Spacetime Quantum Geometry
|
|
- Alfred Sullivan
- 5 years ago
- Views:
Transcription
1 Spacetime Quantum Geometry Peter Schupp Jacobs University Bremen 4th Scienceweb GCOE International Symposium Tohoku University 2012
2 Outline Spacetime quantum geometry Applying the principles of quantum mechanics to space & time Outline spacetime non-commutativity particle physics on non-commutative spaces non-commutative gravity and fuzzy black holes large scale application of small scale math (CMB analysis) higher geometric structures
3 Spacetime non-commutativity Planck scale quantum geometry Heuristic argument: quantum + gravity The gravitational field generated by the concentration of energy required to localize an event in spacetime should not be so strong as to hide the event itself to a distant observer. fundamental length scale, spacetime uncertainty x G c cm uncertainty principle noncommutative spacetime structure [ˆx i, ˆx j ] = iθ ij (x)
4 Spacetime non-commutativity Macroscopic non-commutativity Landau levels charged particle in a constant magnetic field B = A: quantize p = m x e A conjugate to x for m 0 (projection onto 1st Landau level): [ˆx i, ˆx j ] = 2i eb ɛij =: θ ij Fractional Quantum Hall Effect Non-commutative (NC) fluids, NC Chern Simons theory
5 Spacetime non-commutativity Loop quantum gravity, spacetime foam non-perturbative framework defines quantum spacetime in algebraic terms integrating out gravitational degrees of freedom appears to yield effective NC actions with Lie-type NC structure [ˆx i, ˆx j ] = iκ ɛ ijk ˆx k, κ = 4πG (κ-minkowski space) (feasible so far only for 2+1 dimensions)
6 Spacetime non-commutativity Non-commutativity in string theory effective dynamics of open strings ending on D-branes: non-abelian gauge theory in closed string background B-field non-commutative gauge theory string endpoints become non-commutative: f 1 (x(τ 1 ))... f n (x(τ n )) = dx f 1... f n, τ 1 <... < τ n with star product depending on B.
7 Spacetime non-commutativity Star product General x-dependent NC structure: f g = f g + i θ ij i f j g 2 θ ij θ kl i k f j l g ( θ ij j θ kl i k f l g k f i l g) on coordinates: [x i, x j ] = iθ ij
8 Spacetime non-commutativity How does a quantum space look like?
9 Spacetime non-commutativity How does a quantum space look like?
10 Spacetime non-commutativity How does a quantum space look like? (q-minkowski space; Cerchiai, Wess 1998)
11 Particle physics on non-commutative spaces Quantum/Noncommutative Spacetime model of quantum geometry, spacetime uncertainty Particle physics on non-commutative spaces construction of QFT on quantum spacetime experimental signatures? Features controlled Lorentz violation, non-locality, UV/IR mixing, mixing of internal & spacetime symmetries
12 Particle physics on non-commutative spaces Non-commutative Standard Model I Connes, Lott; Madore (+ many others) spacetime augmented by a discrete space Higgs field is NC gauge potential in the discrete direction beautiful geometrical interpretation of the full SM unlucky prediction of the Higgs mass
13 Particle physics on non-commutative spaces Non-commutative Standard Model II Calmet, Jurco, PS, Wess, Wohlgenannt (+ many others) deformed spacetime with -product particle content and structure group of undeformed SM enveloping algebra formalism, SW maps many new SM forbidden interactions
14 Particle physics on non-commutative spaces Star product and Seiberg-Witten map Star product: f g = fg θµν µ f ν g Corresponding expansion of fields via SW map: Â µ [A, θ] = A µ θξν {A ν, ξ A µ + F ξµ } +... Ψ[Ψ, A, θ] = Ψ θµν A ν µ Ψ θµν µ A ν Ψ +... Λ[Λ, A, θ] = Λ θξν {A ν, ξ Λ} +...
15 Particle physics on non-commutative spaces Deformed action Matrix multiplication is augmented by -products. e.g.: noncommutative Yang-Mills-Dirac action: ( Ŝ = d 4 x 1 ) 4 Tr( F µν F µν ) + Ψ i D/ Ψ with NC field strength F µν = µ Â ν ν Â µ i[âµ, Âν]
16 Particle physics on non-commutative spaces Non-perturbative effects at the quantum level Beta function of U(N) NC Yang-Mills theory: β(g 2 ) = g2 ln Λ = 22 3 g 4 N 2 8π 2 like ordinary SU(N) gauge theory but holds also for N = 1 This U(1) NC gauge theory is asymptotically free with strong coupling effects at large distance scales.
