The Entropy of the Complex Scalar Field in a Charged Kerr Black Hole

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dc.creatorLee, Min-Ho
dc.creatorKim, Jae Kwan
dc.date1996-04-22
dc.date.accessioned2026-07-07T04:22:03Z
dc.date.available2026-07-07T04:22:03Z
dc.descriptionBy using the brick wall method we calculate the thermodynamic potential of the complex scalar field in a charged Kerr black hole. Using it we show that in the Hartle-Hawking state the leading term of the entropy is proportional to $\frac{ A _H}{ε^2}$, which becomes divergent as the system approaches the black hole horizon. The origin of the divergence is that the density of states diverges at the horizon.
dc.descriptionLatex,10 pages
dc.identifierhttps://arxiv.org/abs/hep-th/9604130
dc.identifierhttp://arxiv.org/abs/hep-th/9604130
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/54564
dc.subjectHigh Energy Physics - Theory
dc.titleThe Entropy of the Complex Scalar Field in a Charged Kerr Black Hole
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