Stress-energy tensor near a charged, rotating, evaporating black hole

Details Stress-energy tensor near a charged, rotating, evaporating black hole Stress-energy tensor near a charged, rotating, evaporating black hole

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977phrvd..15.3054h&link_type=abstract

Physical Review D (Particles and Fields), Volume 15, Issue 10, 15 May 1977, pp.3054-3057

Physics

32

Scientific paper

The recently developed two-dimensional stress-energy regularization techniques are applied to the two-dimensional analog of the Reissner-Nordström family of black-hole metrics. The calculated stress-energy tensor in all cases contains the thermal radiation discovered by Hawking. Implications for the evolution of the interior of a charged black hole are considered. The calculated stress-energy tensor is found to diverge on the inner, Cauchy, horizon. Thus the effect of quantum mechanics is to cause the Cauchy horizon to become singular. The stress-energy tensor is also calculated for the "most reasonable" two-dimensional analog of the Kerr-Newman family of black-hole metrics. Although the analysis is not as rigorous as in the Reissner-Nordström case, it appears that the correct value for the Hawking radiation also appears in this model.

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