17 Particle physics on non-commutative spaces Photon neutrino interaction neutral particles can interact with photons via -commutator D µ Ψ = µ Ψ i[a µ, Ψ] 1-loop contributions to neutrino self-energy:
18 Particle physics on non-commutative spaces Superluminal neutrinos? deformed dispersion relation ( ) p 2 8π 2 e 2 1 ( 8π 2 ± 2 ) 1 2 e 2 1 } {{ } constant k, independent of θ direction dependent neutrino velocity E 2 = p 2 c 2 (1 + k sin 2 θ). pr 2, Horvat, Ilakovac, PS, Trampetic, You: arxiv: v1 [hep-th]
19 Non-commutative gravity Non-commutative gravity and exact solutions Gravity on non-commutative spacetime Fuzzy black hole solutions
20 Non-commutative gravity Motivation Quantum black holes nice theoretical laboratory for physics beyond QFT/GR information paradox, entropy, holography, singularities,... Major obstacle The existence of a fundamental length scale is a priori incompatible with spacetime symmetries The symmetry (Hopf algebra) must be deformed
21 Non-commutative gravity Drinfel d twisted symmetry: F = exp ( i2 ) θab V a V b, [V a, V b ] = 0 (f ) = F (f )F 1 f g = F(f g) Twisted tensor calculus Two simple rules: The transformation of individual tensors is not deformed Tensors must be -multiplied Twisted quantization, Hopf algebra symmetry in string theory: Asakawa, Watamura (Tohoku University) afternoon session: T. Asakawa NC solitions of gravity
22 Non-commutative gravity Drinfel d twisted symmetry: F = exp ( i2 ) θab V a V b, [V a, V b ] = 0 (f ) = F (f )F 1 f g = F(f g) Twisted tensor calculus Two simple rules: The transformation of individual tensors is not deformed Tensors must be -multiplied Twisted quantization, Hopf algebra symmetry in string theory: Asakawa, Watamura (Tohoku University) afternoon session: T. Asakawa NC solitions of gravity
23 Non-commutative gravity Deformed Einstein equations with non-commutative sources T µν R µν (G, ) = T µν 1 2 G µνt Solutions? Solution = mutually compatible pair: algebra (twist) metric G µν
24 Non-commutative black hole Exact solution with rotational symmetry Star product (twist) for tensors: V W = VW + C n ( λ ρ )Ln ξ + V L n ξ W n=1 left invariant Killing vector fields: ξ ± = ξ 1 ± iξ 2 commutative radius: ρ 2 = x 2 + y 2 + z 2 C n ( λ ρ ) = B(n, ρ λ ) = λ n n! ρ(ρ λ)(ρ 2λ) (ρ (n 1)λ)
25 Non-commutative black hole Metric in isotropic coordinates ( ds 2 = 1 a ) dt 2 + r 2 ρ ρ 2 (dx 2 + dy 2 + dz 2 ) with r = (ρ + a/4) 2 /ρ, a = 2M ρ 2 = g ij x i x j = x 2 + y 2 + z 2 [x i, x j ] = 2iλɛ ijk x k quantized, quasi 2-dimensional onion -spacetime: ρ = 2jλ = nλ; n = 0, 1, 2,...
26 Non-commutative black hole
27 Non-commutative black hole
28 Non-commutative black hole
29 Non-commutative black hole
30 Hilbert Space L 2 (R 3 ) L 2 (S 2 ) We find the following surprising result: States describing events in 3 dim NC bulk are equivalent to wave functions on a sphere (minus a fuzzy sphere) H = n>n C n+1 = C n+1 H hidden NC Schwarzschild solution = Fuzzy Black Hole Holographic behavior appears quite naturally NC: bulk (3D) surface (2D) Heuristically: (1) coordinates are no longer independent: z [x, y] (2) number of commuting operators = two
31 Inside NC black hole two sequences of fuzzy spheres with limit points at r = 0 (singularity) and r = a (horizon)
32 Non-commutative black hole Fuzzy black hole inside and outside, in one figure:
33 Coherent States, Star Products, Entropy Generalized coherent state (SU(2), spin j representation) dω Ω = R Ω j, j, R Ω SU(2)/U(1); (2j+1) 4π Ω Ω = 1 j Star product For A(Ω) := Ω A Ω and B(Ω) := Ω B Ω define: A(Ω) B(Ω) = Ω AB Ω
34 Coherent States, Star Products, Entropy Von Neumann entropy S Q (ρ) = trρ ln ρ = (2j + 1) dω 4π ρ(ω) ln ρ(ω) Now switch off (or ignore) noncommutativity Wehrl entropy dω S W (ρ) = (2j + 1) ρ(ω) ln ρ(ω) 4π dω (2j + 1) 4π Ω Ψ 2 ln Ω Ψ 2 > 0 even for pure states
35 Coherent states and CMB Coherent state analysis of CMB pseudo entropy l
36 Coherent states and CMB CMB at j = 5 with multi-pole vectors ( coherent states)
37 Coherent states and CMB CMB at j = 28
38 Higher geometric structures Beyond non-commutative Recent work in M-theory reveales non-associative higher geometric structures featuring Nambu brackets: Basu-Harvey equations, fuzzy S 3 funnels Bagger-Lambert action for multiple M2 and M5-branes afternoon session: M. Sato 3-algebra Model of M-Theory
39 Higher geometric structures Nambu mechanics multi-hamiltonian dynamics with generalized Poisson brackets e.g. Euler s equations for the spinning top : d dt L i = {L i, L 2, T } i = 1, 2, 3 2 with angular momenta L 1, L 2, L 2, kinetic energy T = L 2 i 2I i Nambu-Poisson bracket [ ] (f, g, h) {f, g, h} det = ɛ ijk i f j g k h (L 1, L 2, L 3 ) and
40 Higher geometric structures Nambu-Poisson (NP) bracket more generally: {f, h 1,..., h p } = Π i j 1...j p (x) i f j1 h 1 jp h p + Fundamental Identity (FI) {{f 0,, f p }, h 1,, h p } = {{f 0, h 1,, h p }, f 1,, f p } {f 0,..., f p 1, {f p, h 1,, h p }}
41 Higher geometric structures Nambu-Dirac-Born-Infeld action (B Jurco & PS 2012) commutative non-commutative symmetry implies S DBI = d n x 1 p 1 [ det 2(p+1) [g] det 2(p+1) g + (B + F) g 1 (B + F) T ] g m = d n x 1 p [Ĝ] 1 [Ĝ+(ˆΦ+ˆF) G 1 det 2(p+1) det 2(p+1) (ˆΦ+ˆF) T ] G m This action interpolates between early proposals based on supersymmetry and more recent work featuring higher geometric structures.
