Thermal jet of black hole.

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Black Holes: Thermal Properties, Black Holes: Jets

Scientific paper

By means of the null-surface equation, it is found that there exist two horizons for a uniformly accelerating rectilinear non-stationary black hole: black hole horizon and its Rindler horizon. When the two horizons touch each other, the Hawking temperature at the contact point vanishes. But at the opposite pole of the black hole, the Hawking temperature will increase rapidly and a thermal jet will be formed.

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