Compactified black holes in five-dimensional U(1)**3 ungauged supergravity
Abstract
We present stationary, nonextremal three charge rotating black hole solutions in the five-dimensional U(1)^3 ungauged supergravity. At infinity, our solutions behave as a four-dimensional flat spacetime with a compact extra-dimension and hence describe spherical black holes with Kaluza-Klein asymptotics.
- Publication:
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arXiv e-prints
- Pub Date:
- September 2010
- DOI:
- 10.48550/arXiv.1009.3568
- arXiv:
- arXiv:1009.3568
- Bibcode:
- 2010arXiv1009.3568T
- Keywords:
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- High Energy Physics - Theory
- E-Print:
- 4 pages