Particle spectrum of the Reissner-Nordström black hole
arXiv:2004.03916 · doi:10.1140/epjc/s10052-020-08761-7
Abstract
The Reissner-Nordström 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-Nordström black hole emits particles in an explicit Planck distribution with temperature corresponding to the surface gravity of its outer horizon.
4 pages, 3 figures
References in corpus (3)
Cited by in corpus (23)
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