The fluctuation of black hole's energy and the upper bound to the temperature of the radiation in the vicinity of black hole

Details The fluctuation of black hole's energy and the upper bound to the temperature of the radiation in the vicinity of black hole The fluctuation of black hole's energy and the upper bound to the temperature of the radiation in the vicinity of black hole

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982acpsn..31.1436z&link_type=abstract

Acta Physica Sinica, vol. 31, Oct. 1982, p. 1436-1439. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

Black Holes (Astronomy), Extremum Values, Radiation Distribution, Space-Time Functions, Temperature Distribution, Canonical Forms, Distribution Functions, Fluctuation Theory, Quantum Mechanics, Schwarzschild Metric

Scientific paper

The distribution function of the temperature in the case of static 1 + 1
dimensions have been obtained by using canonical method of quantum field
in curved space-time. We then estimate the upper bound to the
temperature of the radiation in 1 + 1 dimensional Schwarzschild
space-time by calculating the fluctuation of black hole's energy.

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