On Hawking Radiation of 3D Rotating Hairy Black Holes
A. Belhaj, M. Chabab, H. EL Moumni, K. Masmar, M. B. Sedra
TL;DR
This paper investigates Hawking radiation in three-dimensional rotating hairy black holes, revealing that particle transition probabilities depend on scalar hair charge and rotation but not on particle type.
Contribution
It provides the first detailed analysis of how scalar hair and rotation influence Hawking radiation in 3D black holes.
Findings
Transition probability is independent of particle type.
Scalar hair charge B affects the radiation probability.
Rotation parameter a influences the transition probability.
Abstract
We study the Hawking radiation of 3D rotating hairy black holes. More concretely, we compute the transition probability of a bosonic and fermionic particle in such backgrounds. Thew, we show that the transition probability is independent of the nature of the particle. It is observed that the charge of the scalar hair B and the rotation parameter a control such a probability.
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