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.
arXiv comment4 pages, 3 figures
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- Light and Airy: a simple solution for relativistic quantum acceleration radiation
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- On the microstructure of higher-dimensional Reissner-Nordström black holes in quantum regime
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- Upon the horizon's verge: Thermal particle creation between and approaching horizons
- Moving mirrors and event horizons in non-flat background geometry
- There and Back Again: Quantum Radiation from Round-trip Flying Mirrors
- Analog Hawking radiation emitted by a perfectly reflecting mirror
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- Pure Gauss-Bonnet NUT Black Hole Solution: II