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- W2891809889 abstract "By using the deformed dispersion relation, we study the modified fermions tunneling for rotating charged black hole in de Sitter spacetime. Firstly, the Rarita-Schwinger equation is modified in the gravitational background, and then the deformed Hamilton-Jacobi equation is derived by a semi-classical approximation method. It is shown that the form of the correctional Hamilton-Jacobi equation does not depend on the spin of the fermions field in the semi-classical approximation, and its correctional term is given by − 2 σ m g t t ( ω − e A t ) 2 . Using the correction, we also investigate the fermion tunneling radiation for Kerr-Newman-de Sitter black hole spacetime, and the results show that the correctional temperature and entropy depend on the angular parameters of the horizon of the rotating black hole background." @default.
- W2891809889 created "2018-09-27" @default.
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- W2891809889 date "2018-12-10" @default.
- W2891809889 modified "2023-10-02" @default.
- W2891809889 title "Modified fermions tunneling radiation from Kerr-Newman-de Sitter black hole" @default.
- W2891809889 doi "https://doi.org/10.1360/sspma2018-00307" @default.
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