A jet appearing when a black hole event horizon touches the Rindler horizon.

Details A jet appearing when a black hole event horizon touches the Rindler horizon. A jet appearing when a black hole event horizon touches the Rindler horizon.

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ijtp...36.1359z&link_type=abstract

International Journal of Theoretical Physics, Vol. 36, No. 6, p. 1359 - 1368

Physics

1

Black Holes: Hawking Radiation, Black Holes: Jets

Scientific paper

The Hawking effect of a nonuniformly rectilinearly accelerating Kinnersley black hole is studied. Its horizons are rotationally symmetric. Its Hawking temperature depends not only on the time, but also on the polar angle. When a Kinnersley black hole touches its Rindler horizon, the Hawking temperature at the contact point is reduced to zero. But at the opposite pole of the black hole, the Hawking temperature increases rapidly. A jet appears as a tail of the accelerating black hole.

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