Hawking effect of non-static Kerr black holes.

Details Hawking effect of non-static Kerr black holes. Hawking effect of non-static Kerr black holes.

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ncimb.113..343z&link_type=abstract

Nuovo Cimento B, Vol. 113B, No. 3, p. 343 - 348

Physics

Black Holes

Scientific paper

Through directly finding the solution of the Klein-Gordon equation near the horizon, the authors obtain the location equation of the event horizon and the Hawking radiation temperature. The results indicate that the event horizon location, the angular velocity and the Hawking radiation temperature of non-static Kerr black holes depend not only on the time, but also on the direction angle.

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