A Model for Evaporating Black Holes

Details A Model for Evaporating Black Holes A Model for Evaporating Black Holes

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pthph..71..100k&link_type=abstract

Progress of Theoretical Physics, Vol. 71, No. 1, pp. 100-108

Physics

14

Scientific paper

We consider Vaidya's classical spacetime which represents a mass decreasing black hole by means of an inward energy flow. To consider the particle creation in such a spacetime, we try to know the change of the particle creation rate of the black hole without considering back-reaction problem. We construct a model which varies its mass like v(-1) (v the usual advanced null time) to find that the particle creation in this spacetime is divergent at the final stage. This result means that a real evaporating black hole is not represented by this model, and therefore suggests that the appearance of a zero mass naked singularity cannot be avoided.

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