The Tunneling Radiation from Non-Stationary Spherical Symmetry Black Holes and the Hamilton-Jacobi Equation

We derive the Hamilton-Jacobi equation from the Dirac equation, then, with the help of the Hamilton-Jacobi equation, the the tunneling radiation behavior of the non-stationary spherical symmetry de Sitter black hole is discussed, at last, we obtained the tunneling rate and Hawking temperature. Our r...

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Bibliographic Details
Published inInternational journal of theoretical physics Vol. 56; no. 2; pp. 546 - 553
Main Authors Yang, Shu-Zheng, Feng, Zhong-Wen, Li, Hui-Ling
Format Journal Article
LanguageEnglish
Published New York Springer US 01.02.2017
Springer Nature B.V
Subjects
Black holes
Dirac equation
Elementary Particles
Hamilton-Jacobi equation
Human behavior
Linear equations
Mathematical and Computational Physics
Physics
Physics and Astronomy
Quantum Field Theory
Quantum Physics
Quantum theory
Symmetry
Theoretical
Non-stationary spherical symmetry black hole
Spin particles
Hamilton-Jacobi equation
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Summary:We derive the Hamilton-Jacobi equation from the Dirac equation, then, with the help of the Hamilton-Jacobi equation, the the tunneling radiation behavior of the non-stationary spherical symmetry de Sitter black hole is discussed, at last, we obtained the tunneling rate and Hawking temperature. Our results showed that the Hamilton-Jacobi equation is a fundamental dynamic equation, it can widely be derived from the dynamic equations which describe the particles with any spin. Therefore, people can easy calculate the tunneling behavior from the black holes.
ISSN:0020-7748
1572-9575
DOI:10.1007/s10773-016-3196-3