2015/08/19 by A. Belhaj, M. Chabab, H. El Moumni +3
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Black hole (networking) #Charge (physics) #Cosmology and Gravitation Theories #Entropy (arrow of time) #Geometry #Hawking #Hawking radiation #Mathematical physics #Mathematics #Micro black hole #Physics #Quantum Electrodynamics and Casimir Effect #Quantum electrodynamics #Quantum mechanics #Radiation #Scalar (mathematics) #hep-th
paper · pdf · doi:10.1088/0256-307x/32/10/100401
published in Chinese Physics Letters 32(10), 100401 (Institute of Physics) · 8 pages. latex. Final version accepted by Chin. Phys. Lett (2015)
arxiv created 2015/08/19 · openalex publication_date 2015/10/01 · arxiv updated 2015/10/28 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We study the Hawking radiation of 3D rotating hairy black holes. Specifically, we compute the transition probability of bosonic and fermionic particles in such backgrounds. Then, we show that the transition probability is independent of the nature of the particle. It is observed that the charge of the scalar hairy B and the rotation parameter a control such a probability.