ICHEP conference, Paris, 22/07/10. Emergence Current Paradigm FUNDAMENTAL FORCES: carried by elementary particles.

Slides:



Advertisements
Similar presentations
Gerard t Hooft Spinoza Institute, Utrecht University Utrecht University and.
Advertisements

F. Debbasch (LERMA-ERGA Université Paris 6) and M. Bustamante, C. Chevalier, Y. Ollivier Statistical Physics and relativistic gravity ( )
Statistical mechanics
Martín Schvellinger Instituto de Física de La Plata - CONICET Departamento de Física - UNLP The gauge/gravity duality and Non-Relativistic Quantum Field.
Prof. dr. A. Achterberg, Astronomical Dept., IMAPP, Radboud Universiteit.
Wald’s Entropy, Area & Entanglement Introduction: –Wald’s Entropy –Entanglement entropy in space-time Wald’s entropy is (sometimes) an area ( of some metric)
8/1(Thu), 2013 Parallel talk (Theoretical development) Daisuke Kadoh (KEK) D.K. and Syo Kamata, in preparation TexPoint fonts used in.
 Entanglement & area thermodynamics of Rindler space  Entanglement & area  Entanglement & dimensional reduction (holography) Entanglement, thermodynamics.
Emergent Spacetime XXIII rd Solvay Conference in Physics December, 2005 Nathan Seiberg.
{Based on PRD 81 (2010) [ ], joint work with X.-N. Wu}
Gerard ’t Hooft Dublin November 13, 2007 Utrecht University on.
Entropic Gravity SISSA, Statistical Physics JC Friday 28, 2011 E. Verlinde, arXiv: v2 [hep-th]
Energy. Simple System Statistical mechanics applies to large sets of particles. Assume a system with a countable set of states.  Probability p n  Energy.
Gerard ’t Hooft Spinoza Institute Utrecht University CMI, Chennai, 20 November 2009 arXiv:
Entanglement in Quantum Critical Phenomena, Holography and Gravity Dmitri V. Fursaev Joint Institute for Nuclear Research Dubna, RUSSIA Banff, July 31,
Holographic Dark Energy Preety Sidhu 5 May Black Holes and Entropy Black holes are “maximal entropy objects” Entropy of a black hole proportional.
Quantum Entanglement and Gravity Dmitri V. Fursaev Joint Institute for Nuclear Research and Dubna University “Gravity in three dimensions”, ESI Workshop,
AdS4/CFT3+gravity for Accelerating Conical Singularities arXiv: arXiv: Mohamed Anber HET Bag Lunch Novemberr 12th.
HOLOGRAPHIC SPACE TIME AND SUPERSYMMETRY MBG-60 Conference Cambridge, UK April 2006.
Remarkable power of Einstein’s equation Gary Horowitz UC Santa Barbara Gary Horowitz UC Santa Barbara.
Strings and Black Holes David Lowe Brown University AAPT/APS Joint Fall Meeting.
Classical ConceptsEquations Newton’s Law Kinetic Energy Momentum Momentum and Energy Speed of light Velocity of a wave Angular Frequency Einstein’s Mass-Energy.
CERN Colloquium, 28/04/11. Matter and Forces Current Paradigm FUNDAMENTAL FORCES: carried by elementary particles.
A CRITICAL POINT IN A ADS/QCD MODEL Wu, Shang-Yu (NCTU) in collaboration with He, Song, Yang, Yi and Yuan, Pei-Hung , to appear in JHEP
The Quantum Space-Time Juan Maldacena Institute for Advanced Study 25 th Solvay Conference October 2011.
MSEG 803 Equilibria in Material Systems 6: Phase space and microstates Prof. Juejun (JJ) Hu
Quantum Gravity and Quantum Entanglement (lecture 2) Dmitri V. Fursaev Joint Institute for Nuclear Research Dubna, RUSSIA Talk is based on hep-th/
Entropy bounds Introduction Black hole entropy Entropy bounds Holography.
Entropy localization and distribution in the Hawking radiation Horacio Casini CONICET-Intituto Balseiro – Centro Atómico Bariloche.
An introduction to the Gravity/Fluid correspondence and its applications Ya-Peng Hu College of Science, Nanjing University of Aeronautics and Astronautics,
Louisville March 22, 2006 Andrew Chamblin Memorial An AdS Thermal Properties of Strongly Coupled Gauge Theories with Fundamental Matter from Gauge/Gravity.
Einstein Field Equations and First Law of Thermodynamics Rong-Gen Cai (蔡荣根) Institute of Theoretical Physics Chinese Academy of Sciences.
Shear viscosity of a highly excited string and black hole membrane paradigm Yuya Sasai Helsinki Institute of Physics and Department of Physics University.
Emanuele Berti Aristotle University of Thessaloniki In collaboration with: Kostas Kokkotas, Vitor Cardoso, Hisashi Onozawa Suggested.
On Fuzzball conjecture Seiji Terashima (YITP, Kyoto) based on the work (PRD (2008), arXiv: ) in collaboration with Noriaki Ogawa (YITP)
Black holes sourced by a massless scalar KSM2105, FRANKFURT July, 21th 2015 M. Cadoni, University of Cagliari We construct asymptotically flat black hole.
II Russian-Spanish Congress “Particle and Nuclear Physics at all scales and Cosmology”, Saint Petersburg, Oct. 4, 2013 RECENT ADVANCES IN THE BOTTOM-UP.
Ludwid Boltzmann 1844 – 1906 Contributions to Kinetic theory of gases Electromagnetism Thermodynamics Work in kinetic theory led to the branch of.
Holographic QCD in the medium
Entanglement in Quantum Gravity and Space-Time Topology
Holography, de Sitter space and SUSY breaking Lindefest, Stanford, Mar 7, 2008.
Based on Phys. Rev. D 92, (R) (2015) 中科大交叉学科理论研究中心
Jae-Weon Lee (Jungwon univ.) Collaboration with JJLEE & HCKIM.
Gravity field equations can be derived from the thermodynamic relation for any metric theory of gravity Merav Hadad Ram Brustein, M.H
Gauge/gravity duality in Einstein-dilaton theory Chanyong Park Workshop on String theory and cosmology (Pusan, ) Ref. S. Kulkarni,
Macroscopic Quantum Geometry Craig Hogan University of Chicago and Fermilab.
DPG Conference, Hamburg
Gravity on Matter Equation of State and the Unruh temperature Hyeong-Chan Kim (KNUT) 2016 FRP workshop on String theory and cosmology Seoul, Korea, June.
“Applied” String Theory Pinaki Banerjee The Institute of Mathematical Sciences, Chennai Department of Physics, Visva Bharati 12 th July, 2013.
Causality Problem in Holographic Dark Energy Hyeong-Chan Kim Korea National University of Transportation, with Jungjai Lee (Daejin U.) and Jae-Weon Lee.
Dept.of Physics & Astrophysics
Quantum Mechanical Models for Near Extremal Black Holes
Equation of State and Unruh temperature
Extreme measures for extremal black holes
Institut d’Astrophysique de Paris
Joe Kapusta* University of Minnesota
Quantum mechanics, entropic gravity, &
Thermodynamic Volume in AdS/CFT
Gravity from quantum entanglement Jae-Weon Lee (Jungwon univ.)
3D (Higher Spin) Gravity Black Holes and Statistical Entropy
Solutions of black hole interior, information paradox and the shape of singularities Haolin Lu.
GENERAL RELATIVITY General relativity describes the effect of gravitational fields on space and time.
Quantum mechanics from classical statistics
Based on the work submitted to EPJC
GENERAL RELATIVITY General relativity describes the effect of gravitational fields on space and time.
The Cosmological Constant Problem & Self-tuning Mechanism
Gravity from Entanglement and RG Flow
Entropic Gravity Miao Li 中国科学院理论物理研究所
Thermodynamics of Kerr-AdS Black Holes
Presentation transcript:

