Thermal properties of a uniformly accelerating rectilinear stationary Kerr black hole.

Details Thermal properties of a uniformly accelerating rectilinear stationary Kerr black hole. Thermal properties of a uniformly accelerating rectilinear stationary Kerr black hole.

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999jbnun..35...54c&link_type=abstract

Journal of Beijing Normal University (Natural Sciences), Vol. 35, No. 1, p. 54 - 57

Physics

Kerr Black Holes: Thermal Properties

Scientific paper

Thermal properties of a uniformly accelerating rectilinear stationary Kerr black hole are studied. It is discovered that both the Unruh temperature of the Rindler horizon and the Hawking temperature of the event horizon are no longer constant. They are functions depending on θ. Furthermore, the temperature of every point on the black hole surface can be obtained. When the event horizon collides with the Rindler horizon, the temperature at the contact point will reduce to zero. But, at the opposite pole of the event horizon of black hole, the Hawking temperature will increase.

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