Published May 13, 2011 | Version v1
Journal article

Thermalization of Strongly Coupled Field Theories

  • 1. David Rittenhouse Laboratory, University of Pennsylvania, Philadelphia, Pennsylvania 19104 (United States)
  • 2. Theoretische Natuurkunde, Vrije Universiteit Brussel, and International Solvay Institutes, B-1050 Brussels (Belgium)
  • 3. Institute for Theoretical Physics, University of Amsterdam, 1090 GL Amsterdam (Netherlands)
  • 4. Helsinki Institute of Physics and Department of Physics, FIN-00014 University of Helsinki (Finland)
  • 5. Department of Physics and CTMS, Duke University, Durham, North Carolina 27708 (United States)
  • 6. Institut fuer Theoretische Physik, Universitaet Regensburg, D-93040 Regensburg (Germany)
  • 7. Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University, Nagoya 464-8602 (Japan)

Description

Using the holographic mapping to a gravity dual, we calculate 2-point functions, Wilson loops, and entanglement entropy in strongly coupled field theories in d=2, 3, and 4 to probe the scale dependence of thermalization following a sudden injection of energy. For homogeneous initial conditions, the entanglement entropy thermalizes slowest and sets a time scale for equilibration that saturates a causality bound. The growth rate of entanglement entropy density is nearly volume-independent for small volumes but slows for larger volumes. In this setting, the UV thermalizes first.

Additional details

Publishing Information

Journal Title
Physical Review Letters
Journal Volume
106
Journal Issue
19
Journal Page Range
p. 191601-191601.4
ISSN
0031-9007
CODEN
PRLTAO

INIS

Country of Publication
United States
Country of Input or Organization
Syrian Arab Republic
INIS RN
43017332
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Descriptors DEI
DENSITY; ENTROPY; FIELD THEORIES; GRAVITATION; QUANTUM ENTANGLEMENT; THERMALIZATION; WILSON LOOP
Descriptors DEC
PHYSICAL PROPERTIES; SLOWING-DOWN; THERMODYNAMIC PROPERTIES

Optional Information

Notes
(c) 2011 American Institute of Physics