Correlations between emission events in Rainbow Gravity

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.

arXiv comment17 pages, 5 figures. Updated to match the published version to appear in Annals of Physics. Some modifications in the text but the results are unchanged

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