Gravitons, Inflatons, Twisted Bits
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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. -
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 -
Quantum Symmetries and Stringy Instantons
PUPT–1464 hep-th@xxx/9406091 Quantum Symmetries and Stringy Instantons ⋆ Jacques Distler and Shamit Kachru† Joseph Henry Laboratories Princeton University Princeton, NJ 08544 USA The quantum symmetry of many Landau-Ginzburg orbifolds appears to be broken by Yang-Mills instantons. However, isolated Yang-Mills instantons are not solutions of string theory: They must be accompanied by gauge anti-instantons, gravitational instantons, or topologically non-trivial configurations of the H field. We check that the configura- tions permitted in string theory do in fact preserve the quantum symmetry, as a result of non-trivial cancellations between symmetry breaking effects due to the various types arXiv:hep-th/9406091v1 14 Jun 1994 of instantons. These cancellations indicate new constraints on Landau-Ginzburg orbifold spectra and require that the dilaton modulus mix with the twisted moduli in some Landau- Ginzburg compactifications. We point out that one can find similar constraints at all fixed points of the modular group of the moduli space of vacua. June 1994 †Address after June 30: Department of Physics, Harvard University, Cambridge, MA 02138. ⋆ Email: [email protected], [email protected] . Research supported by NSF grant PHY90-21984, and the A. P. Sloan Foundation. 1. Introduction Landau-Ginzburg orbifolds [1,2] describe special submanifolds in the moduli spaces of Calabi-Yau models, at “very small radius.” New, stringy features of the physics are therefore often apparent in the Landau-Ginzburg theories. For example, these theories sometimes manifest enhanced gauge symmetries which do not occur in the field theory limit, where the large radius manifold description is valid. -
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. -
Inflation in String Theory: - Towards Inflation in String Theory - on D3-Brane Potentials in Compactifications with Fluxes and Wrapped D-Branes
1935-6 Spring School on Superstring Theory and Related Topics 27 March - 4 April, 2008 Inflation in String Theory: - Towards Inflation in String Theory - On D3-brane Potentials in Compactifications with Fluxes and Wrapped D-branes Liam McAllister Department of Physics, Stanford University, Stanford, CA 94305, USA hep-th/0308055 SLAC-PUB-9669 SU-ITP-03/18 TIFR/TH/03-06 Towards Inflation in String Theory Shamit Kachru,a,b Renata Kallosh,a Andrei Linde,a Juan Maldacena,c Liam McAllister,a and Sandip P. Trivedid a Department of Physics, Stanford University, Stanford, CA 94305, USA b SLAC, Stanford University, Stanford, CA 94309, USA c Institute for Advanced Study, Princeton, NJ 08540, USA d Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400 005, INDIA We investigate the embedding of brane inflation into stable compactifications of string theory. At first sight a warped compactification geometry seems to produce a naturally flat inflaton potential, evading one well-known difficulty of brane-antibrane scenarios. Care- arXiv:hep-th/0308055v2 23 Sep 2003 ful consideration of the closed string moduli reveals a further obstacle: superpotential stabilization of the compactification volume typically modifies the inflaton potential and renders it too steep for inflation. We discuss the non-generic conditions under which this problem does not arise. We conclude that brane inflation models can only work if restric- tive assumptions about the method of volume stabilization, the warping of the internal space, and the source of inflationary energy are satisfied. We argue that this may not be a real problem, given the large range of available fluxes and background geometries in string theory. -
Some Comments on Equivariant Gromov-Witten Theory and 3D Gravity (A Talk in Two Parts) This Theory Has Appeared in Various Interesting Contexts
