Correlations between emission events in Rainbow Gravity
Creators
- 1. Departament of Physics, Universidade Federal do Ceará, Campus do Pici, Fortaleza-CE, C. P. 6030, 60455-760 (Brazil)
Description
Highlights: • It is studied emission correlations between particle emission events in black holes. • Particles emitted have highly correlated moments before the BH stops radiating. • Rainbow Gravity allows maintaining the rest of it stored in its remnant. 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.
Availability note (English)
Available from http://dx.doi.org/10.1016/j.aop.2021.168436Additional details
Identifiers
- DOI
- 10.1016/j.aop.2021.168436;
- PII
- S0003491621000427;
Publishing Information
- Journal Title
- Annals of Physics (New York)
- Journal Volume
- 428
- Journal Page Range
- vp.
- ISSN
- 0003-4916
- CODEN
- APNYA6
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 53101507
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- BLACK HOLES; EVAPORATION; GRAVITATION; METRICS; NUMERICAL ANALYSIS
- Descriptors DEC
- MATHEMATICS; PHASE TRANSFORMATIONS
Optional Information
- Copyright
- Copyright (c) 2021 Elsevier Inc. All rights reserved.