bilby.gw.source.gwsignal_binary_black_hole
- bilby.gw.source.gwsignal_binary_black_hole(frequency_array, mass_1, mass_2, luminosity_distance, a_1, tilt_1, phi_12, a_2, tilt_2, phi_jl, theta_jn, phase, **kwargs)[source]
A binary black hole waveform model using GWsignal
- Parameters:
- frequency_array: array_like
The frequencies at which we want to calculate the strain
- mass_1: float
The mass of the heavier object in solar masses
- mass_2: float
The mass of the lighter object in solar masses
- luminosity_distance: float
The luminosity distance in megaparsec
- a_1: float
Dimensionless primary spin magnitude
- tilt_1: float
Primary tilt angle
- phi_12: float
Azimuthal angle between the two component spins
- a_2: float
Dimensionless secondary spin magnitude
- tilt_2: float
Secondary tilt angle
- phi_jl: float
Azimuthal angle between the total binary angular momentum and the orbital angular momentum
- theta_jn: float
Angle between the total binary angular momentum and the line of sight
- phase: float
The phase at coalescence
- kwargs: dict
Optional keyword arguments Supported arguments:
waveform_approximant
reference_frequency
minimum_frequency
maximum_frequency
catch_waveform_errors
pn_amplitude_order
mode_array: Activate a specific mode array and evaluate the model using those modes only. e.g. waveform_arguments = dict(waveform_approximant=’IMRPhenomHM’, mode_array=[[2,2],[2,-2]]) returns the 22 and 2-2 modes only of IMRPhenomHM. You can only specify modes that are included in that particular model. e.g. waveform_arguments = dict(waveform_approximant=’IMRPhenomHM’, mode_array=[[2,2],[2,-2],[5,5],[5,-5]]) is not allowed because the 55 modes are not included in this model. Be aware that some models only take positive modes and return the positive and the negative mode together, while others need to call both. e.g. waveform_arguments = dict(waveform_approximant=’IMRPhenomHM’, mode_array=[[2,2],[4,-4]]) returns the 22 and 2-2 of IMRPhenomHM. However, waveform_arguments = dict(waveform_approximant=’IMRPhenomXHM’, mode_array=[[2,2],[4,-4]]) returns the 22 and 4-4 of IMRPhenomXHM.
- Returns:
- dict: A dictionary with the plus and cross polarisation strain modes
Notes
This function is a temporary wrapper to the interface that will likely be significantly changed or removed in a future release. This version is only intended to be used with SEOBNRv5HM and SEOBNRv5PHM and does not have full functionality for other waveform models.