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    • Keywords


      Hamilton-Jacobi method; energy conservation; Bekenstein-Hawking entropy; tunneling rate; spatial distance.

    • 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.

    • Author Affiliations


      Xiao-Xiong Zeng1 Jian-Song Hou1 Shu-Zheng Yang1

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

  • Pramana – Journal of Physics | News

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      Posted on July 25, 2019

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