KKW Analysis for the Dyadosphere of a Charged Black Hole

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dc.creatorRadinschi, I.
dc.date2005-11-28
dc.date.accessioned2026-07-07T06:49:45Z
dc.date.available2026-07-07T06:49:45Z
dc.descriptionThe 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.
dc.descriptionLaTex
dc.identifierhttps://arxiv.org/abs/gr-qc/0511142
dc.identifierhttp://arxiv.org/abs/gr-qc/0511142
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/104468
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleKKW Analysis for the Dyadosphere of a Charged Black Hole
dc.typetext

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