Homotopy and Super M-Branes
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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). -
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. -
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. -
Resolution of ADE Singularities
Resolution of Kleinian Singularities James J. Green April 25, 2014 abstract Firstly, the classification of finite subgroups of SL(2; C), a result of Felix Klein in 1884, is presented. The polynomial invariant subrings of these groups are then found. The generators of these subrings 3 satisfy a polynomial relation in three variables, which can be realised as a hypersurface in C . Each of these surfaces have a singularity at the origin; these are the Kleinian singularities. These singularities are blown-up, and their resolution graphs are shown to be precisely the Coxeter- Dynkin diagrams ADE. The target readership of this project is intended to be undergraduates with a foundational knowledge of group theory, topology and algebraic geometry. 1 1 Classifying the Finite Subgroups of SL(2; C) 1.1 Important Subgroups of the General Linear Group Recall: The general linear group of a vector space V over a field F is given by GL(V ) = ff : V −! V j f is linear and invertibleg: n In particular, we denote GL(F ) by GL(n; F). Since we can view linear maps as matrices, GL(n; F) can also be viewed as the set of invertible n × n matrices with entries in F. The next few definitions include important subgroups of GL(n; F). Definition 1.1. The special linear group over F is given by SL(n; F) = fA 2 GL(n; F) j det A = 1g: Definition 1.2. The orthogonal group over F is given by T O(n; F) = fA 2 GL(n; F) j AA = Ig where AT denotes the transpose of A, and I denotes the n × n identity matrix. -
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 . -
Swampland Constraints on 5D N = 1 Supergravity Arxiv:2004.14401V2
Prepared for submission to JHEP Swampland Constraints on 5d N = 1 Supergravity Sheldon Katz, a Hee-Cheol Kim, b;c Houri-Christina Tarazi, d Cumrun Vafa d aDepartment of Mathematics, MC-382, University of Illinois at Urbana-Champaign, Ur- bana, IL 61801, USA bDepartment of Physics, POSTECH, Pohang 790-784, Korea cAsia Pacific Center for Theoretical Physics, Postech, Pohang 37673, Korea dDepartment of Physics, Harvard University, Cambridge, MA 02138, USA Abstract: We propose Swampland constraints on consistent 5-dimensional N = 1 supergravity theories. We focus on a special class of BPS magnetic monopole strings which arise in gravitational theories. The central charges and the levels of current algebras of 2d CFTs on these strings can be calculated by anomaly inflow mechanism and used to provide constraints on the low-energy particle spectrum and the effective action of the 5d supergravity based on unitarity of the worldsheet CFT. In M-theory, where these theories are realized by compactification on Calabi-Yau 3-folds, the spe- cial monopole strings arise from wrapped M5-branes on special (\semi-ample") 4- cycles in the threefold. We identify various necessary geometric conditions for such cycles to lead to requisite BPS strings and translate these into constraints on the low-energy theories of gravity. These and other geometric conditions, some of which can be related to unitarity constraints on the monopole worldsheet, are additional arXiv:2004.14401v2 [hep-th] 13 Jul 2020 candidates for Swampland constraints on 5-dimensional N = 1 supergravity -
Thermal Giant Gravitons
NORDITA-2012-53 NSF-KITP-12-128 Thermal Giant Gravitons Jay Armas 1, Troels Harmark 2, Niels A. Obers 1, Marta Orselli 1 and Andreas Vigand Pedersen 1 1 The Niels Bohr Institute, Copenhagen University Blegdamsvej 17, DK-2100 Copenhagen Ø, Denmark 2 NORDITA Roslagstullsbacken 23, SE-106 91 Stockholm, Sweden [email protected], [email protected], [email protected] [email protected], [email protected] Abstract 5 We study the giant graviton solution as the AdS5 × S background is heated up to finite temperature. The analysis employs the thermal brane probe technique based on the blackfold approach. We focus mainly on the thermal giant graviton corresponding to a thermal D3- brane probe wrapped on an S3 moving on the S5 of the background at finite temperature. We find several interesting new effects, including that the thermal giant graviton has a minimal possible value for the angular momentum and correspondingly also a minimal possible radius of the S3. We compute the free energy of the thermal giant graviton in the low temperature arXiv:1207.2789v2 [hep-th] 3 Aug 2012 regime, which potentially could be compared to that of a thermal state on the gauge theory side. Moreover, we analyze the space of solutions and stability of the thermal giant graviton and find that, in parallel with the extremal case, there are two available solutions for a given temperature and angular momentum, one stable and one unstable. In order to write down the equations of motion, action and conserved charges for the thermal giant graviton we present a slight generalization of the blackfold formalism for charged black branes. -
Black Holes and String Theory
