We study the Hawking radiation of the Kerr-Newman-dS black hole on its event horizon and cosmological horizon from the tunneling approach of Parikh and Wilczek. In order to eliminate the motion on the rotating degree of freedom of a tunneling particle coming from the rotation of the Kerr-Newman-dS black hole, we choose a reference system that is co-rotating with the black hole horizon. Using such a method, we can derive the Hawking temperature of a general rotating black hole from the tunneling approach clearly. Then, to use the general result to the Kerr-Newman-dS case, we reproduce the Hawking temperatures of the Kerr-Newman-dS black hole on its event horizon and cosmological horizon from the tunneling approach.
%0 Journal Article
%1 citeulike:4027214
%A Ma, Zheng Z.
%D 2009
%J Classical and Quantum Gravity
%K black-holes, hawking-temperature, kerr-newmann, tunneling
%N 4
%P 045002+
%R http://dx.doi.org/10.1088/0264-9381/26/4/045002
%T Hawking temperature of a Kerr–Newman–dS black hole from tunneling
%U http://dx.doi.org/10.1088/0264-9381/26/4/045002
%V 26
%X We study the Hawking radiation of the Kerr-Newman-dS black hole on its event horizon and cosmological horizon from the tunneling approach of Parikh and Wilczek. In order to eliminate the motion on the rotating degree of freedom of a tunneling particle coming from the rotation of the Kerr-Newman-dS black hole, we choose a reference system that is co-rotating with the black hole horizon. Using such a method, we can derive the Hawking temperature of a general rotating black hole from the tunneling approach clearly. Then, to use the general result to the Kerr-Newman-dS case, we reproduce the Hawking temperatures of the Kerr-Newman-dS black hole on its event horizon and cosmological horizon from the tunneling approach.
@article{citeulike:4027214,
abstract = {We study the Hawking radiation of the Kerr-Newman-dS black hole on its event horizon and cosmological horizon from the tunneling approach of Parikh and Wilczek. In order to eliminate the motion on the rotating degree of freedom of a tunneling particle coming from the rotation of the Kerr-Newman-dS black hole, we choose a reference system that is co-rotating with the black hole horizon. Using such a method, we can derive the Hawking temperature of a general rotating black hole from the tunneling approach clearly. Then, to use the general result to the Kerr-Newman-dS case, we reproduce the Hawking temperatures of the Kerr-Newman-dS black hole on its event horizon and cosmological horizon from the tunneling approach.},
added-at = {2009-02-18T14:54:47.000+0100},
author = {Ma, Zheng Z.},
biburl = {https://www.bibsonomy.org/bibtex/2f3a7a036149cedc65d77aa077d316614/janpaniev},
citeulike-article-id = {4027214},
doi = {http://dx.doi.org/10.1088/0264-9381/26/4/045002},
interhash = {377214801a15a05552e4ff214c635ab9},
intrahash = {f3a7a036149cedc65d77aa077d316614},
journal = {Classical and Quantum Gravity},
keywords = {black-holes, hawking-temperature, kerr-newmann, tunneling},
number = 4,
pages = {045002+},
posted-at = {2009-02-10 00:15:28},
priority = {2},
timestamp = {2009-02-18T14:54:49.000+0100},
title = {Hawking temperature of a Kerr\–Newman\–dS black hole from tunneling},
url = {http://dx.doi.org/10.1088/0264-9381/26/4/045002},
volume = 26,
year = 2009
}