Hawking Radiation of Charged Particles as Tunneling from Higher Dimensional Reissner-Nordstrom-de Sitter Black Holes
arXiv:hep-th/0603082
Abstract
Recent work that treats the Hawking radiation as a semi-classical tunnelling process from the four-dimensional Schwarzschild and Reissner-Nordstrom black holes is extended to the case of higher dimensional Reissner-Nordstrom-de Sitter black holes. The result shows that the tunnelling rate is related to the change of Bekenstein-Hawking entropy and the exact radiant spectrum is no longer precisely thermal after considering the black hole background as dynamical and incorporating the self-gravitation effect of the emitted particles when the energy conservation and electric charge conservation are taken into account.
13 pages, no figure, enlarged version
Cited by in corpus (5)
- Charged Fermions Tunnelling from Kerr-Newman Black Holes
- Tunnelling From Gödel Black Holes
- Hawking Radiation via Tunneling from Hot NUT-Kerr-Newman-Kasuya Spacetime
- Quantum corrections and black hole spectroscopy
- Radiation Spectra and Effective Temperatures in Higher-Dimensional Charged-de Sitter Black Holes