Conifold Holography
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Wall Crossing and M-Theory
Wall Crossing and M-theory The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Aganagic, Mina, Hirosi Ooguri, Cumrun Vafa, and Masahito Yamazaki. 2011. Wall crossing and M-theory. Publications of the Research Institute for Mathematical Sciences 47(2): 569-584. Published Version doi:10.2977/PRIMS/44 Citable link http://nrs.harvard.edu/urn-3:HUL.InstRepos:7561260 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Open Access Policy Articles, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#OAP CALT-68-2746 IPMU09-0091 UT-09-18 Wall Crossing and M-Theory Mina Aganagic1, Hirosi Ooguri2,3, Cumrun Vafa4 and Masahito Yamazaki2,3,5 1Center for Theoretical Physics, University of California, Berkeley, CA 94720, USA 2California Institute of Technology, Pasadena, CA 91125, USA 3 IPMU, University of Tokyo, Chiba 277-8586, Japan 4Jefferson Physical Laboratory, Harvard University, Cambridge, MA 02138, USA 5Department of Physics, University of Tokyo, Tokyo 113-0033, Japan Abstract arXiv:0908.1194v1 [hep-th] 8 Aug 2009 We study BPS bound states of D0 and D2 branes on a single D6 brane wrapping a Calabi- Yau 3-fold X. When X has no compact 4-cyles, the BPS bound states are organized into a free field Fock space, whose generators correspond to BPS states of spinning M2 branes in M- theory compactified down to 5 dimensions by a Calabi-Yau 3-fold X. -
Non-Holomorphic Cycles and Non-BPS Black Branes Arxiv
Non-Holomorphic Cycles and Non-BPS Black Branes Cody Long,1;2 Artan Sheshmani,2;3;4 Cumrun Vafa,1 and Shing-Tung Yau2;5 1Jefferson Physical Laboratory, Harvard University Cambridge, MA 02138, USA 2Center for Mathematical Sciences and Applications, Harvard University Cambridge, MA 02139, USA 3Institut for Matematik, Aarhus Universitet 8000 Aarhus C, Denmark 4 National Research University Higher School of Economics, Russian Federation, Laboratory of Mirror Symmetry, Moscow, Russia, 119048 5Department of Mathematics, Harvard University Cambridge, MA 02138, USA We study extremal non-BPS black holes and strings arising in M-theory compactifica- tions on Calabi-Yau threefolds, obtained by wrapping M2 branes on non-holomorphic 2-cycles and M5 branes on non-holomorphic 4-cycles. Using the attractor mechanism we compute the black hole mass and black string tension, leading to a conjectural for- mula for the asymptotic volumes of connected, locally volume-minimizing representa- tives of non-holomorphic, even-dimensional homology classes in the threefold, without arXiv:2104.06420v1 [hep-th] 13 Apr 2021 knowledge of an explicit metric. In the case of divisors we find examples where the vol- ume of the representative corresponding to the black string is less than the volume of the minimal piecewise-holomorphic representative, predicting recombination for those homology classes and leading to stable, non-BPS strings. We also compute the central charges of non-BPS strings in F-theory via a near-horizon AdS3 limit in 6d which, upon compactification on a circle, account for the asymptotic entropy of extremal non- supersymmetric 5d black holes (i.e., the asymptotic count of non-holomorphic minimal 2-cycles). -
Abdus Salam Educational, Scientific and Cultural XA0500266 Organization International Centre
the united nations abdus salam educational, scientific and cultural XA0500266 organization international centre international atomic energy agency for theoretical physics 1 a M THEORY AND SINGULARITIES OF EXCEPTIONAL HOLONOMY MANIFOLDS Bobby S. Acharya and Sergei Gukov Available at: http://www.ictp.it/-pub-off IC/2004/127 HUTP-03/A053 RUNHETC-2003-26 United Nations Educational Scientific and Cultural Organization and International Atomic Energy Agency THE ABDUS SALAM INTERNATIONAL CENTRE FOR THEORETICAL PHYSICS M THEORY AND SINGULARITIES OF EXCEPTIONAL HOLONOMY MANIFOLDS Bobby S. Acharya1 The Abdus Salam International Centre for Theoretical Physics, Trieste, Italy and Sergei Gukov2 Jefferson Physical Laboratory, Harvard University, Cambridge, MA 02138, USA. Abstract M theory compactifications on Gi holonomy manifolds, whilst supersymmetric, require sin- gularities in order to obtain