The Shah-Vaidya charged cosmological black hole metric is shown to be an exact solution of Einstein-Maxwell equations with a cuscuton field, and its causal structure is classified into four parameter regions with different horizon counts and naked singularities.
(36) and (39)] for which the a(t)r→ 0 limit corresponds toR→∞ , whileR = 0 cor- responds to a(t)r = (−m±|q|)/2, where the isotropic coordinater is allowed to assume negative values
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
gr-qc 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Charged cosmological black holes: a thorough study of a family of solutions
The Shah-Vaidya charged cosmological black hole metric is shown to be an exact solution of Einstein-Maxwell equations with a cuscuton field, and its causal structure is classified into four parameter regions with different horizon counts and naked singularities.