Abstract
In this work, we study emission correlations in Rainbow Gravity (RG)
black holes known to have black hole remnants. Non-thermal corrections
are responsible for generating non-zero correlations between particle
emission events during the black hole evaporation process. With this in
mind, we calculate the temperatures considering back-reaction effects.
Then, we obtain the correlations between emission events for a RG metric
proposed by Magueijo and Smolin. We also discuss through a numerical
analysis the emission correlations behavior in the last stages of
evaporation of the black hole. (C) 2021 Elsevier Inc. All rights
reserved.
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