EXTREME HAWKING RADIATION
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Date
2020
Authors
Good, Michael R.R.
Journal Title
Journal ISSN
Volume Title
Publisher
arxiv
Abstract
Modeling the collapse of an extreme Reissner-Nordstr¨om (ERN) black hole by solving the corre sponding moving mirror model for the trajectory that asymptotically approaches uniform accelera tion, 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
Description
Keywords
Type of access: Open Access, radiation, extreme Reissner-Nordstr¨om
Citation
Good, M. R. (2020). Extremal Hawking radiation. Physical Review D, 101(10). https://doi.org/10.1103/physrevd.101.104050