The Bekenstein-Hawking Corpuscular Cascading from the Back-Reacted Black Hole

Exciting peculiarities of Planck-scale physics have immediate effects on the Bekenstein-Hawking radiation emitted from black holes (BHs). In this paper, using the tunneling formalism, we determine the Bekenstein-Hawking temperature for the vector particles from a back-reacted black hole (BBH) constr...

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Main Author: Ali Övgün
Format: Article
Language:English
Published: Wiley 2017-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2017/1573904
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author Ali Övgün
author_facet Ali Övgün
author_sort Ali Övgün
collection DOAJ
description Exciting peculiarities of Planck-scale physics have immediate effects on the Bekenstein-Hawking radiation emitted from black holes (BHs). In this paper, using the tunneling formalism, we determine the Bekenstein-Hawking temperature for the vector particles from a back-reacted black hole (BBH) constructed from a conformal scalar field surrounded by a BTZ (Banados-Teitelboim-Zanelli) BH. Then, under the effect of the generalized uncertainty principle, we extend our calculations for scalar particles to understand the effects of quantum gravity. Then, we calculate an evaporation time for the BBH, the total number of Bekenstein-Hawking particles, and the quantum corrections of the number. We observe that remnants of the BH evaporation occur and that they affect the Bekenstein-Hawking temperature of the BBH as well as the total number of Bekenstein-Hawking particles.
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spelling doaj-art-98ad35a15e104eba9b1a4961a03e7b472025-08-20T03:37:22ZengWileyAdvances in High Energy Physics1687-73571687-73652017-01-01201710.1155/2017/15739041573904The Bekenstein-Hawking Corpuscular Cascading from the Back-Reacted Black HoleAli Övgün0Instituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla 4950, Valparaíso, ChileExciting peculiarities of Planck-scale physics have immediate effects on the Bekenstein-Hawking radiation emitted from black holes (BHs). In this paper, using the tunneling formalism, we determine the Bekenstein-Hawking temperature for the vector particles from a back-reacted black hole (BBH) constructed from a conformal scalar field surrounded by a BTZ (Banados-Teitelboim-Zanelli) BH. Then, under the effect of the generalized uncertainty principle, we extend our calculations for scalar particles to understand the effects of quantum gravity. Then, we calculate an evaporation time for the BBH, the total number of Bekenstein-Hawking particles, and the quantum corrections of the number. We observe that remnants of the BH evaporation occur and that they affect the Bekenstein-Hawking temperature of the BBH as well as the total number of Bekenstein-Hawking particles.http://dx.doi.org/10.1155/2017/1573904
spellingShingle Ali Övgün
The Bekenstein-Hawking Corpuscular Cascading from the Back-Reacted Black Hole
Advances in High Energy Physics
title The Bekenstein-Hawking Corpuscular Cascading from the Back-Reacted Black Hole
title_full The Bekenstein-Hawking Corpuscular Cascading from the Back-Reacted Black Hole
title_fullStr The Bekenstein-Hawking Corpuscular Cascading from the Back-Reacted Black Hole
title_full_unstemmed The Bekenstein-Hawking Corpuscular Cascading from the Back-Reacted Black Hole
title_short The Bekenstein-Hawking Corpuscular Cascading from the Back-Reacted Black Hole
title_sort bekenstein hawking corpuscular cascading from the back reacted black hole
url http://dx.doi.org/10.1155/2017/1573904
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