Small Black Holes in Randall-Sundrum type I Scenario

Details Small Black Holes in Randall-Sundrum type I Scenario Small Black Holes in Randall-Sundrum type I Scenario

2003-09-16

arxiv.org/abs/gr-qc/0309076v3

Phys.Rev. D69 (2004) 064022

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Version published at Phys. Rev. D69:064022 (2004)

Scientific paper

10.1103/PhysRevD.69.064022

An approximation method to study the properties of a small black hole located on the TeV brane in the Randall-Sundrum type I scenario is presented. The method enables us to find the form of the metric close to the matter distribution when its asymptotic form is given. The short range solution is found as an expansion in the ratio between the Schwarzschild radius of the black hole and the curvature length of the bulk. Long range properties are introduced using the linearized gravity solution as an asymptotic boundary condition. The solution is found up to first order. It is valid in the region close to the horizon but is not valid on the horizon. The regularity of the horizon is still under study.

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