The solution of a modified Hamilton–Jacobi equation with Lorentz-violating scalar field

A modified Hamilton–Jacobi equation with Lorentz-violating scalar field in the curved spacetime is used to research tunneling radiation from the horizons of Reissner–Nordstr o ¨ m de Sitter black hole. We investigate the influence of different etheric-like vector u α on the solution of the modified...

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Bibliographic Details
Published inGeneral relativity and gravitation Vol. 52; no. 11
Main Authors Zhang, Jie, Liu, Menquan, Liu, Zhie, Sha, Bei, Tan, Xia, Liu, Yuzhen
Format Journal Article
LanguageEnglish
Published New York Springer US 01.11.2020
Springer Nature B.V
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Summary:A modified Hamilton–Jacobi equation with Lorentz-violating scalar field in the curved spacetime is used to research tunneling radiation from the horizons of Reissner–Nordstr o ¨ m de Sitter black hole. We investigate the influence of different etheric-like vector u α on the solution of the modified Hamilton–Jacobi equation by using both the semi-classical approximation and beyond the semi-classical approximation. We find that the solution of the modified Hamilton–Jacobi equation strongly depends on the choices of u α . As u α = δ t α u t , the Lorentz-violating scalar field can enhances black holes’ Hawking temperature but reduces its entropy. However, the case will reverses as u α = δ r α u r . Our conclusions are applicable to other spherically symmetric charged black holes.
ISSN:0001-7701
1572-9532
DOI:10.1007/s10714-020-02762-3