Abstract
Hawking radiation arising from the electromagnetic fields in the Kerr–Newman black hole is studied exactly by using the Newman–Penrose formalism and the tortoise coordinate. It is shown that the thermal radiation spectrum due to the photons in the Kerr–Newman black hole does not depend on the spins of the particles, and the effect is exactly same as that of the Klein–Gordon scalar particles.
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REFERENCES
Ahmed, M. (1987). Classical and QuantumGravity 4, 431.
Ahmed, M. and Mondal, A. K. (1993).Physics Letters A 184, 37.
Carmeli, M. (1982).Classical Fields: General Relativity and Gauge Theory, Wiley-Interscience, New York.
Chandrasekhar, S. (1992). The Mathematical Theory of Black Hole,Oxford University Press, Oxford.
Dai, X. and Zhao, Z. (1992). Acta Physica Sinica 41, 869.
Dai, X., Zhao, Z., and Liu, L. (1993). Science in China A 23,69.
Damour, T. and Ruffini, R. (1976). Physical Review D 14,332.
Hawking, S. W. (1975). Communications in Mathematical Physics 43, 199.
Jing, J. L. and Wang, Y. J. (1996). International Journal ofTheoretical Physics 35, 11841.
Jing, J. L. and Wang, Y. J. (1997). International Journal ofTheorietical Physics 36, 1745.
Kerr, R. P. (1963). Physical Review Letters 11, 237.
Liu, L. and Xu, D. Y. (1980). Acta Physica Sinica 29,1617.
Newman, E. T., Couch, E., Chinnapared, K., Exton, A., Prakash, A., and Torrence, R. (1965). Journal of Mathematical Physics 6, 918.
Sannan, S. (1988). General Relativity and Gravitation 20,239.
Zhao, Z. and Gui, Y. X. (1983). Acta Astophysica 3, 146.
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Jing, J. Hawking Radiation Arising from the Electromagnetic Fields in the Kerr–Newman Black Hole. International Journal of Theoretical Physics 41, 101–107 (2002). https://doi.org/10.1023/A:1013225717494
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DOI: https://doi.org/10.1023/A:1013225717494