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Hawking effect of some axially symmetric non-stationary black holes

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Il Nuovo Cimento B (1971-1996)

Summary

The Hawking effects of the non-stationary Kerr black hole and the non-uniformly rectilinearly accelerating Kinnersley black hole are researched. Their event horizons are rotationally symmetric, but not spherically symmetric. Their Hawking temperature not only depends on time, but also on the polar angles.

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References

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Authors and Affiliations

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

    Zhao Zheng & Luo Zhi-qiang

  2. Teaching Group of Physics, Workers University of Qi Lu Petrochemistry Industrial Company, 255400, Xindian, Shandong, PRC

    Dai Xian-xin

Authors
  1. Zhao Zheng
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  2. Luo Zhi-qiang
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  3. Dai Xian-xin
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Additional information

Supported by the National Natural Science Foundation of China.

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Zheng, Z., Zhi-qiang, L. & Xian-xin, D. Hawking effect of some axially symmetric non-stationary black holes. Nuovo Cim B 109, 483–491 (1994). https://doi.org/10.1007/BF02728389

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  • DOI: https://doi.org/10.1007/BF02728389

PACS 97.60.Lf

PACS 04.20

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