VAIDYA SPACE-TIME AS AN EVAPORATING BLACK HOLE

Feb, 1984
10 pages
Published in:
  • Prog.Theor.Phys. 71 (1984) 1422
Report number:
  • RRK 84-4

Citations per year

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Abstract: (Oxford Journals)
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).