42 Thank you for listening!
Membrane σ-models and quantization of non-geometric flux backgrounds
Membrane σ-models and quantization of non-geometric flux backgrounds Peter Schupp Jacobs University Bremen ASC workshop Geometry and Physics Munich, November 19-23, 2012 joint work with D. Mylonas and
More informationChern-Simons Theory and Its Applications. The 10 th Summer Institute for Theoretical Physics Ki-Myeong Lee
Chern-Simons Theory and Its Applications The 10 th Summer Institute for Theoretical Physics Ki-Myeong Lee Maxwell Theory Maxwell Theory: Gauge Transformation and Invariance Gauss Law Charge Degrees of
More informationκ = f (r 0 ) k µ µ k ν = κk ν (5)
1. Horizon regularity and surface gravity Consider a static, spherically symmetric metric of the form where f(r) vanishes at r = r 0 linearly, and g(r 0 ) 0. Show that near r = r 0 the metric is approximately
More informationNon-associative Deformations of Geometry in Double Field Theory
Non-associative Deformations of Geometry in Double Field Theory Michael Fuchs Workshop Frontiers in String Phenomenology based on JHEP 04(2014)141 or arxiv:1312.0719 by R. Blumenhagen, MF, F. Haßler, D.
More informationWorkshop on Testing Fundamental Physics Principles Corfu, September 22-28, 2017.
Workshop on Testing Fundamental Physics Principles Corfu, September 22-28, 2017.. Observables and Dispersion Relations in κ-minkowski and κ-frw noncommutative spacetimes Paolo Aschieri Università del Piemonte
More informationSymmetries, Horizons, and Black Hole Entropy. Steve Carlip U.C. Davis
Symmetries, Horizons, and Black Hole Entropy Steve Carlip U.C. Davis UC Davis June 2007 Black holes behave as thermodynamic objects T = κ 2πc S BH = A 4 G Quantum ( ) and gravitational (G) Does this thermodynamic
More informationQuantum Nambu Geometry in String Theory
in String Theory Centre for Particle Theory and Department of Mathematical Sciences, Durham University, Durham, DH1 3LE, UK E-mail: chong-sun.chu@durham.ac.uk Proceedings of the Corfu Summer Institute
More informationNoncommutative Scalar Quasinormal Modes of the ReissnerNordström Black Hole
Corfu Summer Institute Training School Quantum Spacetime and Physics Models Corfu, September 16-23, 2017 Noncommutative Scalar Quasinormal Modes of the ReissnerNordström Black Hole University of Belgrade,
More informationTwist deformation quantization, gravity and Einstein spaces. Paolo Aschieri U.Piemonte Orientale, Alessandria
Bayrischzell 15.5.2010 Noncommutativity and Physics: Spacetime Quantum Geometry Twist deformation quantization, gravity and Einstein spaces Paolo Aschieri U.Piemonte Orientale, Alessandria I recall the
More informationHolographic entanglement entropy
Holographic entanglement entropy Mohsen Alishahiha School of physics, Institute for Research in Fundamental Sciences (IPM) 21th Spring Physics Conference, 1393 1 Plan of the talk Entanglement entropy Holography
More informationNoncommutative Spacetime Geometries
Munich 06.11.2008 Noncommutative Spacetime Geometries Paolo Aschieri Centro Fermi, Roma, U.Piemonte Orientale, Alessandria Memorial Conference in Honor of Julius Wess I present a general program in NC
More informationNoncommutative Geometry for Quantum Spacetime
Noncommutative Geometry for Quantum Spacetime The view from below Fedele Lizzi Università di Napoli Federico II Institut de Ciencies del Cosmo, Barcelona SIGrav, Alessandria 2014 I think we would all agree
More informationThe Phase Diagram of the BMN Matrix Model
Denjoe O Connor School of Theoretical Physics Dublin Institute for Advanced Studies Dublin, Ireland Workshop on Testing Fundamental Physics Principles Corfu2017, 22-28th September 2017 Background: V. Filev
More informationSPACETIME FROM ENTANGLEMENT - journal club notes -
SPACETIME FROM ENTANGLEMENT - journal club notes - Chris Heinrich 1 Outline 1. Introduction Big picture: Want a quantum theory of gravity Best understanding of quantum gravity so far arises through AdS/CFT
More informationGravity, Strings and Branes
