Charged particle tunnels from the stationary and non-stationary Kerr-Newman black holes

Details Charged particle tunnels from the stationary and non-stationary Kerr-Newman black holes Charged particle tunnels from the stationary and non-stationary Kerr-Newman black holes

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007gregr..39.1503c&link_type=abstract

General Relativity and Gravitation, Volume 39, Issue 9, pp.1503-1515

Physics

14

Hamilton&Ndash, Jacobi Equation, Charged Particle, Self-Gravitational Interaction, Kerr&Ndash, Newman Black Hole

Scientific paper

Considering the unfixed background space-time and self-gravitational interaction, we view the Hawking radiation of a stationary Kerr-Newman black hole by Hamilton-Jacobi method. Meanwhile, extending this work to non-stationary black holes, we attempt to investigate the Hawking radiation of the non-stationary Kerr-Newman black hole. Both of the results show the tunneling probabilities are related to the change of Bekenstein- Hawking entropy and the radiation spectrums deviate from the purely thermal one, which is in accordance with the known result.

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