Journal
PHYSICAL REVIEW D
Volume 102, Issue 6, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.102.064002
Keywords
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Funding
- European Union FEDER funds
- Ministry of Science, Innovation and Universities
- Spanish Agencia Estatal de Investigacion [FPA2016-76821-P, RED2018-102661-T, RED2018-102573-E, FPA2017-90687REDC]
- Vicepresid'encia i Conselleria d'Innovacio, Recerca i Turisme, Conselleria d'Educacio, i Universitats del Govern de les Illes Balears i Fons Social Europeu, Generalitat Valenciana [PROMETEO/2019/071]
- EU COST Actions [CA18108, CA17137, CA16214, CA16104]
- Spanish Ministry of Education, Culture and Sport [FPU15/03344, FPU15/01319]
- European Union's Horizon 2020 research and innovation programme, under the Marie Sklodowska-Curie Grant [751492]
- Barcelona Supercomputing Center (BSC) from the Red Espanola de Supercomputacion (RES) [AECT-2019-2-0010, AECT-2019-1-0022, AECT-2019-1-0014, AECT-2018-3-0017, AECT-2018-2-0022, AECT-2018-1-0009, AECT-2017-3-0013, AECT-2017-2-0017, AECT-2017-1-0017, AECT-2016-3-0014, AECT2016-2-0009]
- PRACE [2015133131]
- National Science Foundation [PHY-0757058, PHY-0823459]
- U.S. National Science Foundation
- French Centre National de Recherche Scientifique (CNRS)
- Italian Istituto Nazionale della Fisica Nucleare (INFN)
- Dutch Nikhef
- Polish institute
- Hungarian institute
- Marie Curie Actions (MSCA) [751492] Funding Source: Marie Curie Actions (MSCA)
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We present the IMRPHENOMXHM frequency domain phenomenological waveform model for the inspiral, merger, and ringdown of quasicircular nonprecessing black hole binaries. The model extends the IMRPHENOMXAS waveform model [G. Pratten, S. Husa, C. Garcia-Quiros, M. Colleoni, A. Ramos-Buades, H. Estelles, and R. Jaume, preceding paper, Phys. Rev. D 102, 064001 (2020)], which describes the dominant quadrupole modes l = vertical bar m vertical bar = 2, to the harmonics (l vertical bar m vertical bar) = (2, 1), (3, 3), (3, 2), (4,4), and includes mode mixing effects for the (3,2) spherical harmonic. IMRPHENOMXHM is calibrated against hybrid waveforms, which match an inspiral phase described by the effective-one-body model and post-Newtonian amplitudes for the subdominant harmonics to numerical relativity waveforms and numerical solutions to the perturbative Teukolsky equation for large mass ratios up to 1000.
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