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arXiv · 2003.07016

Extreme Hawking Radiation

Michael R. R. Good
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Abstract

Modeling the collapse of an extreme Reissner-Nordström (ERN) black hole by solving the corresponding moving mirror model for the trajectory that asymptotically approaches uniform acceleration, we obtain the non-zero beta coefficients for all times. Finite energy is emitted, the radiation spectra is non-thermal (non-steady / not Planck), soft particles characterize the evaporation, and particle production at ultra-late times is damped. Entanglement entropy diverges with no Page curve turn-over, demonstrating non-thermal information loss. The radiation obeys time-reversal symmetry.

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Michael R. R. Good. 2020-03-16. Extreme Hawking Radiation. https://doi.org/10.1103/physrevd.101.104050

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