Quantum thermal effect of quasi-static evaporating charged black hole.

Details Quantum thermal effect of quasi-static evaporating charged black hole. Quantum thermal effect of quasi-static evaporating charged black hole.

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997sccha..40..201z&link_type=abstract

Science in China, Series A, Vol. 40, No. 2, p. 201 - 205

Computer Science

1

Black Holes: Temperatures

Scientific paper

The study of the quantum thermal effect of a non-static black hole is generalized to the space-time with coordinates (t,r) as variables. Tortoise coordinate equations which are different from not only static space-time but also the non-static space-time described by the advanced-Eddington coordinate v have been chosen. Under the condition that the effect of Hawking evaporation is considered, the temperature of the black hole and the location of the horizon are shown. The results indicate that the Hawking radiation temperature can be regarded as a compensating effect under the time-scale transformation.

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