Renormalised electromagnetic energy density on the horizon of a Kerr black hole

Details Renormalised electromagnetic energy density on the horizon of a Kerr black hole Renormalised electromagnetic energy density on the horizon of a Kerr black hole

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988cqgra...5l.187j&link_type=abstract

Classical and Quantum Gravity (ISSN 0264-9381), vol. 5, Nov. 1, 1988, p. L187-L189. SNSF-supported research.

Astronomy and Astrophysics

Astronomy

5

Black Holes (Astronomy), Electromagnetic Fields, Schwarzschild Metric, Space-Time Functions, Energy Distribution, Kerr Electrooptical Effect, Tensor Analysis

Scientific paper

Consideration is given to the problem of calculating the renormalized stress energy tensor of matter in thermal equilibrium with a black hole. In this paper, the values obtained by Elster (1984) and by Frolov and Zel'nikov (1985) for the renormalized energy density of the electromagnetic field in the Hartle-Hawking vacuum state on the horizon of a Schwarzschild black hole and on the pole of the event horizon of a Kerr black hole, respectively, are corrected.

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