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- W3119306186 abstract "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." @default.
- W3119306186 created "2021-01-18" @default.
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- W3119306186 date "2021-01-01" @default.
- W3119306186 modified "2023-09-23" @default.
- W3119306186 title "Gravitational Event Horizon" @default.
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