CCRG Movies 2007
Fly Through Movies 2007
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Kick
The camera postion is just slightly hovering over each black hole looking at the other black hole. Two black holes in a binary (both with large spin) inspiral towards each other and merge. The merged black hole is kicked (recoils) along the z axis.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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Kick
The camera postion is just slightly hovering over each black hole looking at the other black hole. Two black holes in a binary (both with large spin) inspiral towards each other and merge. The merged black hole is kicked (recoils) along the z axis.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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102: Three Black Hole Merger
The camera postion is just slightly hovering over the black hole of the bottom right corner and is looking at the center of the space. The interaction of a black-hole binary and a third black hole (all black holes have the same masses) produces very interesting trajectories prior to merging. Two distinct mergers are apparent.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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102: Three Black Hole Merger Without Tracing of the History
The camera postion is just slightly hovering over the black hole of the bottom right corner and is looking at the center of the space. The interaction of a black-hole binary and a third black hole (all black holes have the same masses) produces very interesting trajectories prior to merging. Two distinct mergers are apparent.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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Movies with fixed Camera Postion 2007
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101: Three Black Hole Merger
The interaction of a black-hole binary and a third black hole (all black holes have the same masses) produces very interesting trajectories prior to merging. Two distinct mergers are apparent.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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102: Three Black Hole Merger
The interaction of a black-hole binary and a third black hole (all black holes have the same masses) produces very interesting trajectories prior to merging. Two distinct mergers are apparent.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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103: Three Black Hole Merger
Here a black-hole binary interacts with a third black hole perpendicular to its orbital plane. All three black holes merge at nearly the same time.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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Kick
Two black holes in a binary (both with large spin) inspiral towards each other and merge. The merged black hole is kicked (recoils) along the z axis.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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Kick - Z Position = 0
Two black holes in a binary (both with large spin) inspiral towards each other and merge. The merged black hole is kicked (recoils) along the z axis. The view is in the Z axis = 0.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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101: Three Black Hole Merger Without Tracing of the History
The interaction of a black-hole binary and a third black hole (all black holes have the same masses) produces very interesting trajectories prior to merging. Two distinct mergers are apparent.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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102: Three Black Hole Merger Without Tracing of the History
The interaction of a black-hole binary and a third black hole (all black holes have the same masses) produces very interesting trajectories prior to merging. Two distinct mergers are apparent.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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103: Three Black Hole Merger Without Tracing of the History
Here a black-hole binary interacts with a third black hole perpendicular to its orbital plane. All three black holes merge at nearly the same time
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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Kick Without Tracing of the History
Two black holes in a binary (both with large spin) inspiral towards each other and merge. The merged black hole is kicked (recoils) along the z axis. |
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Kick - Z Position = 0
Two black holes in a binary (both with large spin) inspiral towards each other and merge. The merged black hole is kicked (recoils) along the z axis. The view is in the Z axis = 0.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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Gravity Waves
A visualization of the gravitational radiation released by a black-hole binary merger.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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Gravity Waves
A visualization of the gravitational radiation released by a black-hole binary merger.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
mov avi mp4 mov quality is better, sorry
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Gravity Waves
A visualization of the gravitational radiation released by a black-hole binary merger.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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Gravity Waves
A visualization of the gravitational radiation released by a black-hole binary merger.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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Gravity Waves
A visualization of the gravitational radiation released by a black-hole binary merger.
Simulation: Manuela Campanelli, Lousto Carlos, and Yosef Zlochower
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Colliding Galaxies
A visualization of the two colliding galaxies.
Simulation: David Merritt
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