Gravity, Strings and Branes Joaquim Gomis Universitat Barcelona Miami, 23 April 2009 Fundamental Forces Strong Weak Electromagnetism QCD Electroweak SM Gravity Standard Model Basic building blocks, quarks,
More informationQuantum Gravity and Black Holes
Quantum Gravity and Black Holes Viqar Husain March 30, 2007 Outline Classical setting Quantum theory Gravitational collapse in quantum gravity Summary/Outlook Role of metrics In conventional theories the
More informationGeneral Relativity and Cosmology Mock exam
Physikalisches Institut Mock Exam Universität Bonn 29. June 2011 Theoretische Physik SS 2011 General Relativity and Cosmology Mock exam Priv. Doz. Dr. S. Förste Exercise 1: Overview Give short answers
More informationHolography and (Lorentzian) black holes
Holography and (Lorentzian) black holes Simon Ross Centre for Particle Theory The State of the Universe, Cambridge, January 2012 Simon Ross (Durham) Holography and black holes Cambridge 7 January 2012
More informationGravity, Strings and Branes
Gravity, Strings and Branes Joaquim Gomis International Francqui Chair Inaugural Lecture Leuven, 11 February 2005 Fundamental Forces Strong Weak Electromagnetism QCD Electroweak SM Gravity Standard Model
More informationEMERGENT GEOMETRY FROM QUANTISED SPACETIME
EMERGENT GEOMETRY FROM QUANTISED SPACETIME M.SIVAKUMAR UNIVERSITY OF HYDERABAD February 24, 2011 H.S.Yang and MS - (Phys Rev D 82-2010) Quantum Field Theory -IISER-Pune Organisation Quantised space time
More informationHolography for 3D Einstein gravity. with a conformal scalar field
Holography for 3D Einstein gravity with a conformal scalar field Farhang Loran Department of Physics, Isfahan University of Technology, Isfahan 84156-83111, Iran. Abstract: We review AdS 3 /CFT 2 correspondence
More informationOn divergent 3-vertices in noncommutative SU(2) gauge theory
On divergent 3-vertices in noncommutative SU2 gauge theory arxiv:hep-th/0410085v1 8 Oct 2004 Maja Burić and Voja Radovanović Faculty of Physics, P.O. Box 368, 11001 Belgrade, Serbia and Montenegro Abstract
More informationGlobal Seiberg-Witten quantization for U(n)-bundles on tori
Global Seiberg-Witten quantization for U(n)-bundles on tori Andreas Deser 1,2 Based on arxiv:1809.05426 with Paolo Aschieri 2,3 1 Faculty of Mathematics and Physics, Charles University, Prague 2 Istituto
More informationApproaches to Quantum Gravity A conceptual overview
Approaches to Quantum Gravity A conceptual overview Robert Oeckl Instituto de Matemáticas UNAM, Morelia Centro de Radioastronomía y Astrofísica UNAM, Morelia 14 February 2008 Outline 1 Introduction 2 Different
More informationConnection Variables in General Relativity
Connection Variables in General Relativity Mauricio Bustamante Londoño Instituto de Matemáticas UNAM Morelia 28/06/2008 Mauricio Bustamante Londoño (UNAM) Connection Variables in General Relativity 28/06/2008
More informationQuantization of 2-plectic Manifolds
School of Mathematical and Computer Sciences Heriot Watt University, Edinburgh Based on: Bayrischzell Workshop, 22.5.2011 Josh DeBellis, CS and Richard Szabo arxiv:1001.3275 (JMP), arxiv:1012.2236 (JHEP)
More informationAnalog Duality. Sabine Hossenfelder. Nordita. Sabine Hossenfelder, Nordita Analog Duality 1/29
Analog Duality Sabine Hossenfelder Nordita Sabine Hossenfelder, Nordita Analog Duality 1/29 Dualities A duality, in the broadest sense, identifies two theories with each other. A duality is especially
More informationQuantization of the open string on exact plane waves and non-commutative wave fronts
Quantization of the open string on exact plane waves and non-commutative wave fronts F. Ruiz Ruiz (UCM Madrid) Miami 2007, December 13-18 arxiv:0711.2991 [hep-th], with G. Horcajada Motivation On-going
More information8.821 String Theory Fall 2008
MIT OpenCourseWare http://ocw.mit.edu 8.821 String Theory Fall 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. 8.821 F2008 Lecture 03: The decoupling
More informationIntroduction to AdS/CFT
Introduction to AdS/CFT Who? From? Where? When? Nina Miekley University of Würzburg Young Scientists Workshop 2017 July 17, 2017 (Figure by Stan Brodsky) Intuitive motivation What is meant by holography?
