Energy distribution in the dyadosphere of a charged black hole

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dc.creatorXulu, S. S.
dc.date2003-04-22
dc.date.accessioned2026-07-07T03:27:47Z
dc.date.available2026-07-07T03:27:47Z
dc.descriptionThe event horizon of a charged black hole is, according to Ruffini\cite{Ruffini} and Preparata \emph{et al.}\cite{PreparataEtAl}, surrounded by a special region called the \emph{dyadosphere} where the electromagnetic field exceeds the Euler-Heisenberg critical value for electron-positron pair production. We obtain the energy distribution in the dyadosphere region for a Reissner-Nordström black hole. We find that the energy-momentum prescriptions of Einstein, Landau-Lifshitz, Papapetrou, and Weinberg give the same and acceptable energy distribution.
dc.description10 pages, no figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0304081
dc.identifierhttp://arxiv.org/abs/gr-qc/0304081
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34569
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleEnergy distribution in the dyadosphere of a charged black hole
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