The Kerr black hole and rotating black string by intersecting M-branes

dc.creatorTanabe, Makoto
dc.date2008-04-24
dc.date.accessioned2026-07-07T09:34:56Z
dc.date.available2026-07-07T09:34:56Z
dc.descriptionWe construct the non-BPS black brane representation from the Kerr metric using the U-duality and symmetries in string or M-theory. We give the general rule to get the brane configuration and we apply it especially for Kerr metric. We find the three charged solution in M-theory and after the compactification it becomes rotating black string solution in five dimension. We also find the four charged solution containing the pp-wave in M-theory, and we can find charged dilaton rotating black hole solution in four dimension after the torus compactification. This solution has the other representation in string theory, which is easy to apply the AdS/CFT correspondence.
dc.description6 pages, no figures
dc.identifierhttps://arxiv.org/abs/0804.3831
dc.identifierhttp://arxiv.org/abs/0804.3831
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/159671
dc.subjectHigh Energy Physics - Theory
dc.titleThe Kerr black hole and rotating black string by intersecting M-branes
dc.typetext

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