Fluxes of higher-spin currents and Hawking radiation from charged black holes

被引:40
|
作者
Iso, Satoshi
Morita, Takeshi
Umetsu, Hiroshi
机构
[1] High Energy Accelerator Res Org, KEK, Inst Particle & Nucl Studies, Tsukuba, Ibaraki 3050801, Japan
[2] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan
[3] Okayama Inst Quantum Phys, Okayama 7000015, Japan
关键词
D O I
10.1103/PhysRevD.76.064015
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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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页数:8
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