More informationM-Theory and Matrix Models
Department of Mathematical Sciences, University of Durham October 31, 2011 1 Why M-Theory? Whats new in M-Theory The M5-Brane 2 Superstrings Outline Why M-Theory? Whats new in M-Theory The M5-Brane There
More informationarxiv:hep-th/ v1 15 Aug 2000
hep-th/0008120 IPM/P2000/026 Gauged Noncommutative Wess-Zumino-Witten Models arxiv:hep-th/0008120v1 15 Aug 2000 Amir Masoud Ghezelbash,,1, Shahrokh Parvizi,2 Department of Physics, Az-zahra University,
More informationExercise 1 Classical Bosonic String
Exercise 1 Classical Bosonic String 1. The Relativistic Particle The action describing a free relativistic point particle of mass m moving in a D- dimensional Minkowski spacetime is described by ) 1 S
More informationEmergent space-time and gravity in the IIB matrix model
Emergent space-time and gravity in the IIB matrix model Harold Steinacker Department of physics Veli Losinj, may 2013 Geometry and physics without space-time continuum aim: (toy-?) model for quantum theory
More informationHalf BPS solutions in type IIB and M-theory
Half BPS solutions in type IIB and M-theory Based on work done in collaboration with Eric D Hoker, John Estes, Darya Krym (UCLA) and Paul Sorba (Annecy) E.D'Hoker, J.Estes and M.G., Exact half-bps type
More informationThéorie des cordes: quelques applications. Cours IV: 11 février 2011
Particules Élémentaires, Gravitation et Cosmologie Année 2010-11 Théorie des cordes: quelques applications Cours IV: 11 février 2011 Résumé des cours 2009-10: quatrième partie 11 février 2011 G. Veneziano,
More informationA Brief Introduction to AdS/CFT Correspondence
Department of Physics Universidad de los Andes Bogota, Colombia 2011 Outline of the Talk Outline of the Talk Introduction Outline of the Talk Introduction Motivation Outline of the Talk Introduction Motivation
More informationTopological DBI actions and nonlinear instantons
8 November 00 Physics Letters B 50 00) 70 7 www.elsevier.com/locate/npe Topological DBI actions and nonlinear instantons A. Imaanpur Department of Physics, School of Sciences, Tarbiat Modares University,
More informationQuantum Field Theory on NC Curved Spacetimes
Quantum Field Theory on NC Curved Spacetimes Alexander Schenkel (work in part with Thorsten Ohl) Institute for Theoretical Physics and Astrophysics, University of Wu rzburg Workshop on Noncommutative Field
More informationAdS/CFT Correspondence and Entanglement Entropy
AdS/CFT Correspondence and Entanglement Entropy Tadashi Takayanagi (Kyoto U.) Based on hep-th/0603001 [Phys.Rev.Lett.96(2006)181602] hep-th/0605073 [JHEP 0608(2006)045] with Shinsei Ryu (KITP) hep-th/0608213
More informationFourth Aegean Summer School: Black Holes Mytilene, Island of Lesvos September 18, 2007
Fourth Aegean Summer School: Black Holes Mytilene, Island of Lesvos September 18, 2007 Central extensions in flat spacetimes Duality & Thermodynamics of BH dyons New classical central extension in asymptotically
More informationIntroduction to String Theory ETH Zurich, HS11. 9 String Backgrounds
Introduction to String Theory ETH Zurich, HS11 Chapter 9 Prof. N. Beisert 9 String Backgrounds Have seen that string spectrum contains graviton. Graviton interacts according to laws of General Relativity.
More informationExchange statistics. Basic concepts. University of Oxford April, Jon Magne Leinaas Department of Physics University of Oslo
University of Oxford 12-15 April, 2016 Exchange statistics Basic concepts Jon Magne Leinaas Department of Physics University of Oslo Outline * configuration space with identifications * from permutations
More informationBlack hole thermodynamics under the microscope
DELTA 2013 January 11, 2013 Outline Introduction Main Ideas 1 : Understanding black hole (BH) thermodynamics as arising from an averaging of degrees of freedom via the renormalisation group. Go beyond
More informationBlack Hole Entropy in the presence of Chern-Simons terms
Black Hole Entropy in the presence of Chern-Simons terms Yuji Tachikawa School of Natural Sciences, Institute for Advanced Study Dec 25, 2006, Yukawa Inst. based on hep-th/0611141, to appear in Class.
