Hawking radiation in a $d$-dimensional static spherically-symmetric black Hole surrounded by quintessence

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dc.creatorChen, Songbai
dc.creatorWang, Bin
dc.creatorSu, Rukeng
dc.date2008-01-14
dc.date2008-04-20
dc.date.accessioned2026-07-07T11:39:52Z
dc.date.available2026-07-07T11:39:52Z
dc.descriptionWe present a solution of Einstein equations with quintessential matter surrounding a $d$-dimensional black hole, whose asymptotic structures are determined by the state of the quintessential matter. We examine the thermodynamics of this black hole and find that the mass of the black hole depends on the equation of state of the quintessence, while the first law is universal. Investigating the Hawking radiation in this black hole background, we observe that the Hawking radiation dominates on the brane in the low-energy regime. For different asymptotic structures caused by the equation of state of the quintessential matter surrounding the black hole, we learn that the influences by the state parameter of the quintessence on Hawking radiation are different.
dc.description16 pages, Accepted for publication in Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/0801.2053
dc.identifierhttp://arxiv.org/abs/0801.2053
dc.identifierPhys.Rev.D77:124011,2008
dc.identifierdoi:10.1103/PhysRevD.77.124011
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200076
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHawking radiation in a $d$-dimensional static spherically-symmetric black Hole surrounded by quintessence
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