Hawking radiation in GHS and non-extremal D1-D5 blackhole via covariant anomalies

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dc.creatorGangopadhyay, Sunandan
dc.creatorKulkarni, Shailesh
dc.date2007-10-04
dc.date.accessioned2026-07-07T11:19:46Z
dc.date.available2026-07-07T11:19:46Z
dc.descriptionWe apply the method of Banerjee and Kulkarni (arXiv:0707.2449, [hep-th]) to provide a derivation of Hawking radiation from the GHS (stringy) blackhole which falls in the class of the most general spherically symmetric blackholes ($\sqrt{-g}\neq 1$) and also the non-extremal $D1-D5$ blackhole using only covariant gravitational anomalies.
dc.description8 pages latex file
dc.identifierhttps://arxiv.org/abs/0710.0974
dc.identifierhttp://arxiv.org/abs/0710.0974
dc.identifierPhys.Rev.D77:024038,2008
dc.identifierdoi:10.1103/PhysRevD.77.024038
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193799
dc.subjectHigh Energy Physics - Theory
dc.titleHawking radiation in GHS and non-extremal D1-D5 blackhole via covariant anomalies
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