Valeri P Frolov et al 2004 Class. Quantum Grav. 21 3483 doi:10.1088/0264-9381/21/14/011
Valeri P Frolov1, Dmitri V Fursaev2 and Dejan Stojković3
Show affiliationsWe study interaction of rotating higher-dimensional black holes with a brane in spacetimes with large extra dimensions. We demonstrate that in a general case a rotating black hole attached to a brane can lose bulk components of its angular momenta. A stationary black hole can have only those components of the angular momenta which are connected with Killing vectors generating transformations preserving a position of the brane. In a final stationary state the null Killing vector generating the black hole horizon is tangent to the brane. We discuss first the interaction of a cosmic string and a domain wall with the 4D Kerr black hole. We then prove the general result for slowly rotating higher-dimensional black holes interacting with branes. The characteristic time when a rotating black hole with gravitational radius r0 reaches this final stationary state is T ~ rp−10/(Gσ), where G is the higher-dimensional gravitational coupling constant, σ is the brane tension and p is the number of extra dimensions.
04.70.Bw Classical black holes
11.27.+d Extended classical solutions; cosmic strings, domain walls, texture
Issue 14 (21 July 2004)
Received 13 March 2004
Published 23 June 2004
Valeri P Frolov et al 2004 Class. Quantum Grav. 21 3483
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