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The Bekenstein-Hawking Corpuscular Cascading from the Back-Reacted Black Hole
Author
Source
Advances in High Energy Physics
Issue
Vol. 2017, Issue 2017 (31 Dec. 2017), pp.1-9, 9 p.
Publisher
Hindawi Publishing Corporation
Publication Date
2017-08-20
Country of Publication
Egypt
No. of Pages
9
Main Subjects
Abstract EN
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.
American Psychological Association (APA)
Övgün, Ali. 2017. The Bekenstein-Hawking Corpuscular Cascading from the Back-Reacted Black Hole. Advances in High Energy Physics،Vol. 2017, no. 2017, pp.1-9.
https://search.emarefa.net/detail/BIM-1121950
Modern Language Association (MLA)
Övgün, Ali. The Bekenstein-Hawking Corpuscular Cascading from the Back-Reacted Black Hole. Advances in High Energy Physics No. 2017 (2017), pp.1-9.
https://search.emarefa.net/detail/BIM-1121950
American Medical Association (AMA)
Övgün, Ali. The Bekenstein-Hawking Corpuscular Cascading from the Back-Reacted Black Hole. Advances in High Energy Physics. 2017. Vol. 2017, no. 2017, pp.1-9.
https://search.emarefa.net/detail/BIM-1121950
Data Type
Journal Articles
Language
English
Notes
Includes bibliographical references
Record ID
BIM-1121950