Quantum ergosphere and Hawking process.

Physics

Scientific paper

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Black Holes: Hawking Radiation

Scientific paper

The author studies both spherically symmetric and rotating (Kerr) nonstationary black holes and discusses the radiation of these black holes via the Hawking process. He finds that the thermal radiation spectrum of a nonstationary black hole is obviously dependent on the spin state of a particle and is different from the case of a stationary black hole. This effect originates from the quantum ergosphere. The author also finds that the field equations of spin s = 0, 1/2, 1 and 2 can combine into a generalized Teukolsky-type master equation with sources for any spherically symmetric black hole.

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