  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.