Some comments on equivariant Gromov-Witten theory and 3d gravity (a talk in two parts) This theory has appeared in various interesting contexts. For instance, it is a candidate dual to (chiral?) supergravity with deep negative cosmologicalShamit constant. Kachru Witten (Stanford & SLAC) Sunday, April 12, 15 Tuesday, August 11, 15 Much of the talk will be review of things well known to various parts of the audience. To the extent anything very new appears, it is based on two recent collaborative papers: * arXiv : 1507.00004 with Benjamin, Dyer, Fitzpatrick * arXiv : 1508.02047 with Cheng, Duncan, Harrison Some slightly older work with other (also wonderful) collaborators makes brief appearances. Tuesday, August 11, 15 Today, I’d like to talk about two distinct topics. Each is related to the general subjects of this symposium, but neither has been central to any of the talks we’ve heard yet. 1. Extremal CFTs and quantum gravity ...where we see how special chiral CFTs with sparse spectrum may be important in gravity... II. Equivariant Gromov-Witten & K3 ...where we see how certain enumerative invariants of K3 may be related to subjects we’ve heard about... Tuesday, August 11, 15 I. Extremal CFTs and quantum gravity A fundamental role in our understanding of quantum gravity is played by the holographic correspondence between conformal field theories and AdS gravity. In the basic dictionary between these subjects conformal symmetry AdS isometries $ primary field of dimension ∆ bulk quantum field of mass m(∆) $ ...... Tuesday, August 11, 15 -
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. -
Non-Higgsable Clusters for 4D F-Theory Models
Non-Higgsable clusters for 4D F-theory models The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Morrison, David R., and Washington Taylor. “Non-Higgsable Clusters for 4D F-Theory Models.” J. High Energ. Phys. 2015, no. 5 (May 2015). As Published http://dx.doi.org/10.1007/jhep05(2015)080 Publisher Springer-Verlag Version Final published version Citable link http://hdl.handle.net/1721.1/98237 Terms of Use Creative Commons Attribution Detailed Terms http://creativecommons.org/licenses/by/4.0/ Published for SISSA by Springer Received: January 6, 2015 Accepted: April 18, 2015 Published: May 18, 2015 Non-Higgsable clusters for 4D F-theory models JHEP05(2015)080 David R. Morrisona and Washington Taylorb aDepartments of Mathematics and Physics, University of California, Santa Barbara, Santa Barbara, CA 93106, U.S.A. bCenter for Theoretical Physics, Department of Physics, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, U.S.A. E-mail: [email protected], [email protected] Abstract: We analyze non-Higgsable clusters of gauge groups and matter that can arise at the level of geometry in 4D F-theory models. Non-Higgsable clusters seem to be generic features of F-theory compactifications, and give rise naturally to structures that include the nonabelian part of the standard model gauge group and certain specific types of potential dark matter candidates. In particular, there are nine distinct single nonabelian gauge group factors, and only five distinct products of two nonabelian gauge group factors with matter, including SU(3) × SU(2), that can be realized through 4D non-Higgsable clusters. -
Arxiv:1808.09134V2 [Hep-Th] 24 Sep 2018
KIAS-P18089 Algebraic surfaces, Four-folds and Moonshine Kimyeong Lee1, ∗ and Matthieu Sarkis1, y 1School of Physics, Korea Institute for Advanced Study, Seoul 02455, Korea The aim of this note is to point out an interesting fact related to the elliptic genus of complex algebraic surfaces in the context of Mathieu moonshine. We also discuss the case of 4-folds. INTRODUCTION terms of the holomorphic Euler characteristic of a for- mal series with holomorphic vector bundle coefficients. In their seminal paper [1], Eguchi, Ooguri and We give for it a simple expression in terms the self- Tachikawa made the interesting observation that the el- intersection number of the canonical class and the Euler liptic genus of K3 admits a decomposition in terms of number. One can then deduce the behaviour of the ellip- N = 4 super-Virasoro characters, whose coefficients hap- tic genus under blow ups, allowing us to state in which 2 pen to correspond to the dimension of representations sense any surface with positive K may be relevant for a geometric understanding of Mathieu moonshine. of the largest Mathieu sporadic group M24. This phe- nomenon was formalized in a precise conjecture related We finally discuss how the discussion for surfaces can be extended for 4-folds. to the existence of a graded module for M24 whose prop- erties would precisely mimic the experimental observa- tion of [1]. This conjecture was then proved by Gan- Conventions: non [2]. Many authors have made important contribu- • We will omit the modular argument and denote tions towards understanding Mathieu moonshine from by θ(z) the odd Jacobi theta function θ(τ; z) when a physics perspective in terms of the BPS spectrum of unambiguous, cf. -
Vacua with Small Flux Superpotential
