KKW Analysis for the Dyadosphere of a Charged Black Hole

Details KKW Analysis for the Dyadosphere of a Charged Black Hole KKW Analysis for the Dyadosphere of a Charged Black Hole

2005-11-28

arxiv.org/abs/gr-qc/0511142v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

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Scientific paper

The Keski-Vakkuri, Kraus and Wilczek (KKW) analysis is used to compute the temperature and entropy in the dyadosphere of a charged black hole solution. For our purpose we choose the dyadosphere region of the Reissner-Nordstrom black hole solution. Our results show that the expressions of the temperature and entropy in the dyadosphere of this charged black hole are not the Hawking temperature and the Bekenstein-Hawking entropy, respectively.

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