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Remarks on Hawking radiation as tunneling from a uniformly accelerating black hole

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Abstract

Motivated by the Hamilton-Jacobi method of Angheben et al, we investigate the Hawking tunneling radiation from a uniformly accelerating rectilinear black hole for which the horizons and entropy are functions of θ. After several coordinate transformations, we conclude that when the self-gravitational interaction and energy conservation are taken into account, the actual radiation spectrum deviates from the thermal one and the tunneling rate is the function of θ though it is still related to the change of the Bekenstein-Hawking entropy.

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Authors and Affiliations

  1. Institute of Theoretical Physics, China West Normal University, Nanchang, 637002, Sichuan, People’s Republic of China

    Xiao-Xiong Zeng, Jian-Song Hou & Shu-Zheng Yang

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  1. Xiao-Xiong Zeng
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  2. Jian-Song Hou
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  3. Shu-Zheng Yang
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Correspondence to Xiao-Xiong Zeng.

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Zeng, XX., Hou, JS. & Yang, SZ. Remarks on Hawking radiation as tunneling from a uniformly accelerating black hole. Pramana - J Phys 70, 409–415 (2008). https://doi.org/10.1007/s12043-008-0058-4

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  • DOI: https://doi.org/10.1007/s12043-008-0058-4

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