Hawking Radiation of Charged Particles as Tunneling from Higher Dimensional Reissner-Nordstrom-de Sitter Black Holes

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dc.creatorWu, Shuang-Qing
dc.creatorJiang, Qing-Quan
dc.date2006-03-10
dc.date2006-06-27
dc.date.accessioned2026-07-07T07:06:14Z
dc.date.available2026-07-07T07:06:14Z
dc.descriptionRecent work that treats the Hawking radiation as a semi-classical tunnelling process from the four-dimensional Schwarzschild and Reissner-Nordstrom black holes is extended to the case of higher dimensional Reissner-Nordstrom-de Sitter black holes. The result shows that the tunnelling rate is related to the change of Bekenstein-Hawking entropy and the exact radiant spectrum is no longer precisely thermal after considering the black hole background as dynamical and incorporating the self-gravitation effect of the emitted particles when the energy conservation and electric charge conservation are taken into account.
dc.description13 pages, no figure, enlarged version
dc.identifierhttps://arxiv.org/abs/hep-th/0603082
dc.identifierhttp://arxiv.org/abs/hep-th/0603082
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/109949
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHawking Radiation of Charged Particles as Tunneling from Higher Dimensional Reissner-Nordstrom-de Sitter Black Holes
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