Particle spectrum of the Reissner-Nordstrom black hole

被引：23
|
作者：
Good, Michael R. R. [1 ,3 ,4 ]
Ong, Yen Chin [1 ,2 ]
机构：
[1] Yangzhou Univ, Ctr Gravitat & Cosmol, Yangzhou, Jiangsu, Peoples R China
[2] Yangzhou Univ, Coll Phys Sci & Technol, Yangzhou, Jiangsu, Peoples R China
[3] Nazarbayev Univ, Phys Dept, Nur Sultan, Kazakhstan
[4] Nazarbayev Univ, Energet Cosmos Lab, Nur Sultan, Kazakhstan
来源：
EUROPEAN PHYSICAL JOURNAL C | 2020年 / 80卷 / 12期
基金：
中国国家自然科学基金;
关键词：
RADIATION;
D O I：
10.1140/epjc/s10052-020-08761-7
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
The Reissner-Nordstrom black hole - moving mirror correspondence is solved. The beta coefficients reveal that charge makes a black hole radiate fewer particles (neutral massless scalars) per frequency. An old Reissner-Nordstrom black hole emits particles in an explicit Planck distribution with temperature corresponding to the surface gravity of its outer horizon.
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页数：5
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