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We consider finite deformations of the p+2-dimensional Schwarzschild geometry which obey the vacuum Einstein equation, preserve the mean curvature and induced conformal metric on a sphere a distance $\lambda$ from the horizon and are regular on the future horizon.
1902
Earlier work this paper cites.
T. Damour, in: “Quelques propriétés mécaniques, électromagnétiques, thermodynamiques et quantiques des trous noirs”; Thèse de Doctorat d’Etat, Université Pierre et Marie Curie, Paris VI, 1979
1979
Earlier work this paper cites.
T. Damour, “Surface effects in Black Hole Physics,” in Proceedings of the second Marcel Grossmann Meeting on general Relativity
1982
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R. H. Price and K. S. Thorne, “Membrane Viewpoint on Black Holes: Properties and eEvolution of the Stretched Horizon,” Phys. Rev. D 33
1986
Cited alongside, same era.
G. Policastro, D. T. Son and A. O. Starinets, “The shear viscosity of strongly coupled N = 4 supersymmetric Yang-Mills plasma,” Phys. Rev. Lett. 87
2001
Cited alongside, same era.
Cited in the paper.
Cited in the paper.
V. Lysov, A. Strominger, “From Petrov-Einstein to Navier-Stokes,” [arXiv:1104.5502 [hep-th]]
Cited in the paper.
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