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

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Abstract

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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Authors and Affiliations

  1. Institute of Theoretical Physics, China West Normal University, Nanchong, 637002, Sichuan, China

    Deyou Chen & Shuzheng Yang

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  1. Deyou Chen
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  2. Shuzheng Yang
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Correspondence to Deyou Chen.

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Chen, D., Yang, S. Charged particle tunnels from the stationary and non-stationary Kerr–Newman black holes. Gen Relativ Gravit 39, 1503–1515 (2007). https://doi.org/10.1007/s10714-007-0478-3

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  • DOI: https://doi.org/10.1007/s10714-007-0478-3

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