Quantum nonthermal effect of the Vaidya-Bonner-de Sitter black hole

Using the Hamilton-Jacobi equation of a scalar particle in the curve space-time and a correct- dimension new tortoise coordinate transformation, the quantum nonthermal radiation of the Vaidya-Bonner-de Sitter black hole is investigated. The energy condition for the occurrence of the Starobinsky-Unru...

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Bibliographic Details
Published inFrontiers of physics Vol. 9; no. 1; pp. 94 - 97
Main Author 潘伟珍 杨学军 余国祥
Format Journal Article
LanguageEnglish
Published Berlin/Heidelberg Springer Berlin Heidelberg 01.02.2014
Springer Nature B.V
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Summary:Using the Hamilton-Jacobi equation of a scalar particle in the curve space-time and a correct- dimension new tortoise coordinate transformation, the quantum nonthermal radiation of the Vaidya-Bonner-de Sitter black hole is investigated. The energy condition for the occurrence of the Starobinsky-Unruh process is obtained. The event horizon surface gravity and the Hawking temperature on the event horizon are also given.
Bibliography:Using the Hamilton-Jacobi equation of a scalar particle in the curve space-time and a correct- dimension new tortoise coordinate transformation, the quantum nonthermal radiation of the Vaidya-Bonner-de Sitter black hole is investigated. The energy condition for the occurrence of the Starobinsky-Unruh process is obtained. The event horizon surface gravity and the Hawking temperature on the event horizon are also given.
quantum nonthermal radiation, Hamilton-Jacobi equation, new tortoise coordinatetransformation, Vaidya-Bonner-de Sitter black hole
Wei-Zhen Pan, Xue-Jun Yang, Guo-Xiang Yu( Department of Physics and Electronic Information, Shaoxing University, Shaoxing 312000, China)
11-5994/O4
ISSN:2095-0462
2095-0470
DOI:10.1007/s11467-013-0383-z