Evaporation of a black hole off of a tense brane

De-Chang Dai, Nemanja Kaloper, Glenn D. Starkman, and Dejan Stojković
Phys. Rev. D 75, 024043 – Published 31 January 2007

Abstract

We calculate the greybody factors for scalar, vector and graviton fields in the background of an exact black hole localized on a tensional 3-brane in a world with two large extra dimensions. Finite brane tension modifies the standard results for the case with of a black hole on a brane with negligible tension. For a black hole of a fixed mass, the power carried away into the bulk diminishes as the tension increases, because the effective Planck constant, and therefore entropy of a fixed mass black hole, increase. In this limit, the semiclassical description of black hole decay becomes more reliable.

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  • Received 16 November 2006

DOI:https://doi.org/10.1103/PhysRevD.75.024043

©2007 American Physical Society

Authors & Affiliations

De-Chang Dai1, Nemanja Kaloper2, Glenn D. Starkman1,3, and Dejan Stojković1

  • 1Department of Physics, Case Western Reserve University, Cleveland, Ohio 44106, USA
  • 2Department of Physics, University of California, Davis California 95616, USA
  • 3Astrophysics Department, University of Oxford, Oxford, OX1 3RH, United Kingdom

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Issue

Vol. 75, Iss. 2 — 15 January 2007

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