Hawking radiation as tunneling for spherically symmetric black holes: A generalized treatment

Simple item page
dc.creatorSarkar, Sudipta
dc.creatorKothawala, Dawood
dc.date2007-09-27
dc.date.accessioned2026-07-07T11:19:37Z
dc.date.available2026-07-07T11:19:37Z
dc.descriptionWe present a derivation of Hawking radiation through tunneling mechanism for a general class of asymptotically flat, spherically symmetric spacetimes. The tunneling rate $Γ\sim \exp{(ΔS)}$ arises as a consequence of the first law of thermodynamics, TdS=dE + PdV. Therefore, this approach demonstrates how tunneling is intimately connected with the first law of thermodynamics through the principle of conservation of energy. The analysis is also generally applicable to any reasonable theory of gravity so long as the first law of thermodynamics for horizons holds in the form, TdS=dE + PdV.
dc.descriptionRevTeX 4; 11 pages; no figures
dc.identifierhttps://arxiv.org/abs/0709.4448
dc.identifierhttp://arxiv.org/abs/0709.4448
dc.identifierPhys.Lett.B659:683-687,2008
dc.identifierdoi:10.1016/j.physletb.2007.11.056
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193745
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleHawking radiation as tunneling for spherically symmetric black holes: A generalized treatment
dc.typetext

Files

Collections

arXiv