The Incompressible Rindler fluid versus the Schwarzschild-AdS fluid
arXiv:1206.6924 · doi:10.1093/ptep/pts069
Abstract
We study the proposal by Bredberg et al. (1006.1902), where the fluid is defined by the Brown-York tensor on a timelike surface at r=r_c in black hole backgrounds. We consider both Rindler space and the Schwarzschild-AdS (SAdS) black hole. The former describes an incompressible fluid, whereas the latter describes the vanishing bulk viscosity at arbitrary r_c, but these two results do not contradict with each other. We also find an interesting "coincidence" with the black hole membrane paradigm which gives a negative bulk viscosity. In order to show these results, we rewrite the hydrodynamic stress tensor via metric perturbations using the conservation equation. The resulting expressions are suitable to compare with the Brown-York tensor.
18 pages, PTEPHY; v2: added discussion
References in corpus (1)
Cited by in corpus (6)
- Towards a general fluid/gravity correspondence
- Holographic charged fluid dual to third order Lovelock gravity
- Petrov type I Spacetime and Dual Relativistic Fluids
- Petrov type I Condition and Rindler Fluid in Vacuum Einstein-Gauss-Bonnet Gravity
- Linear responses of D0-branes via gauge/gravity correspondence
- Compressible Fluids in the Membrane Paradigm: non-AdS Fluid/Gravity correspondences