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Published in 2020 at "Physical Review D"
DOI: 10.1103/physrevd.101.104050
Abstract: Modeling the collapse of an extreme Reissner-Nordstrom (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…
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Keywords:
radiation;
extremal hawking;
hawking radiation;