Catalog of precessing black-hole-binary numerical-relativity simulations

被引:10
|
作者
Hamilton, Eleanor [1 ,2 ]
Fauchon-Jones, Edward [1 ,3 ]
Hannam, Mark [1 ]
Hoy, Charlie [1 ,4 ]
Kalaghatgi, Chinmay [1 ,5 ,6 ,7 ]
London, Lionel [1 ,7 ,8 ,9 ,10 ]
Thompson, Jonathan E. [1 ,11 ]
Yeeles, Dave [1 ,12 ]
Ghosh, Shrobana [1 ]
Khan, Sebastian [1 ]
Kolitsidou, Panagiota [1 ]
Vano-Vinuales, Alex [1 ,2 ,13 ]
机构
[1] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, Wales
[2] Univ Zurich, Phys Inst, Winterthurerstr 190, CH-8057 Zurich, Switzerland
[3] Imperial Coll London, South Kensington Campus, London SW7 2AZ, England
[4] Univ Portsmouth, Portsmouth PO1 3FX, England
[5] Nikhef, Sci Pk 105, NL-1098 XG Amsterdam, Netherlands
[6] Univ Utrecht, Inst Gravitat & Subatom Phys GRASP, Princetonpl 1, NL-3584 CC Utrecht, Netherlands
[7] Univ Amsterdam, Inst High Energy Phys, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands
[8] Kings Coll London, London WC2R 2LS, England
[9] Kavli Inst Astrophys & Space Res, MIT, 77 Massachusetts Ave,37-664H, Cambridge, MA 02139 USA
[10] LIGO Lab, 77 Massachusetts Ave,37-664H, Cambridge, MA 02139 USA
[11] CALTECH, Theoret Astrophys Grp, Pasadena, CA 91125 USA
[12] Acad Sinica, Inst Phys, Taipei 115201, Taiwan
[13] Univ Lisboa UL, Inst Super Tecn IST, Dept Fis, CENTRA, Ave Rovisco Pais 1, P-1049001 Lisbon, Portugal
基金
美国国家科学基金会; 瑞士国家科学基金会; 欧洲研究理事会; 英国科学技术设施理事会;
关键词
GRAVITATIONAL-WAVES; COMPACT BINARIES; FINAL SPIN; COALESCENCE;
D O I
10.1103/PhysRevD.109.044032
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a public catalog of numerical -relativity binary -black -hole simulations. The catalog contains datasets from 80 distinct configurations of precessing binary -black -hole systems, with mass ratios up to m2/m1 = 8, dimensionless spin magnitudes on the larger black hole up to j hole is nonspinning), and a range of five values of spin misalignment for each mass-ratio/spin combination. We discuss the physical properties of the configurations in our catalog, and assess the accuracy of the initial configuration of each simulation and of the gravitational waveforms. We perform a careful analysis of the errors due to the finite resolution of our simulations and the finite distance from the source at which we extract the waveform data and provide a conservative estimate of the mismatch accuracy. We find that the upper limit on the mismatch uncertainty of our waveforms (including multipoles l <= 5) is 0.4%. In doing this we present a consistent approach to combining mismatch uncertainties from multiple error sources. We compare this release to previous catalogs and discuss how these new simulations complement the existing public datasets. In particular, this is the first catalog to uniformly cover this parameter space of single -spin binaries and there was previously only sparse coverage of the precessing-binary parameter space for mass ratios greater than or similar to 5. We discuss applications of these new data, and the most urgent directions for future simulation work.
引用
收藏
页数:29
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