the tower of light states correspond to D0-branes or M-theory KK modes. -
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. -
From Vibrating Strings to a Unified Theory of All Interactions
Barton Zwiebach From Vibrating Strings to a Unified Theory of All Interactions or the last twenty years, physicists have investigated F String Theory rather vigorously. The theory has revealed an unusual depth. As a result, despite much progress in our under- standing of its remarkable properties, basic features of the theory remain a mystery. This extended period of activity is, in fact, the second period of activity in string theory. When it was first discov- ered in the late 1960s, string theory attempted to describe strongly interacting particles. Along came Quantum Chromodynamics— a theoryof quarks and gluons—and despite their early promise, strings faded away. This time string theory is a credible candidate for a theoryof all interactions—a unified theoryof all forces and matter. The greatest complication that frustrated the search for such a unified theorywas the incompatibility between two pillars of twen- tieth century physics: Einstein’s General Theoryof Relativity and the principles of Quantum Mechanics. String theory appears to be 30 ) zwiebach mit physics annual 2004 the long-sought quantum mechani- cal theory of gravity and other interactions. It is almost certain that string theory is a consistent theory. It is less certain that it describes our real world. Nevertheless, intense work has demonstrated that string theory incorporates many features of the physical universe. It is reasonable to be very optimistic about the prospects of string theory. Perhaps one of the most impressive features of string theory is the appearance of gravity as one of the fluctuation modes of a closed string. Although it was not discov- ered exactly in this way, we can describe a logical path that leads to the discovery of gravity in string theory. -
Intersecting Surface Defects and 3D Superconformal Indices
Published for SISSA by Springer Received: February 2, 2021 Accepted: April 19, 2021 Published: May 18, 2021 JHEP05(2021)155 Intersecting surface defects and 3d superconformal indices Junfeng Liu, Yiwen Pan and Hong-Hao Zhang School of Physics, Sun Yat-Sen University, Guangzhou 510275, China E-mail: [email protected], [email protected], [email protected] Abstract: We compute the 3d N = 2 superconformal indices for 3d/1d coupled systems, which arise as the worldvolume theories of intersecting surface defects engineered by Higgsing 5d N = 1 gauge theories. We generalize some known 3d dualities, including non-Abelian 3d mirror symmetry and 3d/3d correspondence, to some of the simple 3d/1d coupled systems. Finally we propose a q-Virasoro construction for the superconformal indices. Keywords: Duality in Gauge Field Theories, Supersymmetry and Duality ArXiv ePrint: 2101.05689 Open Access , c The Authors. https://doi.org/10.1007/JHEP05(2021)155 Article funded by SCOAP3. Contents 1 Introduction1 2 Higgsing and surface defects3 3 Intersecting surface defects on S4 × S1 6 3.1 Higgsing6 3.2 Index of intersecting gauge theory 10 JHEP05(2021)155 3.2.1 Reduction to 2d 12 4 3d dualities 13 4.1 3d mirror symmetry 13 4.1.1 U(1) 1 theory 14 4.1.2 3d mirror2 symmetry from fiber-base duality 16 4.2 3d/3d correspondence 21 5 q-Virasoro construction 24 A Special functions 28 B Instanton partition function 29 C Factorization of 3d index 31 1 Introduction Since the seminal work by Pestun [1], numerous exact results have been derived using the technique of supersymmetric localization for supersymmetric theories in different dimensions. -
Arxiv:2002.11085V1 [Hep-Th]
On-Shell Electric-Magnetic Duality and the Dual Graviton 1,2 2 Nathan Moynihan and Jeff Murugan ∗ 1High Energy Physics, Cosmology & Astrophysics Theory group, 2The Laboratory for Quantum Gravity & Strings Department of Mathematics and Applied Mathematics, University of Cape Town, Rondebosch, Cape Town 7700, South Africa Using on-shell amplitude methods, we explore 4-dimensional Electric-Magnetic duality and its double copy. We show explicitly that the on-shell scattering amplitudes know about ‘dual’ photons (and dual gravitons), that the off-shell photon propagator double copies to the graviton propagator and that the magnetic part of the propagator is essential for the double copy to hold. We also show that there is an equivalent gravito-magnetic