Charged Particles' Tunneling from Hot-NUT-Kerr-Newman-Kasuya Spacetime

Details Charged Particles' Tunneling from Hot-NUT-Kerr-Newman-Kasuya Spacetime Charged Particles' Tunneling from Hot-NUT-Kerr-Newman-Kasuya Spacetime

2007-07-07

arxiv.org/abs/0707.1079v3

Int J Theor Phys (2008) 47: 2203--2217

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

To appear in: Int. J. Theor. Phys

Scientific paper

10.1007/s10773-008-9652-y

We study the Hawking radiation as charged particles' tunneling across the horizons of the Hot-NUT-Kerr-Newman-Kasuya spacetime by considering the spacetime background as dynamical and incorporating the self-gravitation effect of the emitted particles when the energy conservation, the angular momentum conservation, and the electric charge conservation are taken into account. Our result shows that the tunneling rate is related to the change of Bekenstein-Hawking entropy and the radiant spectrum is not pure thermal, but is consistent with an underlying unitary theory. The emission process is a reversible one, and the information is preserved as a natural result of the first law of black hole thermodynamics.

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