Hawking radiation from charged black holes via gauge and gravitational anomalies

被引：208

作者：

Iso, S ^{[1
]}

Umetsu, H

Wilczek, F

机构：

[1] MIT, Ctr Theoret Phys, Nucl Sci Lab, Cambridge, MA 02139 USA

[2] MIT, Dept Phys, Cambridge, MA 02139 USA

[3] KEK, High Energy Accelerator Res Org, Inst Particle & Nucl Studies, Tsukuba, Ibaraki 3050801, Japan

[4] Okayama Inst Quantum Phys, Okayama 7000015, Japan

来源：

PHYSICAL REVIEW LETTERS | 2006年 / 96卷 / 15期

关键词：

D O I：

10.1103/PhysRevLett.96.151302

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

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.

引用

页数：4

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