Hawking radiation from charged black holes via gauge and gravitational anomalies.
Hawking radiation from charged black holes via gauge and gravitational anomalies.
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DOI：
10.1103/physrevlett.96.151302
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发表时间：
2006-02
影响因子：
8.6
通讯作者：
S. Iso;H. Umetsu;F. Wilczek
中科院分区：
文献类型：
--
作者：
S. Iso;H. Umetsu;F. Wilczek
推广Robinson和Wolczek的方法，我们证明了为了避免在量子水平上的一般协方差和规范不变性的破坏，在Reissner-Nordström黑洞背景中带电量子场的每个出射部分波的总电荷和能量通量必须等于具有适当化学势的（1 + 1）维黑体在霍金温度下的总电荷和能量通量。
Extending the method of Robinson and Wolczek, we show that in order to avoid a breakdown of general covariance and gauge invariance at the quantum level the total flux of charge and energy in each outgoing partial wave of a charged quantum field in a Reissner-Nordström black hole background must be equal to that of a (1 + 1)-dimensional blackbody at the Hawking temperature with the appropriate chemical potential.