Numerical-relativity-informed effective-one-body model for black-hole–neutron-star mergers with higher modes and spin precession

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 13 Apr 2023Embargo end date: 01 Jan 2022 English Publisher:American Physical Society (APS)Journal:Physical Review D, volume 107 (issn: 2470-0010, eissn: 2470-0029,

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Authors: Gonzalez, Alejandra; Gamba, Rossella; Breschi, Matteo; Zappa, Francesco; Carullo, Gregorio; Bernuzzi, Sebastiano; Nagar, Alessandro;

doi: 10.1103/physrevd.107.084026 , 10.5281/zenodo.6226934 , 10.5281/zenodo.6226935 , 10.48550/arxiv.2212.03909

arXiv: 2212.03909

Numerical-relativity-informed effective-one-body model for black-hole–neutron-star mergers with higher modes and spin precession

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Abstract

We present data release associated to "Numerical-Relativity-Informed Effective-One-Body model for Black-Hole-Neutron-Star Mergers with Higher Modes and Spin Precession" [1]. The BHNS model in this work is implemented and publicly available in TEOBResumS. The analysis of both artificial and real GW data was performed with bajes [2]. [1] A. Gonzalez et al., Numerical-Relativity-Informed Effective-One-Body model for Black-Hole-Neutron-Star Mergers with Higher Modes and Spin Precession, arXiv:2212.03909 [gr-qc] [2] M.Breschi et. al., Bayesian inference of multimessenger astrophysical data: Methods and applications to gravitational waves, Phys. Rev. D 104 (2021) no.4, 042001, doi:10.1103/PhysRevD.104.042001, arXiv:2102.00017 [gr-qc]

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Keywords

waveform, bhns, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), eob, GW, General Relativity and Quantum Cosmology

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