Abstract
After taking into account energy conservation and the particle’s self-gravitation interaction, Hawking radiation of the massive particle as tunneling from Schwarzshild-anti-de Sitter black hole is studied by using Parikh-Wilczek’s semi-classical quantum tunneling approach. Meanwhile, Hawking radiation as tunneling from the black hole is reexamined by developing Angheben–Nadalini–Vanzo–Zerbini (ANVZ) covariant method to cover energy conservation and the particle’s self-gravitation interaction. Both the results perfectly generalize those obtained by Parikh and Wilczek, and show that the tunneling rate is related to the change of Bekenstein-Hawking entropy, and the factual emission spectrum is not exactly thermal, but satisfies the underlying unitary theory.
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PACS: 04.70-s, 9760. Lf.
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Yang, SZ., Jiang, QQ. Research on Hawking Radiation as Tunneling from Schwarzshild-anti-de Sitter Black Hole. Int J Theor Phys 46, 2138–2145 (2007). https://doi.org/10.1007/s10773-006-9334-6
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DOI: https://doi.org/10.1007/s10773-006-9334-6