Authors: Victor Demjanenko
A gravitational horizon is expected in the vicinity of moving black holes. Black holes are well understood to have event horizons which capture matter and light. The Kerr solution to the outer event horizon boundary is evidence of the gravitational distortion formed from rotating black holes. Rotating black holes moving relative to each other will also feel effects due to their rotation. A portion of their mass effectively disappears beyond a boundary which is the gravitational horizon.
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[v1] 2021-01-02 12:39:22
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