Viscosity bound violation in higher derivative gravity
Creators
- 1. Department of Physics, Stanford University, Stanford, CA 94305 (United States)
- 2. Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5 (Canada) and Department of Physics and Astronomy, University of Waterloo, Waterloo, Ontario N2L 3G1 (Canada)
- 3. Center for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, MA 02139 (United States)
Description
Motivated by the vast string landscape, we consider the shear viscosity to entropy density ratio in conformal field theories dual to Einstein gravity with curvature square corrections. After field redefinitions these theories reduce to Gauss-Bonnet gravity, which has special properties that allow us to compute the shear viscosity nonperturbatively in the Gauss-Bonnet coupling. By tuning of the coupling, the value of the shear viscosity to entropy density ratio can be adjusted to any positive value from infinity down to zero, thus violating the conjectured viscosity bound. At linear order in the coupling, we also check consistency of four different methods to calculate the shear viscosity, and we find that all of them agree. We search for possible pathologies associated with this class of theories violating the viscosity bound
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.77.126006;
- arXiv
- arXiv:0712.0805v3;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 77
- Journal Issue
- 12
- Journal Page Range
- p. 126006-126006.17
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 40075758
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- CONFORMAL INVARIANCE; CORRECTIONS; COUPLING; DENSITY; ENTROPY; GRAVITATION; QUANTUM FIELD THEORY; RELATIVISTIC RANGE; VISCOSITY
- Descriptors DEC
- ENERGY RANGE; FIELD THEORIES; INVARIANCE PRINCIPLES; PHYSICAL PROPERTIES; THERMODYNAMIC PROPERTIES
Optional Information
- Notes
- (c) 2008 The American Physical Society