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.
%0 Journal Article
%1 WOS:000645091200011
%A Gomes, D A
%A Lima, F C E
%A Almeida, C A S
%C 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA
%D 2021
%I ACADEMIC PRESS INC ELSEVIER SCIENCE
%J ANNALS OF PHYSICS
%K Back-reaction Black Gravity; Rainbow correlation; effect} hole; {Emission
%R 10.1016/j.aop.2021.168436
%T Correlations between emission events in Rainbow Gravity
%V 428
%X 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.
@article{WOS:000645091200011,
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.},
added-at = {2022-05-23T20:00:14.000+0200},
address = {525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA},
author = {Gomes, D A and Lima, F C E and Almeida, C A S},
biburl = {https://www.bibsonomy.org/bibtex/26f084974471a7e3b547e91399ece0c6c/ppgfis_ufc_br},
doi = {10.1016/j.aop.2021.168436},
interhash = {216c02eb35708792effdd0ecacfdd7a4},
intrahash = {6f084974471a7e3b547e91399ece0c6c},
issn = {0003-4916},
journal = {ANNALS OF PHYSICS},
keywords = {Back-reaction Black Gravity; Rainbow correlation; effect} hole; {Emission},
publisher = {ACADEMIC PRESS INC ELSEVIER SCIENCE},
pubstate = {published},
timestamp = {2022-05-23T20:00:14.000+0200},
title = {Correlations between emission events in Rainbow Gravity},
tppubtype = {article},
volume = 428,
year = 2021
}