Noncommutative Schwarzschild Black Hole and Area Law

dc.creatorBanerjee, Rabin
dc.creatorMajhi, Bibhas Ranjan
dc.creatorModak, Sujoy Kumar
dc.date2008-02-15
dc.date2009-03-10
dc.date.accessioned2026-07-07T13:06:33Z
dc.date.available2026-07-07T13:06:33Z
dc.descriptionUsing a graphical analysis, we show that for the horizon radius $r_h\gtrsim 4.8\sqrtθ$, the standard semiclassical Bekenstein-Hawking area law for noncommutative Schwarzschild black hole exactly holds for all orders of $θ$. We also give the corrections to the area law to get the exact nature of the Bekenstein-Hawking entropy when $r_h<4.8\sqrtθ$ till the extremal point $r_h=3.0\sqrtθ$.
dc.description11 pages, 8 figures, refs. added, minor modifications, to appear in Class. Quant. Grav
dc.identifierhttps://arxiv.org/abs/0802.2176
dc.identifierhttp://arxiv.org/abs/0802.2176
dc.identifierClass.Quant.Grav.26:085010,2009
dc.identifierdoi:10.1088/0264-9381/26/8/085010
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/227814
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNoncommutative Schwarzschild Black Hole and Area Law
dc.typetext

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