Hristu Culetu

Ovidius University, Constanta, Romania

On the near horizon approximation for the Schwarzschild black hole

An anisotropic fluid with a negative radial pressure p = -ρ is supposed to exist near the horizon of a Schwarzschild black hole (BH). The constant energy density ρ depends only on the BH mass. The structure of the stress tensor is similar with that obtained previously for the interior region of a BH excepting the time dependence.