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[ascl:2307.019] IMRPhenomD: Phenomenological waveform model

The IMRPhenomD model generates gravitational wave signals for merging black hole binaries with non-precessing spins. The waveforms are produced in the frequency domain and include the inspiral, merger and ringdown parts for the dominant spherical harmonic mode of the signal. Part of LALSuite (ascl:2012.021) and also available as an independent code, IMRPhenomD is written in C and is calibrated against data from numerical relativity simulations. A re-implementation of IMRPhenomD in Python, PyIMRPhenomD (ascl:2307.023), is available.

Code site:
https://github.com/eXtremeGravityInstitute/LISA-Massive-Black-Hole/blob/main/IMRPhenomD.c https://git.ligo.org/lscsoft/lalsuite/-/blob/master/lalsimulation/lib/LALSimIMRPhenomD.c
Used in:
https://ui.adsabs.harvard.edu/abs/2016PhRvD..93h4042P
Described in:
https://ui.adsabs.harvard.edu/abs/2016PhRvD..93d4006H https://ui.adsabs.harvard.edu/abs/2016PhRvD..93d4007K
Bibcode:
2023ascl.soft07019P

Views: 701

ascl:2307.019
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