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Hence, considering that the isotropic coordinate is real, the domain of the areal radius coordi- nateR should be restricted to the intervalsR+≤R< ∞ and 0≤R≤R−

Undercharged case: m2 >q 2 In this case, the lapse function N(R) has two roots R± =m± √ m2−q2, andN 2(R) is negative in the intervalR− <R<R +

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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 2

    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.