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On Hawking Radiation of 3D Rotating Hairy Black Holes |
| Belhaj A.1,2**, Chabab M.2, El Moumni H.2, Masmar K.2, Sedra M. B.3 |
1Département de Physique, Faculté Polydisciplinaire, Université Sultan Moulay Slimane, Béni Mellal, Morocco
2High Energy Physics and Astrophysics Laboratory, FSSM, Cadi Ayyad University, Marrakesh, Morocco
3Département de Physique, LHESIR, Faculté des Sciences, Université Ibn Tofail, Kénitra, Morocco
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| Cite this article: |
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Belhaj A., Chabab M., El Moumni H. et al 2015 Chin. Phys. Lett. 32 100401 |
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Abstract 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.
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Received: 10 April 2015
Published: 30 October 2015
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| PACS: |
04.50.-h
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(Higher-dimensional gravity and other theories of gravity)
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04.70.-s
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(Physics of black holes)
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04.70.Dy
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(Quantum aspects of black holes, evaporation, thermodynamics)
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