Accurate correction of arbitrary spin fermion quantum tunneling from non-stationary Kerr-de Sitter black hole based on corrected Lorentz dispersion relation

Abstract According to a corrected dispersion relation proposed in the study on the string theory and quantum gravity theory, the Rarita-Schwinger equation was precisely modified, which resulted in the Rarita-Schwinger-Hamilton-Jacobi equation. Using this equation, the characteristics of arbitrary sp...

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Published inChinese physics C Vol. 44; no. 12; p. 125104
Main Authors Sha, Bei, Liu, Zhi-E, Liu, Yu-Zhen, Tan, Xia, Zhang, Jie, Yang, Shu-Zheng
Format Journal Article
LanguageEnglish
Published 01.12.2020
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Summary:Abstract According to a corrected dispersion relation proposed in the study on the string theory and quantum gravity theory, the Rarita-Schwinger equation was precisely modified, which resulted in the Rarita-Schwinger-Hamilton-Jacobi equation. Using this equation, the characteristics of arbitrary spin fermion quantum tunneling radiation from non-stationary Kerr-de Sitter black holes were determined. A number of accurately corrected physical quantities, such as surface gravity, chemical potential, tunneling probability, and Hawking temperature, which describe the properties of black holes, were derived. This research has enriched the research methods and enabled increased precision in black hole physics research.
ISSN:1674-1137
2058-6132
DOI:10.1088/1674-1137/abb4d6