Shear viscosity of a highly excited string and the black hole membrane paradigm
arXiv:1010.5380 · doi:10.1103/PhysRevD.83.026002
Abstract
Black hole membrane paradigm states that a certain viscous membrane seems to be sitting on a stretched horizon of a black hole from the viewpoint of a distant observer. We show that the shear viscosity of the fictitious membrane can be reproduced by a highly excited string covering the stretched horizon except for a numerical coefficient.
arXiv comment22 pages, no figure, minor corrections
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Cited by in corpus (6)
- String in AdS Black Hole: A Thermo Field Dynamic Approach
- Hagedorn String Thermodynamics in Curved Spacetimes and near Black Hole Horizons
- Linear responses of D0-branes via gauge/gravity correspondence
- Closed string transport coefficients and the membrane paradigm
- Shear Viscosity to Entropy Density for a Black Brane in 5-dimensional Einstein-Yang-Mills Gravity
- Transport coefficients of D1-D5-P system and the membrane paradigm