ICHEP conference, Paris, 22/07/10

Emergence

Current Paradigm FUNDAMENTAL FORCES: carried by elementary particles

Emergence of Particles and Forces

Gravity as an Emergent Force  At a microscopic scale Nature is described by many degrees of freedom, most of which are invisible and at first sight irrelevant for the observed macroscopic physics.  Gravity arises due to the fact that the amount of phase space volume (“information”) occupied by these microscopic degrees of freedom is influenced by the observable macroscopic variables, like the positions of material objects.

 Black hole thought experiments. Consider a particle gradually lowered in to a black hole. Classically, the energy associated with the particle gets redshifted, and vanishes when the particle is at the horizon. Penrose Christodoulou Bekenstein Hawking

Black Hole Entropy => Holographic Principle Maximal information associated with a part of space can be encoded in a # of bits equal to the area in Planck units

ADS/CFT CORRESPONDENCE EQUIVALENCE BETWEEN FIELD THEORY ON THE “BOUNDARY” AND GRAVITY IN THE “BULK” ONE SPACE DIMENSION EMERGES CORRESPONDING TO THE “SCALE” OF THE BOUNDARY THEORY. RADIAL EVOLUTION IS LIKE RENORMALIZATION GROUP FLOW.

Entropic force (wikipedia) An entropic force is a macroscopic force whose properties are determined not by the character of an underlying microscopic force, but by the whole system's statistical tendency to increase its entropy.

 Thought experiment “stretched horizon” black hole

 Consistency with black hole thermodynamics implies

information is stored on holographic screens moving a particle over one Compton wavelength leads to one more bit of information A HEURISTIC DERIVATION OF GRAVITY

To get a force one needs a temperature. By taking that temperature to be the Unruh temperature one finds Newton’s law of inertia

In order to get an entropic force I need a temperature

Holographic screens at equipotential (= equal redshift) surfaces

What about General Relativity? Surface of constant redshift Komar mass => Einstein equation

Rindler Horizon Suggestive link with QM: What is this velocity v ?

Cosmological Horizon De Sitter Space

Cosmological Horizon

Cosmological Horizon

Equipotential surface v = escape velocity

Schroedinger eqn with H depending on infinitely slow variable Instantaneous eigenstates Adiabatic Reaction Force Semiclassically

What lives on the screens? According to string theory: open strings. Integrating out the UV open strings produces closed strings in the emerged space.

Open closed string duality x Open string one loop diagram Massless pole in dual channel

UV/IR correspondence Open string with UV cut off Closed string / gravity with UV cut off

Matrix description of gravity.

Gravity as an Emergent Force  At a microscopic scale Nature is described by many degrees of freedom, most of which are invisible and at first sight irrelevant for the observed macroscopic physics.  Gravity arises due to the fact that the amount of phase space volume (“information”) occupied by these microscopic degrees of freedom is influenced by the observable macroscopic variables, like the positions of material objects.

Dirac monopool At the locus of coinciding eigenvalues one can construct Non-abelian Berry