Published February 22, 2022
| Version v1
Journal article
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Numerical-Relativity-Informed Effective-One-Body model for Black-Hole-Neutron-Star Mergers with Higher Modes and Spin Precession
Authors/Creators
- 1. Friedrich Schiller University, Jena
- 2. Dipartimento di Fisica, Universita di Torino
Description
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]
Files
TEOBResumS_BHNS.zip
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(199.9 MB)
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