Radiating black hole solutions in arbitrary dimensions

2007/09/08 by S. G. Ghosh, A. K. Dawood · 3 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Quantum Electrodynamics and Casimir Effect #gr-qc

paper · pdf · doi:10.1007/s10714-007-0511-6

published as Gen.Rel.Grav.40:9-21,2008 · RevTeX 9 pages, no figures

openalex publication_date 2007/09/08 · arxiv created 2008/01/28 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

We prove a theorem that characterizes a large family of non-static solutions to Einstein equations in N-dimensional space-time, representing, in general, spherically symmetric Type II fluid. It is shown that the best known Vaidya-based (radiating) black hole solutions to Einstein equations, in both four dimensions (4D) and higher dimensions (HD), are particular cases from this family. The spherically symmetric static black hole solutions for Type I fluid can also be retrieved. A brief discussion on the energy conditions, singularities and horizons is provided.

Citations

• LETTER: Generalized Vaidya Solutions
• Quintessence and black holes

Cited by

• Three types of superpotentials for perturbations in the Einstein–Gauss–Bonnet gravity
• NONSTATIC CHARGED BTZ-LIKE BLACK HOLES IN N+1 DIMENSIONS
• Thermodynamic structure of field equations near apparent horizon for radiating black holes

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