Non-Extreme Black Holes from Intersecting M-Branes

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dc.creatorOhta, Nobuyoshi
dc.creatorShimizu, Takashi
dc.date1997-01-21
dc.date1999-01-29
dc.date.accessioned2026-07-07T12:19:49Z
dc.date.available2026-07-07T12:19:49Z
dc.descriptionWe investigate the possibility of extending non-extreme black hole solutions made of intersecting M-branes to those with two non-extreme deformation parameters, similar to Reissner-Nordstrøm solutions. General analysis of possible solutions is carried out to reduce the problem of solving field equations to a simple algebraic one for static spherically-symmetric case in $D$ dimensions. The results are used to show that the extension to two-parameter solutions is possible for $D=4,5$ dimensions but not for higher dimensions, and that the area of horizon always vanishes in the extreme limit for black hole solutions for $D \geq 6$ except for two very special cases which are identified. Various solutions are also summarized.
dc.description28 pages, Latex, misprints in published version corrected
dc.identifierhttps://arxiv.org/abs/hep-th/9701095
dc.identifierhttp://arxiv.org/abs/hep-th/9701095
dc.identifierInt.J.Mod.Phys.A13:1305-1328,1998
dc.identifierdoi:10.1142/S0217751X98000615
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/212888
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNon-Extreme Black Holes from Intersecting M-Branes
dc.typetext

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