The Bekenstein-Hawking Corpuscular Cascading from the Backreacted Black Hole
arXiv:1609.07804 · doi:10.1155/2017/1573904
Abstract
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 backreacted 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.
10 pages, accepted for publication in Advances in High Energy Physics
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Cited by in corpus (5)
- GUP Modified Hawking Radiation in Bumblebee Gravity
- Investigating the Connection between Generalized Uncertainty Principle and Asymptotically Safe Gravity in Black Hole Signatures through Shadow and Quasinormal Modes
- Tunneling of Massive Vector Particles from Types of BTZ-like Black Holes
- Tunneling of Massive Vector Particles under the Influence of Quantum Gravity
- Tunneling of Glashow-Weinberg-Salam model particles from Black Hole Solutions in Rastall Theory