This is an extended version of the previous paper [S. Iso, T. Morita, and H. Umetsu, Phys. Rev. D 75, 124004 (2007).]. Quantum fields near horizons can be described in terms of an infinite set of two-dimensional conformal fields. We first generalize the method of Christensen and Fulling to charged black holes to derive fluxes of energy and charge. These fluxes can be obtained by employing a conformal field theory technique. We then apply this technique to obtain the fluxes of higher-spin currents and show that the thermal distribution of Hawking radiation from a charged black hole can be completely reproduced by investigating transformation properties of the higher-spin currents under conformal and gauge transformations.
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Sogang Univ, Dept Phys, Seoul 100611, South Korea
Sogang Univ, Ctr Quantum Spacetime, Seoul 100611, South KoreaSogang Univ, Dept Phys, Seoul 100611, South Korea
Kim, Wontae
Shin, Hyeonjoon
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Sogang Univ, Ctr Quantum Spacetime, Seoul 121742, South KoreaSogang Univ, Dept Phys, Seoul 100611, South Korea
Shin, Hyeonjoon
Yoon, Myungseok
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Sogang Univ, Ctr Quantum Spacetime, Seoul 121742, South KoreaSogang Univ, Dept Phys, Seoul 100611, South Korea
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Huazhong Normal Univ, Coll Phys Sci & Technol, Wuhan 430079, Hubei, Peoples R ChinaHuazhong Normal Univ, Coll Phys Sci & Technol, Wuhan 430079, Hubei, Peoples R China
Wu, Shuang-Qing
Peng, Jun-Jin
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Huazhong Normal Univ, Coll Phys Sci & Technol, Wuhan 430079, Hubei, Peoples R China
Wuhan Text Univ, Coll Sci, Wuhan 430074, Hubei, Peoples R ChinaHuazhong Normal Univ, Coll Phys Sci & Technol, Wuhan 430079, Hubei, Peoples R China