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We then conclude that, form2 =q2, theisotropiccoordinate r covers(once) all the range ofR

Extremal case: m2 =q2 In this case, N(R) has a double root R+ = R− = m =|q|, andN 2(R) is non-negative in the whole domain 0≤R< ∞, where it is assumed, as usual, that the areal rad

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Charged cosmological black holes: a thorough study of a family of solutions

gr-qc · 2019-08-14 · conditional · novelty 6.0

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.

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  • Charged cosmological black holes: a thorough study of a family of solutions gr-qc · 2019-08-14 · conditional · none · ref 3

    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.