Hawking temperature of a Kerr Newman dS black hole from tunneling

Mathematics – Logic

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Scientific paper

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.

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