Anomalies, Horizons and Hawking radiation

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dc.creatorGangopadhyay, Sunandan
dc.date2008-09-26
dc.date2008-12-18
dc.date.accessioned2026-07-07T12:54:07Z
dc.date.available2026-07-07T12:54:07Z
dc.descriptionHawking radiation is obtained from the Reissner-Nordström blackhole with a global monopole and the Garfinkle-Horowitz-Strominger blackhole falling in the class of the most general spherically symmetric blackholes $(\sqrt{-g}\neq1)$, using only chiral anomaly near the event horizon and covariant boundary condition at the event horizon. The approach differs from the anomaly cancellation approach since apart from the covariant boundary condition, the chiral anomaly near the horizon is the only input to derive the Hawking flux.
dc.descriptionminor corrections made, To appear in Euro. Phys. Letters
dc.identifierhttps://arxiv.org/abs/0809.4572
dc.identifierhttp://arxiv.org/abs/0809.4572
dc.identifierEurophys.Lett.85:10004,2009
dc.identifierdoi:10.1209/0295-5075/85/10004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/223820
dc.subjectHigh Energy Physics - Theory
dc.titleAnomalies, Horizons and Hawking radiation
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