Absorption cross section of RN black hole

dc.creatorR., Sini
dc.creatorKuriakose, V. C.
dc.date2007-08-23
dc.date.accessioned2026-07-07T12:54:56Z
dc.date.available2026-07-07T12:54:56Z
dc.descriptionThe behavior of a charged scalar field in the RN black hole space time is studied using WKB approximation. In the present work it is assumed that matter waves can get reflected from the event horizon. Using this effect, the Hawking temperature and the absorption cross section for RN black hole placed in a charged scalar field are calculated. The absorption cross section $σ_{abs}$ is found to be inversely proportional to square of the Hawking temperature of the black hole.
dc.description6 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/0708.3146
dc.identifierhttp://arxiv.org/abs/0708.3146
dc.identifierInt.J.Mod.Phys.D18:1-11,2009
dc.identifierdoi:10.1142/S0218271809014236
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/224112
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAbsorption cross section of RN black hole
dc.typetext

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