Global Structure of Evaporating Black Holes

Preprint

4 February 2000

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.gr-qc/9807031

Abstract

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.

Keywords

CONDITIONS IF BOUNDARY
EVAPORATING BLACK
GLOBAL STRUCTURE
CHARGED VAIDYA
SINGULARITY
EVAPORATION
BLACK HOLE
SPACETIME

All Related Versions

Version 1, 1998-07-14, ArXiv
Version 2, 2000-02-04, ArXiv
Published version: Physics Letters B, 449 (1-2), 24.

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