Catalog of 174 Binary Black Hole Simulations for Gravitational Wave Astronomy
This Letter presents a publicly available catalog of 174 numerical binary black hole simulations following up to 35 orbits. The catalog includes 91 precessing binaries, mass ratios up to 8:1, orbital eccentricities from a few percent to 10^(-5), black hole spins up to 98% of the theoretical maximum,...
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ftcaltechauth:oai:authors.library.caltech.edu:2kzkg-1qn50 2024-09-15T18:29:00+00:00 Catalog of 174 Binary Black Hole Simulations for Gravitational Wave Astronomy Mroué, Abdul H. Scheel, Mark A. Szilágyi, Béla Pfeiffer, Harald P. Boyle, Michael Hemberger, Daniel A. Kidder, Lawrence E. Lovelace, Geoffrey Ossokine, Serguei Taylor, Nicholas W. Zenginoğlu, Anıl Buchman, Luisa T. Chu, Tony Foley, Evan Giesler, Matthew Owen, Robert Teukolsky, Saul A. 2013-12-11 https://doi.org/10.1103/PhysRevLett.111.241104 unknown American Physical Society http://arxiv.org/abs/1304.6077v3 https://doi.org/10.1103/PhysRevLett.111.241104 oai:authors.library.caltech.edu:2kzkg-1qn50 eprintid:43588 resolverid:CaltechAUTHORS:20140130-135558192 info:eu-repo/semantics/openAccess Other Physical Review Letters, 111(24), Article No. 241104, (2013-12-11) info:eu-repo/semantics/article 2013 ftcaltechauth https://doi.org/10.1103/PhysRevLett.111.241104 2024-08-06T15:35:05Z This Letter presents a publicly available catalog of 174 numerical binary black hole simulations following up to 35 orbits. The catalog includes 91 precessing binaries, mass ratios up to 8:1, orbital eccentricities from a few percent to 10^(-5), black hole spins up to 98% of the theoretical maximum, and radiated energies up to 11.1% of the initial mass. We establish remarkably good agreement with post-Newtonian precession of orbital and spin directions for two new precessing simulations, and we discuss other applications of this catalog. Formidable challenges remain: e.g., precession complicates the connection of numerical and approximate analytical waveforms, and vast regions of the parameter space remain unexplored. © 2013 American Physical Society. Received 27 May 2013; revised 5 September 2013; published 11 December 2013. We thank Christian Ott and Kip Thorne for helpful discussions. This work was supported in part by NSERC of Canada, the Canada Chairs Program, and the Canadian Institute for Advanced Research; the Sherman Fairchild Foundation; and NSF Grants No. PHY-0969111 and No. PHY-1005426 at Cornell, NSF Grants No. PHY-1068881, No. PHY-1005655, and No. DMS-1065438 at Caltech, and NSF Grant No. PHY-1307489 at Cal State Fullerton. Simulations used in this work were computed with the SpEC code [27]. Computations were performed on the Zwicky cluster at Caltech, which is supported by the Sherman Fairchild Foundation and by NSF Grant No. PHY-0960291; on the NSF XSEDE network under Grant No. TG-PHY990007N; on the Orca Cluster supported by Cal State Fullerton; and on the GPC Supercomputer at the SciNet HPC Consortium [78]. SciNet is funded by the Canada Foundation for Innovation under the auspices of Compute Canada, the Government of Ontario, Ontario Research Fund—Research Excellence, and the University of Toronto. Published - PhysRevLett.111.241104.pdf Submitted - 1304.6077v3.pdf Article in Journal/Newspaper Orca Caltech Authors (California Institute of Technology) Physical Review Letters 111 24 |