More informationInstantons and Sphalerons in a Magnetic Field
Stony Brook University 06/27/2012 GB, G.Dunne & D. Kharzeev, arxiv:1112.0532, PRD 85 045026 GB, D. Kharzeev, arxiv:1202.2161, PRD 85 086012 Outline Motivation & some lattice results General facts on Dirac
More informationSpectral action, scale anomaly. and the Higgs-Dilaton potential
Spectral action, scale anomaly and the Higgs-Dilaton potential Fedele Lizzi Università di Napoli Federico II Work in collaboration with A.A. Andrianov (St. Petersburg) and M.A. Kurkov (Napoli) JHEP 1005:057,2010
More informationApplications of AdS/CFT correspondence to cold atom physics
Applications of AdS/CFT correspondence to cold atom physics Sergej Moroz in collaboration with Carlos Fuertes ITP, Heidelberg Outline Basics of AdS/CFT correspondence Schrödinger group and correlation
More informationGeometry and Physics. Amer Iqbal. March 4, 2010
March 4, 2010 Many uses of Mathematics in Physics The language of the physical world is mathematics. Quantitative understanding of the world around us requires the precise language of mathematics. Symmetries
More informationHolographic Entanglement Entropy
Motivation Time-dependent Multi-region Summary Holographic entanglement entropy for time dependent states and disconnected regions Durham University INT08: From Strings to Things, April 3, 2008 VH, M.
More informationDynamics of heavy quarks in charged N = 4 SYM plasma
Dynamics of heavy quarks in charged N = 4 SYM plasma Aleksi Vuorinen University of Washington, Seattle & Technical University of Vienna C. Herzog and AV, arxiv:0708:0609 [hep-th] Outline N = 4 SYM and
More informationAdS/CFT duality. Agnese Bissi. March 26, Fundamental Problems in Quantum Physics Erice. Mathematical Institute University of Oxford
AdS/CFT duality Agnese Bissi Mathematical Institute University of Oxford March 26, 2015 Fundamental Problems in Quantum Physics Erice What is it about? AdS=Anti de Sitter Maximally symmetric solution of
More informationAspects of integrability in classical and quantum field theories
Aspects of integrability in classical and quantum field theories Second year seminar Riccardo Conti Università degli Studi di Torino and INFN September 26, 2018 Plan of the talk PART 1 Supersymmetric 3D
More informationHolographic Entanglement and Interaction
Holographic Entanglement and Interaction Shigenori Seki RINS, Hanyang University and Institut des Hautes Études Scientifiques Intrication holographique et interaction à l IHES le 30 janvier 2014 1 Contents
More informationNon-Associative Quantum Mechanics from Non-Geometric Strings. Peter Schupp
Non-Associative Quantum Mechanics from Non-Geometric Strings Peter Schupp Jacobs University Bremen Workshop on Non-Associativity in Physics and Related Mathematical Structures, IGS, PennState May 1-3,
More informationLecture 9: RR-sector and D-branes
Lecture 9: RR-sector and D-branes José D. Edelstein University of Santiago de Compostela STRING THEORY Santiago de Compostela, March 6, 2013 José D. Edelstein (USC) Lecture 9: RR-sector and D-branes 6-mar-2013
More informationBianchi I Space-times and Loop Quantum Cosmology
Bianchi I Space-times and Loop Quantum Cosmology Edward Wilson-Ewing Institute for Gravitation and the Cosmos The Pennsylvania State University Work with Abhay Ashtekar October 23, 2008 E. Wilson-Ewing
More informationPath Integral for Spin
Path Integral for Spin Altland-Simons have a good discussion in 3.3 Applications of the Feynman Path Integral to the quantization of spin, which is defined by the commutation relations [Ŝj, Ŝk = iɛ jk
More informationAn extended standard model and its Higgs geometry from the matrix model
An extended standard model and its Higgs geometry from the matrix model Jochen Zahn Universität Wien based on arxiv:1401.2020 joint work with Harold Steinacker Bayrischzell, May 2014 Motivation The IKKT
More informationQuark-gluon plasma from AdS/CFT Correspondence
Quark-gluon plasma from AdS/CFT Correspondence Yi-Ming Zhong Graduate Seminar Department of physics and Astronomy SUNY Stony Brook November 1st, 2010 Yi-Ming Zhong (SUNY Stony Brook) QGP from AdS/CFT Correspondence
More information8.821 F2008 Lecture 05
8.821 F2008 Lecture 05 Lecturer: McGreevy Scribe: Evangelos Sfakianakis September 22, 2008 Today 1. Finish hindsight derivation 2. What holds up the throat? 3. Initial checks (counting of states) 4. next
More informationIntroduction to Modern Quantum Field Theory
Department of Mathematics University of Texas at Arlington Arlington, TX USA Febuary, 2016 Recall Einstein s famous equation, E 2 = (Mc 2 ) 2 + (c p) 2, where c is the speed of light, M is the classical
More informationHawking radiation and universal horizons
LPT Orsay, France June 23, 2015 Florent Michel and Renaud Parentani. Black hole radiation in the presence of a universal horizon. In: Phys. Rev. D 91 (12 2015), p. 124049 Hawking radiation in Lorentz-invariant
More informationPoS(LAT2005)324. D-branes and Topological Charge in QCD. H. B. Thacker University of Virginia
