Non-Extreme Black Holes from Intersecting M-Branes

Details Non-Extreme Black Holes from Intersecting M-Branes Non-Extreme Black Holes from Intersecting M-Branes

1997-01-21

arxiv.org/abs/hep-th/9701095v3

Int.J.Mod.Phys.A13:1305-1328,1998

Physics

High Energy Physics

High Energy Physics - Theory

28 pages, Latex, misprints in published version corrected

Scientific paper

10.1142/S0217751X98000615

We 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-Nordstr{\o}m 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.

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