Vacua with Small Flux Superpotential Mehmet Demirtas,∗ Manki Kim,y Liam McAllister,z and Jakob Moritzx Department of Physics, Cornell University, Ithaca, NY 14853, USA (Dated: February 4, 2020) We describe a method for finding flux vacua of type IIB string theory in which the Gukov-Vafa- −8 Witten superpotential is exponentially small. We present an example with W0 ≈ 2 × 10 on an orientifold of a Calabi-Yau hypersurface with (h1;1; h2;1) = (2; 272), at large complex structure and weak string coupling. 1. INTRODUCTION In x2 we present a general method for constructing vacua with small W0 at large complex structure (LCS) To understand the nature of dark energy in quantum and weak string coupling, building on [9, 10]. In x3 we 1 −8 gravity, one can study de Sitter solutions of string theory. give an explicit example where W0 ≈ 2 × 10 , in an Kachru, Kallosh, Linde, and Trivedi (KKLT) have ar- orientifold of a Calabi-Yau hypersurface in CP[1;1;1;6;9]. gued that there exist de Sitter vacua in compactifications In x4 we show that our result accords well with the sta- on Calabi-Yau (CY) orientifolds of type IIB string theory tistical predictions of [4]. We show in x5 that at least one [1]. An essential component of the KKLT scenario is a complex structure modulus in our example is as light as small vacuum value of the classical Gukov-Vafa-Witten the K¨ahlermoduli. We explain why this feature occurs in [2] flux superpotential, our class of solutions, and we comment on K¨ahlermoduli stabilization in our vacuum. -
Shamit Kachru Professor of Physics and Director, Stanford Institute for Theoretical Physics
Shamit Kachru Professor of Physics and Director, Stanford Institute for Theoretical Physics CONTACT INFORMATION • Administrative Contact Dan Moreau Email [email protected] Bio BIO Starting fall of 2021, I am winding down a term as chair of physics and then taking an extended sabbatical/leave. My focus during this period will be on updating my background and competence in rapidly growing new areas of interest including machine learning and its application to problems involving large datasets. My recent research interests have included mathematical and computational studies of evolutionary dynamics; field theoretic condensed matter physics, including study of non-Fermi liquids and fracton phases; and mathematical aspects of string theory. I would characterize my research programs in these three areas as being in the fledgling stage, relatively recently established, and well developed, respectively. It is hard to know what the future holds, but you can get some idea of the kinds of things I work on by looking at my past. Highlights of my past research include: - The discovery of string dualities with 4d N=2 supersymmetry, and their use to find exact solutions of gauge theories (with Cumrun Vafa) - The construction of the first examples of AdS/CFT duality with reduced supersymmetry (with Eva Silverstein) - Foundational papers on string compactification in the presence of background fluxes (with Steve Giddings and Joe Polchinski) - Basic models of cosmic acceleration in string theory (with Renata Kallosh, Andrei Linde, and Sandip Trivedi) -
String Cosmology
��������� � ������ ������ �� ��������� ��� ������������� ������� �� � �� ���� ���� ������ ��������� ���� � �� ������� ���������� �� �������� ���������� �� ������� ��������� �� ���������� ������ Lecture 2 Stabilization of moduli in superstring theory Fluxes NS (perturbative string theory) RR (non-perturbative string theory) Non-perturbative corrections to superpotential and Kahler potential Start 2008 Higgs?Higgs? MSSM?MSSM? SplitSplit susysusy?? NoNo susysusy?? IFIF SUSYSUSY ISIS THERETHERE…… The significance of discovery of supersymmetry in nature, which will manifests itself via existence of supersymmetric particles, would be a discovery of the fermionicfermionic dimensionsdimensions ofof spacetimespacetime ItIt willwill bebe thethe mostmost fundamentalfundamental discoverydiscovery inin physicsphysics afterafter EinsteinEinstein’’ss relativityrelativity SUPERSYMMETRY: GravityGravity Supergravity/StringSupergravity/String theorytheory There are no single scalars fields in susy models! Scalars come in pairs, they are always complex in supersymmetry. For example, axion and dilaton or axion and radial modulus. Generically, multi-dimensional moduli space. An effective inflaton may be a particular direction in moduli space. In string theory scalars often have geometrical meaning: distance between branes, size of internal dimensions, size of supersymmetric cycles on which branes can be wrapped, etc StabilizationStabilization ofof modulimoduli isis necessarynecessary forfor stringstring theorytheory toto describedescribe thethe effectiveeffective