Abstract
The Hawking radiation of Dirac particles in a charged Vaidya–de Sitter black hole is investigated by using the method of generalized tortoise coordinate transformation. It is shown that the Hawking radiation of Dirac particles does not exist for P1, Q2 components, but for P2, Q1 components it does. Both the location and the temperature of the event horizon change with time. The thermal radiation spectrum of Dirac particles is the same as that of Klein-Gordon particles.
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Wu, S.Q., Cai, X. Asymmetry of Hawking Radiation of Dirac Particles in a Charged Vaidya–de Sitter Black Hole. International Journal of Theoretical Physics 40, 1349–1357 (2001). https://doi.org/10.1023/A:1017544225356
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DOI: https://doi.org/10.1023/A:1017544225356