ASCL Code Record
[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
Preferred citation method:
https://ui.adsabs.harvard.edu/abs/2016PhRvD..93d4006H and https://ui.adsabs.harvard.edu/abs/2016PhRvD..93d4007K
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