non-Abelian gauge groups, chiral fermions and other properties necessary for a realistic model of particle physics. We review recent progress in understanding the physics of such singularities. Our main aim is to describe the techniques which have been used to develop our understanding of M theory physics near these singularities. In parallel, we also describe similar sorts of singularities in Spin(7) holonomy manifolds which correspond to the properties of three dimensional field theories. As an application, we review how various aspects of strongly coupled gauge theories, such as confinement, mass gap and non-perturbative phase transitions may be given a -
Open Gromov-Witten Invariants and Syz Under Local Conifold Transitions
OPEN GROMOV-WITTEN INVARIANTS AND SYZ UNDER LOCAL CONIFOLD TRANSITIONS SIU-CHEONG LAU Abstract. For a local non-toric Calabi-Yau manifold which arises as smoothing of a toric Gorenstein singularity, this paper derives the open Gromov-Witten invariants of a generic fiber of the special Lagrangian fibration constructed by Gross and thereby constructs its SYZ mirror. Moreover it proves that the SYZ mirrors and disc potentials vary smoothly under conifold transitions, giving a global picture of SYZ mirror symmetry. 1. Introduction Let N be a lattice and P a lattice polytope in NR. It is an interesting classical problem in combinatorial geometry to construct Minkowski decompositions of P . P v On the other hand, consider the family of polynomials v2P \N cvz for cv 2 C with cv 6= 0 when v is a vertex of P . All these polynomials have P as their Newton polytopes. This establishes a relation between geometry and algebra, and the geometric problem of finding Minkowski decompositions is transformed to the algebraic problem of finding polynomial factorizations. One purpose of this paper is to show that the beautiful algebro-geometric correspondence between Minkowski decompositions and polynomial factorizations can be realized via SYZ mirror symmetry. A key step leading to the miracle is brought by a result of Altmann [3]. First of all, a lattice polytope corresponds to a toric Gorenstein singularity X. Altmann showed that Minkowski decompositions of the lattice polytope correspond to (partial) smoothings of X. From string- theoretic point of view different smoothings of X belong to different sectors of the same stringy K¨ahlermoduli. -
Black Brane Evaporation Through D-Brane Bubble Nucleation
HIP-2021-20/TH Black brane evaporation through D-brane bubble nucleation Oscar Henriksson∗ Department of Physics and Helsinki Institute of Physics P.O. Box 64, FI-00014 University of Helsinki, Finland Abstract We study the process of black brane evaporation through the emission of D-branes. Gravi- tational solutions describing black branes in asymptotically anti-de Sitter spacetimes, which are holographically dual to field theory states at finite temperature and density, have previously been found to exhibit an instability due to brane nucleation. Working in the setting of D3-branes on the conifold, we construct static Euclidean solutions describing this nucleation to leading order | D3-branes bubbling off the horizon. Furthermore, we analyze the late-time dynamics of such a D3-brane bubble as it expands and find a steady-state solution including the wall profile and its speed. CONTENTS I. Introduction 2 II. Gravity solutions and field theory dual 3 III. The D3-brane effective action 4 IV. Bubble nucleation 6 arXiv:2106.13254v1 [hep-th] 24 Jun 2021 V. Late time expansion 8 VI. Discussion 11 Acknowledgments 12 References 12 ∗ oscar.henriksson@helsinki.fi 1 I. INTRODUCTION Black holes are unstable to evaporation due to Hawking radiation. Though this fact is on firm theoretical footing, there are still many open questions regarding the precise details of this evaporation, some of which may require a complete theory of quantum gravity to settle. String theory is a strong candidate for such a theory. Besides strings, this framework also introduces other extended objects known as branes. These dynamical objects also gravitate, and a large number of them can be described in the supergravity limit of string theory as a black brane. -
