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Quantum Anomaly and Hawking Radiation of Charged and Magnetized Reissner-Nordström de Sitter Black Hole

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Abstract

The recent work of Robinson and Wilczek that Hawking radiation can be determined by the compensating fluxes is extended to the charged and magnetized Reissner-Nordström de Sitter black hole. We reconstruct the electromagnetic field tensor and the Lagrangian of the field corresponding to the source with electric and magnetic charges to redefine an equivalent charge and gauge potential. We construct the effect field theory between the event horizon and cosmological horizon to respectively determine the compensating fluxes from them, which are shown to exactly equal to those of Hawking radiation, by the covariant anomaly cancellation conditions.

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Authors and Affiliations

  1. Computer Science of College, Chongqing Technology and Business University, Chongqing, 400067, People’s Republic of China

    Yi-Wen Han

  2. Institute of Theoretical Physics, China West Normal University, Nanchong, 637002, Sichuan, People’s Republic of China

    Xiao-Xiong Zeng & Shu-Zheng Yang

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  1. Yi-Wen Han
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  2. Xiao-Xiong Zeng
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  3. Shu-Zheng Yang
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Correspondence to Yi-Wen Han.

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Han, YW., Zeng, XX. & Yang, SZ. Quantum Anomaly and Hawking Radiation of Charged and Magnetized Reissner-Nordström de Sitter Black Hole. Int J Theor Phys 47, 2011–2020 (2008). https://doi.org/10.1007/s10773-007-9645-2

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  • DOI: https://doi.org/10.1007/s10773-007-9645-2

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