Hawking Radiation via Tunneling from Hot NUT-Kerr-Newman-Kasuya Spacetime

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dc.creatorAli, M. Hossain
dc.date2007-06-26
dc.date2007-10-28
dc.date.accessioned2026-07-07T10:56:27Z
dc.date.available2026-07-07T10:56:27Z
dc.descriptionWe study the Hawking thermal spectrum in dragging coordinate system and the tunneling radiation characteristics of hot NUT-Kerr-Newman-Kasuya spacetime. The tunneling rates at the event and cosmological horizon are found to be related to the change of Bekenstein-Hawking entropy. The radiation spectrum is not pure thermal and thus there is a correction to the Hawking thermal spectrum.
dc.descriptionTo appear in Class. Quant. Grav
dc.identifierhttps://arxiv.org/abs/0706.3890
dc.identifierhttp://arxiv.org/abs/0706.3890
dc.identifierClass.Quant.Grav.24:5849-5860,2007
dc.identifierdoi:10.1088/0264-9381/24/23/008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186418
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleHawking Radiation via Tunneling from Hot NUT-Kerr-Newman-Kasuya Spacetime
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