D-branes and Topological Charge in QCD University of Virginia E-mail: hbt8r@virginia.edu The recently observed long-range coherent structure of topological charge fluctuations in QCD is compared with theoretical
More informationarxiv: v1 [hep-th] 3 Feb 2016
Noname manuscript No. (will be inserted by the editor) Thermodynamics of Asymptotically Flat Black Holes in Lovelock Background N. Abbasvandi M. J. Soleimani Shahidan Radiman W.A.T. Wan Abdullah G. Gopir
More informationHolographic Space Time
Holographic Space Time Tom Banks (work with W.Fischler) April 1, 2015 The Key Points General Relativity as Hydrodynamics of the Area Law - Jacobson The Covariant Entropy/Holographic Principle - t Hooft,
More information8.821 String Theory Fall 2008
MIT OpenCourseWare http://ocw.mit.edu 8.821 String Theory Fall 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. 8.821 F2008 Lecture 04 Lecturer: McGreevy
More informationAn introduction to General Relativity and the positive mass theorem
An introduction to General Relativity and the positive mass theorem National Center for Theoretical Sciences, Mathematics Division March 2 nd, 2007 Wen-ling Huang Department of Mathematics University of
More informationWhy we need quantum gravity and why we don t have it
Why we need quantum gravity and why we don t have it Steve Carlip UC Davis Quantum Gravity: Physics and Philosophy IHES, Bures-sur-Yvette October 2017 The first appearance of quantum gravity Einstein 1916:
More informationGeneral Relativity in a Nutshell
General Relativity in a Nutshell (And Beyond) Federico Faldino Dipartimento di Matematica Università degli Studi di Genova 27/04/2016 1 Gravity and General Relativity 2 Quantum Mechanics, Quantum Field
More informationBMS current algebra and central extension
Recent Developments in General Relativity The Hebrew University of Jerusalem, -3 May 07 BMS current algebra and central extension Glenn Barnich Physique théorique et mathématique Université libre de Bruxelles
More informationWiggling Throat of Extremal Black Holes
Wiggling Throat of Extremal Black Holes Ali Seraj School of Physics Institute for Research in Fundamental Sciences (IPM), Tehran, Iran Recent Trends in String Theory and Related Topics May 2016, IPM based
More informationÜbungen zu RT2 SS (4) Show that (any) contraction of a (p, q) - tensor results in a (p 1, q 1) - tensor.
Übungen zu RT2 SS 2010 (1) Show that the tensor field g µν (x) = η µν is invariant under Poincaré transformations, i.e. x µ x µ = L µ νx ν + c µ, where L µ ν is a constant matrix subject to L µ ρl ν ση
More informationBoost-invariant dynamics near and far from equilibrium physics and AdS/CFT.
Boost-invariant dynamics near and far from equilibrium physics and AdS/CFT. Micha l P. Heller michal.heller@uj.edu.pl Department of Theory of Complex Systems Institute of Physics, Jagiellonian University
More informationEntanglement entropy in a holographic model of the Kondo effect
Entanglement entropy in a holographic model of the Kondo effect Mario Flory Max-Planck-Institut für Physik University of Oxford 05.05.2015 Mario Flory Entanglement entropy & Kondo 1 / 30 Overview Part
More informationDuality and Holography
Duality and Holography? Joseph Polchinski UC Davis, 5/16/11 Which of these interactions doesn t belong? a) Electromagnetism b) Weak nuclear c) Strong nuclear d) a) Electromagnetism b) Weak nuclear c) Strong
More informationBFT embedding of noncommutative D-brane system. Abstract
SOGANG-HEP 271/00 BFT embedding of noncommutative D-brane system Soon-Tae Hong,WonTaeKim, Young-Jai Park, and Myung Seok Yoon Department of Physics and Basic Science Research Institute, Sogang University,
More informationA Summary of the Black Hole Perturbation Theory. Steven Hochman
A Summary of the Black Hole Perturbation Theory Steven Hochman Introduction Many frameworks for doing perturbation theory The two most popular ones Direct examination of the Einstein equations -> Zerilli-Regge-Wheeler
More informationIntroduction to Chern-Simons forms in Physics - I
Introduction to Chern-Simons forms in Physics - I Modeling Graphene-Like Systems Dublin April - 2014 Jorge Zanelli Centro de Estudios Científicos CECs - Valdivia z@cecs.cl Lecture I: 1. Topological invariants
More informationQuantum Field Theory and Gravity on Non-Commutative Spaces
Projektbeschreibung Quantum Field Theory and Gravity on Non-Commutative Spaces Grant Application to the Austrian Academy of Sciences Vienna, Austria October 2004 10 1 Background Non-commutative spaces
More informationStrings, gauge theory and gravity. Storrs, Feb. 07
Strings, gauge theory and gravity Storrs, Feb. 07 Outline Motivation - why study quantum gravity? Intro to strings Gravity / gauge theory duality Gravity => gauge: Wilson lines, confinement Gauge => gravity:
More informationand the seeds of quantisation
noncommutative spectral geometry algebra doubling and the seeds of quantisation m.s.,.,, stabile, vitiello, PRD 84 (2011) 045026 mairi sakellariadou king s college london noncommutative spectral geometry
