THEOREM TO GENERATE NON-SPHERICAL RADIATING BLACK HOLE SOLUTIONS
Viktoriya MorozovaInter-University Center for Astronomy and Astrophysics, Post Bag 4 Ganeshkhind, Pune 411007, IndiaSushant G. GhoshBITS, Pilani Dubai, P.B. 500022, Dubai International Academic City, Dubai, UAE
ABI
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.
Topics
Identifiers
Citations and references
Cited by 032 references
Metrics — AkademScholar · Coming soon