Particle spectrum of the Reissner–Nordström black hole
Michael R. R. GoodCenter for Gravitation and Cosmology, Yangzhou University, Yangzhou, ChinaYen Chin OngCenter for Gravitation and Cosmology, Yangzhou University, Yangzhou, China
2020en
ABI
Abstract
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.
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Cited by 30 references