Supersymmetry Breaking from a Calabi-Yau Singularity
hep-th/0505029 NSF-KITP-05-27 Supersymmetry Breaking from a Calabi-Yau Singularity D. Berenstein∗, C. P. Herzog†, P. Ouyang∗, and S. Pinansky∗ † Kavli Institute for Theoretical Physics ∗ Physics Department University of California University of California Santa Barbara, CA 93106, USA Santa Barbara, CA 93106, USA Abstract We conjecture a geometric criterion for determining whether supersymmetry is spon- taneously broken in certain string backgrounds. These backgrounds contain wrapped branes at Calabi-Yau singularites with obstructions to deformation of the complex structure. We motivate our conjecture with a particular example: the Y 2,1 quiver gauge theory corresponding to a cone over the first del Pezzo surface, dP1. This setup can be analyzed using ordinary supersymmetric field theory methods, where we find that gaugino condensation drives a deformation of the chiral ring which has no solu- tions. We expect this breaking to be a general feature of any theory of branes at a singularity with a smaller number of possible deformations than independent anomaly- arXiv:hep-th/0505029v2 7 May 2005 free fractional branes. May 2005 1 Introduction Supersymmetry and supersymmetry breaking are central ideas both in contemporary par- ticle physics and in mathematical physics. In this paper, we argue that for a large new class of D-brane models there exists a simple geometric criterion which determines whether supersymmetry breaking occurs. The models of interest are based on Calabi-Yau singularities with D-branes placed at or near the singularity. By taking a large volume limit, it is possible to decouple gravity from the theory, and ignore the Calabi-Yau geometry far from the branes. -
Singlet Glueballs in Klebanov-Strassler Theory
Singlet Glueballs In Klebanov-Strassler Theory A DISSERTATION SUBMITTED TO THE FACULTY OF THE GRADUATE SCHOOL OF THE UNIVERSITY OF MINNESOTA BY IVAN GORDELI IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF Doctor of Philosophy ARKADY VAINSHTEIN April, 2016 c IVAN GORDELI 2016 ALL RIGHTS RESERVED Acknowledgements First of all I would like to thank my scientific adviser - Arkady Vainshtein for his incredible patience and support throughout the course of my Ph.D. program. I would also like to thank my committee members for taking time to read and review my thesis, namely Ronald Poling, Mikhail Shifman and Alexander Voronov. I am deeply grateful to Vasily Pestun for his support and motivation. Same applies to my collaborators Dmitry Melnikov and Anatoly Dymarsky who have suggested this research topic to me. I am thankful to my other collaborator - Peter Koroteev. I would like to thank Emil Akhmedov, A.Yu. Morozov, Andrey Mironov, M.A. Olshanetsky, Antti Niemi, K.A. Ter-Martirosyan, M.B. Voloshin, Andrey Levin, Andrei Losev, Alexander Gorsky, S.M. Kozel, S.S. Gershtein, M. Vysotsky, Alexander Grosberg, Tony Gherghetta, R.B. Nevzorov, D.I. Kazakov, M.V. Danilov, A. Chervov and all other great teachers who have shaped everything I know about Theoretical Physics. I am deeply grateful to all my friends and colleagues who have contributed to discus- sions and supported me throughout those years including A. Arbuzov, L. Kushnir, K. Kozlova, A. Shestov, V. Averina, A. Talkachova, A. Talkachou, A. Abyzov, V. Poberezh- niy, A. Alexandrov, G. Nozadze, S. Solovyov, A. Zotov, Y. Chernyakov, N. -
Chaos in Matrix Models and Black Hole Evaporation
LLNL-JRNL-681857 UCB-PTH-16/01 SU-ITP-16/02 YITP-16-5 Chaos in Matrix Models and Black Hole Evaporation Evan Berkowitz,a1 Masanori Hanadabcd2 and Jonathan Maltzeb3 a Nuclear and Chemical Sciences Division, Lawrence Livermore National Laboratory, Livermore CA 94550, USA bStanford Institute for Theoretical Physics, Stanford University, Stanford, CA 94305, USA cYukawa Institute for Theoretical Physics, Kyoto University, Kitashirakawa Oiwakecho, Sakyo-ku, Kyoto 606-8502, Japan dThe Hakubi Center for Advanced Research, Kyoto University, Yoshida Ushinomiyacho, Sakyo-ku, Kyoto 606-8501, Japan e Berkeley Center for Theoretical Physics, University of California at Berkeley, Berkeley, CA 94720, USA Abstract Is the evaporation of a black hole described by a unitary theory? In