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1985•Progress of Theoretical PhysicsOpen access

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

Shin-ichi Tadaki, S. Takagi

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Abstract

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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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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Available abstract

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.

Key concepts: Physics, Hawking radiation, Planck, Black hole (networking), Entropy (arrow of time), Schwarzschild radius, Micro black hole, Radiation

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