Quantum thermal effect of non-stationary Kerr black hole.

Details Quantum thermal effect of non-stationary Kerr black hole. Quantum thermal effect of non-stationary Kerr black hole.

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993acaps..13..299z&link_type=abstract

Acta Astrophys. Sin., Vol. 13, No. 4, p. 299 - 304

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

The event horizon of the non-stationary Kerr black hole is rotationally
symmetric, but not spherically symmetric. It's location, angular
velocity and Hawking temperature depend not only on the time, but also
on the polar angle.

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