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Hawking effect of a rotating, arbitrarily accelerating black hole

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Il Nuovo Cimento B (1971-1996)

Summary

Both the event horizon equation and the radiation temperature of a rotating and arbitrarily accelerating non-stationary black hole are shown. The event horizon surface is no longer a sphere. The temperature and the spectral distribution of radiation depend on not only the time, but also the direction angles.

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Authors and Affiliations

  1. Department of Physics, Qingyang Teacher's College, 745000, Xifeng, Gansu, PRC

    Sun Ming-Chao

  2. Department of Physics, Yanbei Teacher's College, 037000, Datong, Shanxi, PRC

    Zhao Ren

  3. Department of Physics, Beijing Normal University, 100875, Beijing, PRC

    Zhao Zheng

Authors
  1. Sun Ming-Chao
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  2. Zhao Ren
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  3. Zhao Zheng
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The authors of this paper have agreed to not receive the proofs for correction.

Work supported by the National Natural Science Foundation of China.

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Ming-Chao, S., Ren, Z. & Zheng, Z. Hawking effect of a rotating, arbitrarily accelerating black hole. Nuovo Cimento B 110, 829–837 (1995). https://doi.org/10.1007/BF02820151

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  • DOI: https://doi.org/10.1007/BF02820151

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