Journal
PHYSICS LETTERS B
Volume 635, Issue 2-3, Pages 151-155Publisher
ELSEVIER
DOI: 10.1016/j.physletb.2006.01.035
Keywords
charged particle; radiation; tunneling rate; Bekenstein-Hawking entropy; energy conservation and charge conservation
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Applying Parikh's semi-classical tunneling method, we consider Hawking radiation of the charged massive particles as a tunneling process from the Reissner-Nordstroin-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. (c) 2006 Published by Elsevier B.V.
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