Interaction of higher dimensional rotating black holes with branes
Mar, 200420 pages
Published in:
- Class.Quant.Grav. 21 (2004) 3483-3498
e-Print:
- gr-qc/0403054 [gr-qc]
Report number:
- ALBERTA-THY-05-04,
- MCTP-04-20
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Abstract: (arXiv)
We study interaction of rotating higher dimensional black holes with a brane in space-times with large extra dimensions. We demonstrate that in a general case a rotating black hole attached to a brane can loose 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 the gravitational radius reaches this final stationary state is , where is the higher dimensional gravitational coupling constant, is the brane tension, and is the number of extra dimensions.- 04.70.Bw
- 97.60.Lf
- 11.25.-w
- black hole: rotator
- higher-dimensional
- membrane model
- vector: Killing
- cosmic string
- domain wall
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