Hawking Fluxes, Back reaction and Covariant Anomalies

dc.creatorKulkarni, Shailesh
dc.date2008-02-18
dc.date2008-09-16
dc.date.accessioned2026-07-07T11:56:07Z
dc.date.available2026-07-07T11:56:07Z
dc.descriptionStarting from the chiral covariant effective action approach of Banerjee and Kulkarni [Phys. Lett. B 659, 827(2008)], we provide a derivation of the Hawking radiation from a charged black hole in the presence of gravitational back reaction. The modified expressions for charge and energy flux, due to effect of one loop back reaction are obtained.
dc.description6 pages, no figures, minor changes and references added, to appear in Classical and Quantum Gravity
dc.identifierhttps://arxiv.org/abs/0802.2456
dc.identifierhttp://arxiv.org/abs/0802.2456
dc.identifierClass.Quant.Grav.25:225023,2008
dc.identifierdoi:10.1088/0264-9381/25/22/225023
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/205477
dc.subjectHigh Energy Physics - Theory
dc.titleHawking Fluxes, Back reaction and Covariant Anomalies
dc.typetext

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