On the near horizon approximation for the Schwarzschild black hole

Details On the near horizon approximation for the Schwarzschild black hole On the near horizon approximation for the Schwarzschild black hole

2009-03-20

arxiv.org/abs/0903.3548v3

Physics

High Energy Physics

High Energy Physics - Theory

5 pages, no figures, minor changes, reference added

Scientific paper

An anisotropic fluid with a negative radial pressure $p = - \rho$ is supposed to exist near the horizon of a Schwarzschild black hole. The constant energy density $\rho$ depends only on the black hole mass. The radial acceleration of the static observers is constant but its modulus has exactly the Rindler form, as was recently suggested by Dahia and Felix da Silva. The structure of the stress tensor is similar with that obtained previously for the interior region of a black hole, excepting the time dependence.

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