A jet appearing when a black hole event horizon touches the rindler horizon |
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Authors: | Zhao Zheng Zhang Jian-hua Jiang Ya-ling |
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Institution: | (1) Department of Physics, Beijing Normal University, 100875 Beijing, China;(2) Department of Physics, Heze Education College, 274016 Shandong Heze, China;(3) Department of Physics, Xiangyang Teachers College, 441053 Hubei Xiangfan, China |
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Abstract: | 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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