Vaidya Spacetime as an Evaporating Black Hole

Physics

Scientific paper

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Scientific paper

The energy-momentum tensor of a scalar field for an evaporating black
hole modeled by the two-dimensional Vaidya metric is examined. It is
shown that the energy flux from a naked singularity, formed when a black
hole disappears, can be divergent even when the mass M disappears with
the condition dM/dv -> 0(v the usual advanced time).

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