Catalog of 174 Binary Black Hole Simulations for Gravitational Wave Astronomy

被引:242
|
作者
Mroue, Abdul H. [1 ]
Scheel, Mark A. [2 ]
Szilagyi, Bela [2 ]
Pfeiffer, Harald P. [1 ,3 ]
Boyle, Michael [4 ]
Hemberger, Daniel A. [2 ,4 ]
Kidder, Lawrence E. [4 ]
Lovelace, Geoffrey [2 ,5 ]
Ossokine, Serguei [1 ,6 ]
Taylor, Nicholas W. [2 ]
Zenginoglu, Anil [2 ]
Buchman, Luisa T. [2 ]
Chu, Tony [1 ]
Foley, Evan [5 ]
Giesler, Matthew [5 ]
Owen, Robert [7 ]
Teukolsky, Saul A. [4 ]
机构
[1] Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada
[2] CALTECH, Pasadena, CA 91125 USA
[3] Canadian Inst Adv Res, Toronto, ON M5G 1Z8, Canada
[4] Cornell Univ, Ctr Radiophys & Space Res, Ithaca, NY 14853 USA
[5] Calif State Univ Fullerton, Gravitat Wave Phys & Astron Ctr, Fullerton, CA 92834 USA
[6] Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 3H4, Canada
[7] Oberlin Coll, Dept Phys & Astron, Oberlin, OH 44074 USA
基金
美国国家科学基金会; 加拿大自然科学与工程研究理事会; 加拿大创新基金会;
关键词
NUMERICAL RELATIVITY; EINSTEIN EQUATIONS; RADIATION; SPIN;
D O I
10.1103/PhysRevLett.111.241104
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
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.
引用
收藏
页数:6
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