Quantum tunneling from rotating black holes with scalar hair in three dimensions
General Relativity and Quantum Cosmology
2016-10-24 v1
Abstract
We study the Hawking radiation (HR) of scalar and Dirac particles (fermions) emitted from a rotating scalar hair black hole (RSHBH) within the context of three dimensional () Einstein gravity using non-minimally coupled scalar field theory. Amalgamating the quantum tunneling approach with the Wentzel--Kramers--Brillouin (WKB) approximation, we obtain the tunneling rates of the outgoing particles across the event horizon. Inserting the resultant tunneling rates into the Boltzmann formula, we then obtain the Hawking temperature () of the RSHBH.
Keywords
Cite
@article{arxiv.1505.01990,
title = {Quantum tunneling from rotating black holes with scalar hair in three dimensions},
author = {I. Sakalli and H. Gursel},
journal= {arXiv preprint arXiv:1505.01990},
year = {2016}
}