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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| Format: | Article |
| Language: | English |
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Wiley
2017-01-01
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| 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. |
| format | Article |
| id | doaj-art-98ad35a15e104eba9b1a4961a03e7b47 |
| institution | Kabale University |
| issn | 1687-7357 1687-7365 |
| language | English |
| publishDate | 2017-01-01 |
| publisher | Wiley |
| record_format | Article |
| series | Advances in High Energy Physics |
| 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 |
| work_keys_str_mv | AT aliovgun thebekensteinhawkingcorpuscularcascadingfromthebackreactedblackhole AT aliovgun bekensteinhawkingcorpuscularcascadingfromthebackreactedblackhole |