期刊
PHYSICAL REVIEW LETTERS
卷 96, 期 15, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.96.151302
关键词
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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-Nordstrom black hole background must be equal to that of a (1+1)-dimensional blackbody at the Hawking temperature with the appropriate chemical potential.
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