order to shed light on this question |especially aspects of this question such as a black hole's negative specific heat|we consider the real-time dynamics of a solitonic object in matrix quantum mechanics, which can be interpreted as a black hole (black zero-brane) via holography. We point out that the chaotic nature of the system combined with the flat directions of its potential naturally leads to the emission of D0-branes from the black brane, which is suppressed in the large N limit. Simple arguments show that the black zero-brane, like the Schwarzschild black hole, arXiv:1602.01473v3 [hep-th] 15 Jan 2019 has negative specific heat, in the sense that the temperature goes up when it evaporates by emitting D0-branes. While the largest Lyapunov exponent grows during the evaporation, the Kolmogorov-Sinai entropy decreases. These are consequences of the generic properties of matrix models and gauge theory. -
What Lattice Theorists Can Do for Superstring/M-Theory
July 26, 2016 0:28 WSPC/INSTRUCTION FILE review˙2016July23 International Journal of Modern Physics A c World Scientific Publishing Company What lattice theorists can do for superstring/M-theory MASANORI HANADA Yukawa Institute for Theoretical Physics Kyoto University, Kyoto 606-8502, JAPAN The Hakubi Center for Advanced Research Kyoto University, Kyoto 606-8501, JAPAN Stanford Institute for Theoretical Physics Stanford University, Stanford, CA 94305, USA [email protected] The gauge/gravity duality provides us with nonperturbative formulation of superstring/M-theory. Although inputs from gauge theory side are crucial for answering many deep questions associated with quantum gravitational aspects of superstring/M- theory, many of the important problems have evaded analytic approaches. For them, lattice gauge theory is the only hope at this moment. In this review I give a list of such problems, putting emphasis on problems within reach in a five-year span, including both Euclidean and real-time simulations. Keywords: Lattice Gauge Theory; Gauge/Gravity Duality; Quantum Gravity. PACS numbers:11.15.Ha,11.25.Tq,11.25.Yb,11.30.Pb Preprint number:YITP-16-28 1. Introduction During the second superstring revolution, string theorists built a beautiful arXiv:1604.05421v2 [hep-lat] 23 Jul 2016 framework for quantum gravity: the gauge/gravity duality.1, 2 It claims that superstring/M-theory is equivalent to certain gauge theories, at least about certain background spacetimes (e.g. black brane background, asymptotically anti de-Sitter (AdS) spacetime). Here the word ‘equivalence’ would be a little bit misleading, be- cause it is not clear how to define string/M-theory nonperturbatively; superstring theory has been formulated based on perturbative expansions, and M-theory3 is defined as the strong coupling limit of type IIA superstring theory, where the non- perturbative effects should play important roles. -
VISCOSITY and BLACK HOLES 1 Introduction the Discovery Of
VISCOSITY AND BLACK HOLES D.T. SON Institute for Nuclear Theory, University of Washington, Seattle, WA 98195-1550, USA We review recent applications of the AdS/CFT correspondence in strongly coupled systems, in particular the quark gluon plasma. 1 Introduction The discovery of Hawking radiation1 confirmed that black holes are endowed with thermody- namic properties such as entropy and temperature, as first suggested by Bekenstein2 based on the analogy between black hole physics and equilibrium thermodynamics. For black branes, i.e., black holes with translationally invariant horizons, thermodynamics can be extended to hydrodynamics|the theory that describes long-wavelength deviations from thermal equilibrium. Thus, black branes possess hydrodynamic properties of continuous fluids and can be character- ized by kinetic coefficients such as viscosity, diffusion constants, etc. From the perspective of the holographic principle3;4, the hydrodynamic behavior of a black-brane horizon is identified with the hydrodynamic behavior of the dual theory. In this talk, we argue that in theories with gravity duals, the ratio of the shear viscosity to the volume density of entropy is equal to a universal value of ~=4π. A lot of attention has been given to this fact due to the discovery of a perfect liquid behavior at RHIC. We will also review recent attempts to extend AdS/CFT correspondence to nonrelativistic systems. 2 Dimension of η=s The standard textbook definition of the shear viscosity is as follows. Take two large parallel plates separated by a distance d. The space between the two plates is filled with a fluid. Let one plate moves relative to the other with a velocity v. -