part of the graviton propagator which is essential in giving rise to solutions with either angular momentum or NUT charge. Furthermore, we comment on the so-called Weinberg paradox, which states that scattering amplitudes involving the mixing of electric and magnetic monopoles cannot be Lorentz invariant, and would seem to preclude the existence of the ’t Hooft-Polyakov (topological) monopole. We trace this paradox to the magnetic part of the propagator, showing that it can be eliminated if one restricts to proper orthochronous Lorentz transformations. Finally, we compute the fully relativistic cross-section for arbitrary spin dyons using the recently formulated on-shell duality transformation and show that this is always fully Lorentz invariant. INTRODUCTION field theory without a Dirac string singularity necessitates the introduction of a second four-vector potential: the The boostrap program of the 1960’s received considerable dual photon [3–6]. -
The Topology of Moduli Space and Quantum Field Theory* ABSTRACT
SLAC-PUB-4760 October 1988 CT) . The Topology of Moduli Space and Quantum Field Theory* DAVID MONTANO AND JACOB SONNENSCHEIN+ Stanford Linear Accelerator Center Stanford University, Stanford, California 9.4309 ABSTRACT We show how an SO(2,l) gauge theory with a fermionic symmetry may be used to describe the topology of the moduli space of curves. The observables of the theory correspond to the generators of the cohomology of moduli space. This is an extension of the topological quantum field theory introduced by Witten to -- .- . -. investigate the cohomology of Yang-Mills instanton moduli space. We explore the basic structure of topological quantum field theories, examine a toy U(1) model, and then realize a full theory of moduli space topology. We also discuss why a pure gravity theory, as attempted in previous work, could not succeed. Submitted to Nucl. Phys. I3 _- .- --- _ * Work supported by the Department of Energy, contract DE-AC03-76SF00515. + Work supported by Dr. Chaim Weizmann Postdoctoral Fellowship. 1. Introduction .. - There is a widespread belief that the Lagrangian is the fundamental object for study in physics. The symmetries of nature are simply properties of the relevant Lagrangian. This philosophy is one of the remaining relics of classical physics where the Lagrangian is indeed fundamental. Recently, Witten has discovered a class of quantum field theories which have no classical analog!” These topo- logical quantum field theories (TQFT) are, as their name implies, characterized by a Hilbert space of topological invariants. As has been recently shown, they can be constructed by a BRST gauge fixing of a local symmetry. -
The Fuzzball Proposal for Black Holes: an Elementary Review
hep-th/0502050 The fuzzball proposal for black holes: an elementary review1 Samir D. Mathur Department of Physics, The Ohio State University, Columbus, OH 43210, USA [email protected] Abstract We give an elementary review of black holes in string theory. We discuss BPS holes, the microscopic computation of entropy and the ‘fuzzball’ picture of the arXiv:hep-th/0502050v1 3 Feb 2005 black hole interior suggested by microstates of the 2-charge system. 1Lecture given at the RTN workshop ‘The quantum structure of space-time and the geometric nature of fundamental interactions’, in Crete, Greece (September 2004). 1 Introduction The quantum theory of black holes presents many paradoxes. It is vital to ask how these paradoxes are to be resolved, for the answers will likely lead to deep changes in our understanding of quantum gravity, spacetime and matter. Bekenstein [1] argued that black holes should be attributed an entropy A S = (1.1) Bek 4G where A is the area of the horizon and G is the Newton constant of gravitation. (We have chosen units to set c = ~ = 1.) This entropy must be attributed to the hole if we are to prevent a violation of the second law of thermodynamics. We can throw a box of gas with entropy ∆S into a black hole, and see it vanish into the central singularity. This would seem to decrease the entropy of the Universe, but we note that the area of the horizon increases as a result of the energy added by the box. It turns out that if we assign (1.1) as the entropy of the hole then the total entropy is nondecreasing dS dS Bek + matter 0 (1.2) dt dt ≥ This would seem to be a good resolution of the entropy problem, but it leads to another problem.