Hawking effect of some axially symmetric non-stationary black holes.

Details Hawking effect of some axially symmetric non-stationary black holes. Hawking effect of some axially symmetric non-stationary black holes.

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ncimb.109..483z&link_type=abstract

Nuovo Cimento B, Vol. 109, No. 5, p. 483 - 491

Physics

5

Black Holes: Hawking Radiation

Scientific paper

The Hawking effects of the non-stationary Kerr black hole and the
non-uniformly rectilinearly accelerating Kinnersley black hole are
researched. Their event horizons are rotationally symmetric, but not
spherically symmetric. Their Hawking temperature not only depends on
time, but also on the polar angles.

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