Higher Curvature Gravity and the Holographic fluid dual to flat spacetime
arXiv:1105.4482 · doi:10.1007/JHEP08(2011)009
Abstract
Recent works have demonstrated that one can construct a (d+2) dimensional solution of the vacuum Einstein equations that is dual to a (d+1) dimensional fluid satisfying the incompressible Navier-Stokes equations. In one important example, the fluid lives on a fixed timelike surface in the flat Rindler spacetime associated with an accelerated observer. In this paper, we show that the shear viscosity to entropy density ratio of the fluid takes the universal value 1/4πin a wide class of higher curvature generalizations to Einstein gravity. Unlike the fluid dual to asymptotically anti-de Sitter spacetimes, here the choice of gravitational dynamics only affects the second order transport coefficients. We explicitly calculate these in five-dimensional Einstein-Gauss-Bonnet gravity and discuss the implications of our results.
arXiv comment13 pages; v2: modified abstract, added references; v3: added clarifying comments, modified discussion
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Cited by in corpus (22)
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- The relativistic fluid dual to vacuum Einstein gravity
- Towards a general fluid/gravity correspondence
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- Holographic Screens and Transport Coefficients in the Fluid/Gravity Correspondence
- Holographic charged fluid dual to third order Lovelock gravity
- Local Entropy Current in Higher Curvature Gravity and Rindler Hydrodynamics
- Clausius entropy for arbitrary bifurcate null surfaces
- Petrov type I Condition and Dual Fluid Dynamics
- Gravity-mediated holography in fluid dynamics
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