no code implementations • 22 Dec 2020 • Héctor Estellés, Sascha Husa, Marta Colleoni, David Keitel, Maite Mateu-Lucena, Cecilio García-Quirós, Antoni Ramos-Buades, Angela Borchers
In this work we present an extension of the time domain phenomenological model IMRPhenomT for gravitational wave signals from binary black hole coalescences to include subdominant harmonics, specifically the $(l=2, m=\pm 1)$, $(l=3, m=\pm 3)$, $(l=4, m=\pm 4)$ and $(l=5, m=\pm 5)$ spherical harmonics.
General Relativity and Quantum Cosmology
