THEOREM TO GENERATE NON-SPHERICAL RADIATING BLACK HOLE SOLUTIONS

DOI10.1142/S0217732308026613zbMath1179.83059OpenAlexW2082674537MaRDI QIDQ3597377

V. S. Morozova, Sushant G. Ghosh

Publication date: 9 February 2009

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0217732308026613

zbMATH Keywords

exact solutionsblack holesanti-de Sitternon-sphericaltype II fluidradiating

Mathematics Subject Classification ID

Black holes (83C57) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Space-time singularities, cosmic censorship, etc. (83C75) Exact solutions to problems in general relativity and gravitational theory (83C15)

Cites Work

• Generalized Vaidya solutions.
• The external field of a radiating star in general relativity
• Generating static black holes in higher dimensional space-times
• A torus-like black hole
• Null Fluid Collapse in the Plane Symmetric Anti-de Sitter Spacetime
• Topological censorship
• The cosmological term as a source of mass
• Pair production of topological anti-de Sitter black holes
• A simple theorem to generate exact black-hole solutions
• Black hole in three-dimensional spacetime
• Topological Censorship[Phys. Rev. Lett. 71, 1486 (1993)]
• Making anti-de Sitter black holes
• Quintessence and black holes
• Two-dimensional black holes and planar general relativity
• The Large Scale Structure of Space-Time

This page was built for publication: THEOREM TO GENERATE NON-SPHERICAL RADIATING BLACK HOLE SOLUTIONS