Hawking radiation in Reissner-Nordström blackhole with a global monopole via Covariant anomalies and Effective action

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dc.creatorGangopadhyay, Sunandan
dc.date2008-03-25
dc.date.accessioned2026-07-07T11:49:19Z
dc.date.available2026-07-07T11:49:19Z
dc.descriptionWe adopt the covariant anomaly cancellation method as well as the effective action approach to obtain the Hawking radiation from the Reissner-Nordström blackhole with a global monopole falling in the class of the most general spherically symmetric charged blackhole $(\sqrt{-g}\neq1)$, using only covariant boundary condition at the event horizon.
dc.description10 pages Latex
dc.identifierhttps://arxiv.org/abs/0803.3492
dc.identifierhttp://arxiv.org/abs/0803.3492
dc.identifierPhys.Rev.D78:044026,2008
dc.identifierdoi:10.1103/PhysRevD.78.044026
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/203195
dc.subjectHigh Energy Physics - Theory
dc.titleHawking radiation in Reissner-Nordström blackhole with a global monopole via Covariant anomalies and Effective action
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