Published June 2021
| Version v1
Journal article
Thermal dimensional reduction and black hole evaporation
Creators
- 1. Physics Department, Federal University of Lavras, Caixa Postal 3037, 37200-000 Lavras-MG (Brazil)
- 2. Department of Chemistry and Physics, Federal University of Paraíba, Rodovia BR 079 - km 12, 58397-000 Areia-PB (Brazil)
- 3. Institute of Mathematics and Computation, Federal University of Itajubá, 37500-903 Itajubá (Brazil)
Description
We analyze how a quantum-gravity-induced change in the number of thermal dimensions (through a modified dispersion relation) affects the geometry and the thermodynamics of a charged black hole. To that end we resort to Kiselev's solution as the impact such modifications have on the evaporation rate of the black hole becomes more clear. As an application, we study the case for which the thermal dimension is reduced to two.
Availability note (English)
Available from http://dx.doi.org/10.1016/j.physletb.2021.136272Additional details
Identifiers
- DOI
- 10.1016/j.physletb.2021.136272;
- PII
- S0370269321002124;
Publishing Information
- Journal Title
- Physics Letters. Section B
- Journal Volume
- 817
- Journal Page Range
- vp.
- ISSN
- 0370-2693
- CODEN
- PYLBAJ
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 54011398
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- BLACK HOLES; DISPERSION RELATIONS; EVAPORATION; GEOMETRY; QUANTUM GRAVITY; THERMODYNAMICS
- Descriptors DEC
- FIELD THEORIES; MATHEMATICS; PHASE TRANSFORMATIONS; QUANTUM FIELD THEORY
Optional Information
- Copyright
- Copyright (c) 2021 The Author(s). Published by Elsevier B.V.