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      https://www.ias.ac.in/article/fulltext/pram/070/03/0409-0415

    • 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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