Correlations between emission events in Rainbow Gravity
General Physics
2021-04-01 v2
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.
Cite
@article{arxiv.2003.00300,
title = {Correlations between emission events in Rainbow Gravity},
author = {D. A. Gomes and F. C. E. Lima and C. A. S. Almeida},
journal= {arXiv preprint arXiv:2003.00300},
year = {2021}
}
Comments
17 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