Iso Satoshi, Umetsu Hiroshi, Wilczek Frank
Center for Theoretical Physics, Laboratory for Nuclear Science and Department of Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA.
Phys Rev Lett. 2006 Apr 21;96(15):151302. doi: 10.1103/PhysRevLett.96.151302. Epub 2006 Apr 19.
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.
通过扩展罗宾逊和沃尔采克的方法，我们证明，为了避免在量子水平上广义协变性和规范不变性的失效，在雷斯纳 - 诺德斯特龙黑洞背景下，带电量子场的每个出射分波中的电荷和能量总通量必须等于具有适当化学势的霍金温度下的（1 + 1）维黑体的通量。
