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Hawking Radiation of Spin-3/2 Particles from Kerr Black Hole

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Abstract

By using dimensional reduction and consistent anomaly method, we calculate the Hawking flux of the spin- 3/2 field in the Kerr black hole background. The results confirm that the Hawking radiation doesn’t depends on the detail of the fields living near the horizon, at least at the semi-classical level. The Hawking temperature is an universality character of black hole which only depends on the information of the horizon. Our calculation agrees with earlier results obtained by the WKB/tunneling method (Yale and Mann, Phys. Lett. B 673(2), 168–172, 2009).

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Authors and Affiliations

  1. School of Sciences, Southwest Petroleum University, Chengdu, Sichuan, 610500, China

    Shihong Tong

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  1. Shihong Tong
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Correspondence to Shihong Tong.

Additional information

This work is supported by technology fund of Southwest Petroleum University (grant no. 2013XJZ026).

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Tong, S. Hawking Radiation of Spin-3/2 Particles from Kerr Black Hole. Int J Theor Phys 55, 854–860 (2016). https://doi.org/10.1007/s10773-015-2727-7

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  • DOI: https://doi.org/10.1007/s10773-015-2727-7

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