inspiral-range 0.4.1

GW detector inspiral range calculation tools

GW detector inspiral range calculation tools

The inspiral_range package provides tools for calculating various binary inspiral range measures useful as figures of merit for gravitational wave detectors characterized by a strain noise spectral density.

It includes a command-line tool for calculating various inspiral ranges from a supplied file of detector noise spectral density (either ASD or PSD).

See the following references for more information:

• https://arxiv.org/abs/1709.08079
• https://dcc.ligo.org/LIGO-T1500491
• https://dcc.ligo.org/LIGO-T1100338
• https://dcc.ligo.org/LIGO-T030276

Authors:

• Jameson Rollins [e-mail]
• Jolien Creighton [e-mail]

Installation

inspiral_range is available via pip and conda.

$ pip install inspiral_range

inspiral_range depends on scipy for various optimization routines, and astropy for cosmology calculations. The LSC Algorithm Library (LAL) can also be used for faster versions of some calculations. The LAL dependencies (both lal and lalsimulation) can be found in the lalsuite package in pip or conda, or in native packaging available for various supported IGWN supported operating systems. Use the lal extra flag during pip installation to pull in the LAL dependencies:

$ pip install inspiral_range[lal]

Note the following caveats:

cosmology

inspiral_range needs to calculate luminosity distance and differential comoving volume as a function of redshift, which requires specifying a cosmology model. Two different packages are supported for these cosmological calculations:

• astropy (default): pure python and widely available, but slow
• lal: not pure python so not as accessible, but much faster

waveform generation

inspiral_range needs the amplitude of strain waveforms of binary inspiral signals in order to calculate the detection SNR for a given detector noise spectrum. Included in the package is a cached interpolant for equal mass, non-spinning BBH systems. For range calculations for other systems (non-equal masses, including spin) the lalsimulation package is required for waveform calculations.

Usage

library usage

The package includes multiple functions for calculating various range measures for a given PSD.

Analytical methods:

• sensemon_range
• sensemon_horizon
• int73

Cosmologically-corrected measures (see arxiv:1709.08079):

• horizon (Mpc)
• horizon_redshift (z)
• volume (Mpc^3)
• range (Mpc)
• response_frac (Mpc)
• response_frac_redshift (z)
• reach_frac (Mpc)
• reach_frac_redshift (z)

By default, all functions calculate measures for 1.4/1.4 M_sol BNS inspirals:

>>> import inspiral_range
>>> freq, psd = np.loadtxt('PSD.txt')
>>> range_bns = inspiral_range.range(freq, psd)

But other masses can be used as well:

>>> range_bbh = inspiral_range.range(freq, psd, m1=30, m2=30)

When calculating multiple measures together it is more efficient to generate the fiducial waveform first and then pass it to the various functions:

>>> H = inspiral_range.CBCWaveform(freq, m1=30, m2=30)
>>> horizon = inspiral_range.horizon(freq, psd, H=H)
>>> range = inspiral_range.range(freq, psd, H=H)

The cosmology being used can be modified with the Cosmology class:

>>> cosmo = inspiral_range.Cosmology(h=70.0)
>>> H = inspiral_range.CBCWaveform(freq, cosmo=cosmo)

The 'cosmo' parameter can also be supplied directly to the range calculator:

>>> range = inspiral_range.range(freq, psd, cosmo=cosmo)

A convenience function all_ranges is included that calculates most of the range metrics together in an efficient way (all return values in Mpc):

• range
• horizon
• response_50
• response_10
• reach_50
• reach_90
• sensemon_range
• sensemon_horizon

e.g.:

>>> metrics, H = inspiral_range.all_ranges(freq, psd)

command line interface

The package also include a command line interface for easily calculating ranges for a given ASD or PSD specified in a two-column text file:

$ python3 -m inspiral_range -p PSD.txt m1=30 m2=30