Phenomenological Theory of the Equilibrium State of the System with a Black Hole and Radiation

Details Phenomenological Theory of the Equilibrium State of the System with a Black Hole and Radiation Phenomenological Theory of the Equilibrium State of the System with a Black Hole and Radiation

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pthph..73..288t&link_type=abstract

Progress of Theoretical Physics, Vol. 73, No. 1, pp. 288-291

Physics

1

Scientific paper

We improve Hawking's equilibrium theory of an isolated system consisting
of a black hole and radiation, taking account of the modification of the
energy and the entropy of the radiation due to the background
Schwarzschild geometry. The effect is found to become recognizable when
the total energy is less than about 104 times Planck mass.

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