Laying the foundation of the effective-one-body waveform models SEOBNRv5: Improved accuracy and efficiency for spinning nonprecessing binary black holes

被引：55

作者：

Pompili, Lorenzo ^{[1
]}

Buonanno, Alessandra ^{[1
,2
]}

Estelles, Hector ^{[1
]}

Khalil, Mohammed ^{[1
,2
,3
]}

Meent, Maarten van de ^{[1
,4
]}

Mihaylov, Deyan P. ^{[1
]}

Ossokine, Serguei ^{[1
]}

Puerrer, Michael ^{[1
,5
,6
]}

Ramos-Buades, Antoni ^{[1
]}

Mehta, Ajit Kumar ^{[1
,7
]}

Cotesta, Roberto ^{[8
]}

Marsat, Sylvain ^{[9
]}

Boyle, Michael ^{[10
]}

Kidder, Lawrence E. ^{[10
]}

Pfeiffer, Harald P. ^{[1
,12
]}

Scheel, Mark A. ^{[11
]}

Ruter, Hannes R. ^{[2
]}

Vu, Nils ^{[11
]}

Dudi, Reetika ^{[1
]}

Ma, Sizheng ^{[11
]}

Mitman, Keefe ^{[11
]}

Melchor, Denyz ^{[13
]}

Thomas, Sierra ^{[13
,14
]}

Sanchez, Jennifer ^{[15
]}

机构：

[1] Albert Einstein Inst, Max Planck Inst Grav Phys, Muhlenberg 1, D-14476 Potsdam, Germany

[2] Univ Maryland, Dept Phys, College Pk, MD 20742 USA

[3] Perimeter Inst Theoret Phys, 31 Caroline St North, Waterloo, ON N2L 2Y5, Canada

[4] Niels Bohr Inst, Niels Bohr Int Acad, Blegdamsvej 17, DK-2100 Copenhagen, Denmark

[5] Univ Rhode Isl, Dept Phys, East Hall, Kingston, RI 02881 USA

[6] Univ Rhode Isl, Ctr Computat Res, Tyler Hall, Kingston, RI 02881 USA

[7] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA

[8] Johns Hopkins Univ, William H Miller Dept Phys & Astron 3, 3400 N Charles St, Baltimore, MD 21218 USA

[9] Univ Toulouse, CNRS, UPS, IMRCP,Lab 2 Infinis Toulouse L2IT IN2P3, F-31062 Toulouse 9, France

[10] Cornell Univ, Cornell Ctr Astrophys & Planetary Sci, Ithaca, NY 14853 USA

[11] CALTECH, Theoret Astrophys 350-17, Pasadena, CA 91125 USA

[12] Univ Coimbra, Dept Phys, CFisUC, Coimbra 3004516, Portugal

[13] Calif State Univ Fullerton, Nicholas & Lee Begovich Ctr Gravitat Wave Phys & A, Fullerton, CA 92831 USA

[14] Syracuse Univ, Dept Phys, Syracuse, NY 13244 USA

[15] Northwestern Univ, Ctr Interdisciplinary Explorat & Res Astrophys CIE, 1800 Sherman Ave, Evanston, IL 60201 USA

来源：

PHYSICAL REVIEW D | 2023年 / 108卷 / 12期

基金：

澳大利亚研究理事会; 英国科学技术设施理事会; 新加坡国家研究基金会; 日本学术振兴会; 美国国家科学基金会;

关键词：

Northwestern University; 1800 Sherman Ave; Evanston; Illinois; 60201; USA;

D O I：

10.1103/PhysRevD.108.124035

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present SEOBNRv5HM, a more accurate and faster inspiral-merger-ringdown gravitational waveform model for quasicircular, spinning, nonprecessing binary black holes within the effective-one-body (EOB) formalism. Compared to its predecessor, SEOBNRv4HM, the waveform model (i) incorporates recent high-order post-Newtonian results in the inspiral, with improved resummations, (ii) includes the gravitational modes (l, imi) = (3, 2), (4, 3), in addition to the (2,2), (3,3), (2,1), (4,4), (5,5) modes already implemented in SEOBNRv4HM, (iii) is calibrated to larger mass ratios and spins using a catalog of 442 numerical-relativity (NR) simulations and 13 additional waveforms from black-hole perturbation theory, and (iv) incorporates information from second-order gravitational self-force in the nonspinning modes and radiation-reaction force. Computing the unfaithfulness against NR simulations, we find that for the dominant (2,2) mode the maximum unfaithfulness in the total mass range 10-300M circle dot is below 10-3 for 90% of the cases (38% for SEOBNRv4HM). When including all modes up to l = 5 we find 98% (49%) of the cases with unfaithfulness below 10-2 (10-3), while these numbers reduce to 88% (5%) when using SEOBNRv4HM. Furthermore, the model shows improved agreement with NR in other dynamical quantities (e.g., the angular momentum flux and binding energy), providing a powerful check of its physical robustness. We implemented the waveform model in a high-performance Python package (pySEOBNR), which leads to evaluation times faster than SEOBNRv4HM by a factor of 10 to 50, depending on the configuration, and provides the flexibility to easily include spin-precession and eccentric effects, thus making it the starting point for a new generation of EOBNR waveform models (SEOBNRv5) to be employed for upcoming observing runs of the LIGO-Virgo-KAGRA detectors.

引用

页数：58

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