Hawking radiation of charged particles as tunneling from Reissner-Nordstrom-de Sitter black holes with a global monopole

Preprint

5 June 2006

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.hep-th/0511123

Abstract

Applying Parikh's semi-classical tunneling method, we consider Hawking radiation of the charged massive particles as a tunneling process from the Reissner-Nordstrom-de Sitter black hole with a global monopole. The result shows that the tunneling rate is related to the change of Bekenstein-Hawking entropy and the radiant spectrum is not a pure thermal one, but is consistent with an underlying unitary theory.

Keywords

RADIATION OF CHARGED
REISSNER NORDSTROM
HAWKING RADIATION
CHARGED PARTICLES
SITTER BLACK
BLACK HOLE
TUNNELING

All Related Versions

Version 1, 2005-11-11, ArXiv
Version 2, 2005-11-14, ArXiv
Version 3, 2005-12-12, ArXiv
Version 4, 2006-02-16, ArXiv
Version 5, 2006-06-05, ArXiv

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