User guide
Waveforms
Parameter distributions
Data Challenges
Tutorials
Development guide
Minke is capable of producing signals which are based on waveforms based on Binary Black Hole (BBH) ringdowns.
Ringdown-like signals, with a sudden rise, and exponential decay in amplitude are expected in the post-merger signal of CBC systems, and in some models of neutron star model excitation [2004PhRvD..70l4015B].
These take the form
for a strain \(h\) at time \(t\), given a decay time \(\tau\) and frequency \(f\).
The BBH Ringdown class in the sources module follows a similar style to other source classes within minke. To produce a single ringdown waveform:
>>> import minke.sources
>>> bbh = minke.sources.BBHRingdown(100.23, 1e-22, np.rad2deg(.1), 10., 0.97, 0.01, 1.0,45.)
then the waveforms themselves can be produced by running
>>> hp, hx, _, _ = bbh._generate()
The waveform will be generated at the LIGO sampling rate (16384 Hz) by default, but this can be changed by specifying a rate keyword. The waveforms are also generated for the (2,2) mode by default, but by adding l and m keywords to the _generate() method this can also be changed.
minke.sources.
BBHRingdown
(time, phi0, mass, spin, massloss, distance, inclination, sky_dist=<function uniform_sky>)[source]¶A class to represent BBH ringdowns.
Methods
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Generate a “low frequency tail” to append to the end of the waveform to overcome problems related to memory in the waveform. |
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Convenience funtion to avoid repeated code |
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Convert a string description of a polarisation to an ellipse eccentricity and an ellipse angle. |
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Produce a plot of the injection. |
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alias of |