Back reaction on a Reissner-Nordström black hole

Details Back reaction on a Reissner-Nordström black hole Back reaction on a Reissner-Nordström black hole

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001phrvd..63l4014w&link_type=abstract

Physical Review D, vol. 63, Issue 12, id. 124014

Physics

1

Quantum Aspects Of Black Holes, Evaporation, Thermodynamics, Exact Solutions, Quantum Field Theory In Curved Spacetime

Scientific paper

The perturbed (``dressed'') metric of the conformally invariant scalar field in a Reissner-Nordström (RN) black hole is given by solving the semiclassical Einstein and Maxwell equations according to York's back-reaction approach. Some properties of the ``dressed'' black hole are obtained, such as its ``dressed'' mass, the location of the event horizon, and its surface gravity. It will also be found that the hypersurfaces of r+ and r-, which are the event and Cauchy horizons in the ``naked'' RN black hole, become spacelike in the perturbed geometry.

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