Hawking radiation of charged particles as tunneling from Reissner-Nordstrom-de Sitter black holes with a global monopole
arXiv:hep-th/0511123 · doi:10.1016/j.physletb.2006.01.035 10.1016/j.physletb.2006.06.009
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.
10 pages, no figure, use elsart.cls. Published version in PLB with corrections
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