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arxiv: gr-qc/9807031 · v2 · submitted 1998-07-14 · 🌀 gr-qc · hep-th

Global Structure of Evaporating Black Holes

Maulik K. Parikh , Frank Wilczek This is my paper
classification 🌀 gr-qc hep-th
keywords blackchargedconditionssingularityspacetimeboundaryconstructioncover
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By extending the charged Vaidya metric to cover all of spacetime, we obtain a Penrose diagram for the formation and evaporation of a charged black hole. In this construction, the singularity is time-like. The entire spacetime can be predicted from initial conditions if boundary conditions at the singularity are known.

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  1. Regular Vaidya solutions of effective gravitational theories

    gr-qc 2025-06 unverdicted novelty 7.0

    Regular Vaidya solutions exist in effective gravitational theories that dynamically describe radiation-driven formation of regular black holes or mimickers without curvature singularities.