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Anomaly analysis of Hawking radiation from Kaluza–Klein black hole with squashed horizon

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Abstract

Considering gravitational and gauge anomalies at the horizon, a new method to derive Hawking radiation from black holes has been developed by Wilczek et al. In this paper, we apply this method to non-rotating and rotating Kaluza–Klein black holes with squashed horizon, respectively. For the rotating case, we found that, after dimensional reduction, an effective U(1) gauge field is generated by an angular isometry. The results show that the gauge current and energy-momentum tensor fluxes are exactly equivalent to Hawking radiation from the event horizon.

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Authors and Affiliations

  1. Institute of Theoretical Physics, Lanzhou University, Lanzhou, 730000, P.R. China

    Shao-Wen Wei, Ran Li, Yu-Xiao Liu & Ji-Rong Ren

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  1. Shao-Wen Wei
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  2. Ran Li
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  3. Yu-Xiao Liu
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  4. Ji-Rong Ren
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Correspondence to Yu-Xiao Liu.

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Wei, SW., Li, R., Liu, YX. et al. Anomaly analysis of Hawking radiation from Kaluza–Klein black hole with squashed horizon. Eur. Phys. J. C 65, 281–287 (2010). https://doi.org/10.1140/epjc/s10052-009-1203-z

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