The First Law of Black Brane Mechanics
DAMTP-2001-67 hep-th/0107228 THE FIRST LAW OF BLACK BRANE MECHANICS Paul K. Townsend and Marija Zamaklar DAMTP, University of Cambridge, Centre for Mathematical Sciences, Wilberforce Road, Cambridge CB3 0WA, UK ABSTRACT We obtain ADM and Komar surface integrals for the energy density, tension and angular momentum density of stationary p-brane solutions of Einstein’s equations. We use them to derive a Smarr-type formula for the energy den- sity and thence a first law of black brane mechanics. The intensive variable conjugate to the worldspace p-volume is an ‘effective’ tension that equals the ADM tension for uncharged branes, but vanishes for isotropic boost-invariant charged branes. 1 Introduction The status of energy in General Relativity is rather special because, for a general space- time, there is no coordinate-independent meaning to the energy in a given local region of a spacelike hypersurface. However, if the spacetime is asymptotically flat then it is possible to define a total energy, which can be expressed as an integral at spatial infinity: the ADM integral [1]. Consider an asymptotically flat spacetime, of d =1+n dimensions, for which the asymptotic form of the metric, in cartesian coordinates xM =(t; xi)(i =1;:::;n)is g η + h (1) MN ∼ MN MN where η is the Minkowski metric and h is a perturbation with the appropriate fall-off at spatial infinity needed to make the energy integral converge. We shall suppose that the action takes the form1 1 I = ddx det gR + I(mat) : (2) 2 Z p− The matter stress-tensor is 2 δI(mat) T (mat) = ; (3) MN −√ det g δgMN − and the Einstein field equation is (mat) GMN = TMN : (4) The ADM energy integral in these conventions is 1 E = dSi (@jhij @ihjj) : (5) 2 I − ∞ In the special case of a stationary asymptotically flat spacetime, for which there exists a normalized timelike Killing vector field k, the energy in any volume V with boundary @V can be expressed as the Komar integral [2] n 1 M N E(V )= − dSMND k : (6) − 4(n 2) Z − @V where dSMN is the co-dimension 2 surface element on the (n 1)-dimensional boundary @V of V . -
Ads Description of Induced Higher Spin Gauge Theories
UV Completion of Some UV Fixed Points Igor Klebanov Talk at ERG2016 Conference ICTP, Trieste September 23, 2016 Talk mostly based on • L. Fei, S. Giombi, IK, arXiv:1404.1094 • S. Giombi, IK, arXiv:1409.1937 • L. Fei, S. Giombi, IK, G. Tarnopolsky, arXiv:1411.1099 • L. Fei, S. Giombi, IK, G. Tarnopolsky, arXiv:1507.01960 • L. Fei, S. Giombi, IK, G. Tarnopolsky, arXiv:1607.05316 The Gross-Neveu Model • In 2 dimensions it has some similarities with the 4-dimensional QCD. • It is asymptotically free and exhibits dynamical mass generation. • Similar physics in the 2-d O(N) non-linear sigma model with N>2. • In dimensions slightly above 2 both the O(N) and GN models have weakly coupled UV fixed points. 2+ e expansion • The beta function and fixed-point coupling are • is the number of 2-component Majorana fermions. • Can develop 2+e expansions for operator scaling dimensions, e.g. Gracey; Kivel, Stepanenko, Vasiliev • Similar expansions in the O(N) sigma model with N>2. Brezin, Zinn-Justin 4-e expansion • The O(N) sigma model is in the same universality class as the O(N) model: • It has a weakly coupled Wilson-Fisher IR fixed point in 4-e dimensions. • Using the two e expansions, the scalar CFTs with various N may be studied in the range 2<d<4. This is an excellent practical tool for CFTs in d=3. The Gross-Neveu-Yukawa Model • The GNY model is the UV completion of the GN model in d<4 Zinn-Justin; Hasenfratz, Hasenfratz, Jansen, Kuti, Shen • IR stable fixed point in 4-e dimensions • Operator scaling dimensions • Using the two e expansions, we can study the Gross-Neveu CFTs in the range 2<d<4.