More informationThe Gauge/Gravity correspondence: linking General Relativity and Quantum Field theory
The Gauge/Gravity correspondence: linking General Relativity and Quantum Field theory Alfonso V. Ramallo Univ. Santiago IFIC, Valencia, April 11, 2014 Main result: a duality relating QFT and gravity Quantum
More informationQuantum mechanics and the geometry of spacetime
Quantum mechanics and the geometry of spacetime Juan Maldacena PPCM Conference May 2014 Outline Brief review of the gauge/gravity duality Role of strong coupling in the emergence of the interior Role of
More informationBlack Hole Entropy: An ADM Approach Steve Carlip U.C. Davis
Black Hole Entropy: An ADM Approach Steve Carlip U.C. Davis ADM-50 College Station, Texas November 2009 Black holes behave as thermodynamic objects T = κ 2πc S BH = A 4 G Quantum ( ) and gravitational
More informationTHE ROLE OF BLACK HOLES IN THE ADS/CFT CORRESPONDENCE
THE ROLE OF BLACK HOLES IN THE ADS/CFT CORRESPONDENCE Jakob Gath Submitted in partial fulfilment of the requirements for the degree of Master of Science of the Imperial College London Imperial College
More informationTOPIC V BLACK HOLES IN STRING THEORY
TOPIC V BLACK HOLES IN STRING THEORY Lecture notes Making black holes How should we make a black hole in string theory? A black hole forms when a large amount of mass is collected together. In classical
More informationTwistor Strings, Gauge Theory and Gravity. Abou Zeid, Hull and Mason hep-th/
Twistor Strings, Gauge Theory and Gravity Abou Zeid, Hull and Mason hep-th/0606272 Amplitudes for YM, Gravity have elegant twistor space structure: Twistor Geometry Amplitudes for YM, Gravity have elegant
More informationTHE BORDER BETWEEN RELATIVITY AND QUANTUM THEORY
THE BORDER BETWEEN RELATIVITY AND QUANTUM THEORY Tevian Dray I: Attempts at Unification II: Spinors III: The Future Abstract Many efforts have been made to fulfill Einstein s dream of unifying general
More informationHolographic Entanglement Entropy for Surface Operators and Defects
Holographic Entanglement Entropy for Surface Operators and Defects Michael Gutperle UCLA) UCSB, January 14th 016 Based on arxiv:1407.569, 1506.0005, 151.04953 with Simon Gentle and Chrysostomos Marasinou
More informationProblem Set 1 Classical Worldsheet Dynamics
MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Physics String Theory (8.821) Prof. J. McGreevy Fall 2007 Problem Set 1 Classical Worldsheet Dynamics Reading: GSW 2.1, Polchinski 1.2-1.4. Try 3.2-3.3.
More informationNewton s Second Law in a Noncommutative Space
Newton s Second Law in a Noncommutative Space Juan M. Romero, J.A. Santiago and J. David Vergara Instituto de Ciencias Nucleares, U.N.A.M., Apdo. Postal 70-543, México D.F., México sanpedro, santiago,
More informationV Finite T, probe branes, quarks, other extensions
Introduction to the AdS/CFT correspondence Outline I CFT review II AdS/CFT correspondence III Large N review IV D3 branes and AdS 5 S 5 V Finite T, probe branes, quarks, other extensions 1 0 References
More informationSpin foam vertex and loop gravity
Spin foam vertex and loop gravity J Engle, R Pereira and C Rovelli Centre de Physique Théorique CNRS Case 907, Université de la Méditerranée, F-13288 Marseille, EU Roberto Pereira, Loops 07 Morelia 25-30
More informationNoncommutative geometry, quantum symmetries and quantum gravity II
Noncommutative geometry, quantum symmetries and quantum gravity II 4-7 July 2016, Wroclaw, Poland XXXVII Max Born Symposium & 2016 WG3 Meeting of COST Action MP1405 Cartan s structure equations and Levi-Civita
More informationHolography Duality (8.821/8.871) Fall 2014 Assignment 2
Holography Duality (8.821/8.871) Fall 2014 Assignment 2 Sept. 27, 2014 Due Thursday, Oct. 9, 2014 Please remember to put your name at the top of your paper. Note: The four laws of black hole mechanics
More informationTopological reduction of supersymmetric gauge theories and S-duality
Topological reduction of supersymmetric gauge theories and S-duality Anton Kapustin California Institute of Technology Topological reduction of supersymmetric gauge theories and S-duality p. 1/2 Outline
More informationAsymptotic Safety in the ADM formalism of gravity
Asymptotic Safety in the ADM formalism of gravity Frank Saueressig Research Institute for Mathematics, Astrophysics and Particle Physics Radboud University Nijmegen J. Biemans, A. Platania and F. Saueressig,
More informationA kappa deformed Clifford Algebra, Hopf Algebras and Quantum Gravity
A kappa deformed Clifford Algebra, Hopf Algebras and Quantum Gravity Carlos Castro Perelman June 2015 Universidad Tecnica Particular de Loja, San Cayetano Alto, Loja, 1101608 Ecuador Center for Theoretical
More informationThe Structure of Spacetime & Noncommutative Geometry
The Structure of Spacetime & Noncommutative Geometry Pointers for a discussion Fedele Lizzi Paris 2008 Disclaimer: This is not a regular talk. Little of nothing of what I will describe has been contributed
More information