3D grazing collision of two black holes

We present results for two colliding black holes (BHs), with angular momentum, spin, and unequal mass. For the first time, gravitational waveforms are computed for a grazing collision from a full 3D numerical evolution. The collision can be followed through the merger to form a single BH, and throug...

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Published in:Physical review letters 2001-12, Vol.87 (27 Pt 1), p.271103-271103, Article 271103
Main Authors: Alcubierre, M, Benger, W, Brügmann, B, Lanfermann, G, Nerger, L, Seidel, E, Takahashi, R
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cited_by cdi_FETCH-LOGICAL-c354t-a9dcde636906c5b41b0bde00c1da9483720202e5b730aac14e77213aae651d3a3
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container_end_page 271103
container_issue 27 Pt 1
container_start_page 271103
container_title Physical review letters
container_volume 87
creator Alcubierre, M
Benger, W
Brügmann, B
Lanfermann, G
Nerger, L
Seidel, E
Takahashi, R
description We present results for two colliding black holes (BHs), with angular momentum, spin, and unequal mass. For the first time, gravitational waveforms are computed for a grazing collision from a full 3D numerical evolution. The collision can be followed through the merger to form a single BH, and through part of the ringdown period of the final BH. The apparent horizon is tracked and studied, and physical parameters, such as the mass of the final BH, are computed. The total energy radiated in gravitational waves is shown to be consistent with the total initial mass of the spacetime and the apparent horizon mass of the final BH.
doi_str_mv 10.1103/PhysRevLett.87.271103
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title 3D grazing collision of two black holes
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