Abstract
We prove a theorem that characterizes a two-parameter family of solutions to Einstein equations with a negative cosmological constant, representing, in general, non-spherical radiating black holes in an anti-de Sitter background. It is shown that the best known non-spherical radiating black hole solutions are particular cases and static non-spherical black hole solutions, for Type I fluid, are also retrieved. A brief discussion on the energy conditions, singularities and horizons is provided.
Original language | English (US) |
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Pages (from-to) | 1115-1127 |
Number of pages | 13 |
Journal | Modern Physics Letters A |
Volume | 23 |
Issue number | 15 |
DOIs | |
State | Published - May 20 2008 |
All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics
- Astronomy and Astrophysics
- General Physics and Astronomy