Black Holes and String Theory Hussain Ali Termezy Submitted in partial fulfilment of the requirements for the degree of Master of Science of Imperial College London September 2012 Contents 1 Black Holes in General Relativity 2 1.1 Black Hole Solutions . 2 1.2 Black Hole Thermodynamics . 5 2 String Theory Background 19 2.1 Strings . 19 2.2 Supergravity . 23 3 Type IIB and Dp-brane solutions 25 4 Black Holes in String Theory 33 4.1 Entropy Counting . 33 Introduction The study of black holes has been an intense area of research for many decades now, as they are a very useful theoretical construct where theories of quantum gravity become relevant. There are many curiosities associated with black holes, and the resolution of some of the more pertinent problems seem to require a quantum theory of gravity to resolve. With the advent of string theory, which purports to be a unified quantum theory of gravity, attention has naturally turned to these questions, and have remarkably shown signs of progress. In this project we will first review black hole solutions in GR, and then look at how a thermodynamic description of black holes is made possible. We then turn to introduce string theory and in particular review the black Dp-brane solutions of type IIB supergravity. Lastly we see how to compute a microscopic account of the Bekenstein entropy is given in string theory. 1 Chapter 1 Black Holes in General Relativity 1.1 Black Hole Solutions We begin by reviewing some the basics of black holes as they arise in the study of general relativity. -
Tasi Lectures on Branes, Black Holes and Anti-De Sitter Space1
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server UM-TH-99-07 hep-th/9912164 TASI LECTURES ON BRANES, BLACK HOLES AND ANTI-DE SITTER SPACE1. M. J. Duff2 Randall Laboratory, Department of Physics, University of Michigan, Ann Arbor, MI 48109-1120 ABSTRACT In the light of the duality between physics in the bulk of anti-de Sitter space and a conformal field theory on the boundary, we review the M2, D3andM5 branes and how their near-horizon geometry yields the compactification of D =11supergravityonS7, Type IIB supergravity on S5 and D =11supergravityonS4, respectively. We discuss the “Membrane at the End of the Universe” idea and its relation to the corresponding superconformal singleton theories that live on the boundary of the AdS4, AdS5 and AdS7 vacua. The massless sectors of these compactifications are described by the maximally supersymmetric D =4,D=5andD= 7 gauged supergravities. We construct the non-linear Kaluza-Klein ans¨atze describing the embeddings of the U(1)4, U(1)3 and U(1)2 truncations of these supergravities, which admit 4-charge AdS4,3-chargeAdS5 and 2- charge AdS7 black hole solutions. These enable us to embed the black hole solutions back in ten and eleven dimensions and reinterpret them as M2, D3andM5 branes spinning in the transverse dimensions with the black hole charges given by the angular momenta of the branes. A comprehensive Appendix lists the field equations, symmetries and transformation rules of D =11supergravity,TypeIIB supergravity, and the M2, D3andM5branes. 1Based on talks delivered at the Theoretical Advanced Study Institute, Boulder, Colorado, June 1999 and the Banff Summer School, Alberta, Canada, June-July 1999. -
Holography of Electrically and Magnetically Charged Black Branes
Eur. Phys. J. C (2019) 79:195 https://doi.org/10.1140/epjc/s10052-019-6705-8 Regular Article - Theoretical Physics Holography of electrically and magnetically charged black branes Zhenhua Zhou1,a, Jian-Pin Wu2,4,b,YiLing3,4,5,c 1 School of Physics and Electronic Information, Yunnan Normal University, Kunming 650500, China 2 Center for Gravitation and Cosmology, College of Physical Science and Technology, Yangzhou University, Yangzhou 225009, China 3 Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China 4 Shanghai Key Laboratory of High Temperature Superconductors, Shanghai 200444, China 5 School of Physics, University of Chinese Academy of Sciences, Beijing 100049, China Received: 3 December 2018 / Accepted: 19 February 2019 / Published online: 4 March 2019 © The Author(s) 2019 Abstract We construct a new class of black brane solu- ity and quadratic-T inverse Hall angle can be simultaneously tions in Einstein-Maxwell-dilaton (EMD) theory, which is reproduced in some special holographic models [19–23]. characterized by two parameters a, b. Based on the obtained Currently it is still challenging to achieve the anomalous solutions, we make detailed analysis on the ground state in scales of strange metal over a wide range of temperature zero temperature limit and find that for many cases it exhibits in holographic approach. It may be limited by the renor- the behavior of vanishing entropy density. We also find that malization group flow which is controlled by the specific the linear-T resistivity can be realized in a large region of bulk geometry subject to Einstein field equations, and the temperature for the specific case of a2 = 1/3, which is the scaling behavior of the near horizon geometry of the back- Gubser-Rocha model dual to a ground state with vanishing ground.