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This Letter presents a publicly available catalog of 174 numerical binary black hole simulations following up to 35 orbits. The catalog includes 91 precessing binaries, mass ratios up to 8:1, orbital eccentricities from a few percent to 10^(-5), black hole spins up to 98% of the theoretical maximum, and radiated energies up to 11.1% of the initial mass. We establish remarkably good agreement with post-Newtonian precession of orbital and spin directions for two new precessing simulations, and we discuss other applications of this catalog. Formidable challenges remain: e.g., precession complicates the connection of numerical and approximate analytical waveforms, and vast regions of the parameter space remain unexplored. © 2013 American Physical Society. Received 27 May 2013; revised 5 September 2013; published 11 December 2013. We thank Christian Ott and Kip Thorne for helpful discussions. This work was supported in part by NSERC of Canada, the Canada Chairs Program, and the Canadian Institute for Advanced Research; the Sherman Fairchild Foundation; and NSF Grants No. PHY-0969111 and No. PHY-1005426 at Cornell, NSF Grants No. PHY-1068881, No. PHY-1005655, and No. DMS-1065438 at Caltech, and NSF Grant No. PHY-1307489 at Cal State Fullerton. Simulations used in this work were computed with the SpEC code [27]. Computations were performed on the Zwicky cluster at Caltech, which is supported by the Sherman Fairchild Foundation and by NSF Grant No. PHY-0960291; on the NSF XSEDE network under Grant No. TG-PHY990007N; on the Orca Cluster supported by Cal State Fullerton; and on the GPC Supercomputer at the SciNet HPC Consortium [78]. SciNet is funded by the Canada Foundation for Innovation under the auspices of Compute Canada, the Government of Ontario, Ontario Research Fund—Research Excellence, and the University of Toronto. Published - PhysRevLett.111.241104.pdf Submitted - 1304.6077v3.pdf |
format |
Article in Journal/Newspaper |
author |
Mroué, Abdul H. Scheel, Mark A. Szilágyi, Béla Pfeiffer, Harald P. Boyle, Michael Hemberger, Daniel A. Kidder, Lawrence E. Lovelace, Geoffrey Ossokine, Serguei Taylor, Nicholas W. Zenginoğlu, Anıl Buchman, Luisa T. Chu, Tony Foley, Evan Giesler, Matthew Owen, Robert Teukolsky, Saul A. |
spellingShingle |
Mroué, Abdul H. Scheel, Mark A. Szilágyi, Béla Pfeiffer, Harald P. Boyle, Michael Hemberger, Daniel A. Kidder, Lawrence E. Lovelace, Geoffrey Ossokine, Serguei Taylor, Nicholas W. Zenginoğlu, Anıl Buchman, Luisa T. Chu, Tony Foley, Evan Giesler, Matthew Owen, Robert Teukolsky, Saul A. Catalog of 174 Binary Black Hole Simulations for Gravitational Wave Astronomy |
author_facet |
Mroué, Abdul H. Scheel, Mark A. Szilágyi, Béla Pfeiffer, Harald P. Boyle, Michael Hemberger, Daniel A. Kidder, Lawrence E. Lovelace, Geoffrey Ossokine, Serguei Taylor, Nicholas W. Zenginoğlu, Anıl Buchman, Luisa T. Chu, Tony Foley, Evan Giesler, Matthew Owen, Robert Teukolsky, Saul A. |
author_sort |
Mroué, Abdul H. |
title |
Catalog of 174 Binary Black Hole Simulations for Gravitational Wave Astronomy |
title_short |
Catalog of 174 Binary Black Hole Simulations for Gravitational Wave Astronomy |
title_full |
Catalog of 174 Binary Black Hole Simulations for Gravitational Wave Astronomy |
title_fullStr |
Catalog of 174 Binary Black Hole Simulations for Gravitational Wave Astronomy |
title_full_unstemmed |
Catalog of 174 Binary Black Hole Simulations for Gravitational Wave Astronomy |
title_sort |
catalog of 174 binary black hole simulations for gravitational wave astronomy |
publisher |
American Physical Society |
publishDate |
2013 |
url |
https://doi.org/10.1103/PhysRevLett.111.241104 |
genre |
Orca |
genre_facet |
Orca |
op_source |
Physical Review Letters, 111(24), Article No. 241104, (2013-12-11) |
op_relation |
http://arxiv.org/abs/1304.6077v3 https://doi.org/10.1103/PhysRevLett.111.241104 oai:authors.library.caltech.edu:2kzkg-1qn50 eprintid:43588 resolverid:CaltechAUTHORS:20140130-135558192 |
op_rights |
info:eu-repo/semantics/openAccess Other |
op_doi |
https://doi.org/10.1103/PhysRevLett.111.241104 |
container_title |
Physical Review Letters |
container_volume |
111 |
container_issue |
24 |
_version_ |
1810470421005336576 |