Source code for sage.data.waveform.conversions

#!/usr/bin/env python
# -*- coding: utf-8 -*-

"""
Filename        : conversions.py
Description     : Short description of the file

Created on 2026-02-16 16:05:31

__author__        = Narenraju Nagarajan
__copyright__     = Copyright 2026, ProjectName
__license__       = MIT Licence
__version__       = 0.0.1
__maintainer__    = Narenraju Nagarajan
__affiliation__   = N/A
__email__         = N/A
__status__        = ['inProgress', 'Archived', 'inUsage', 'Debugging']


GitHub Repository: NULL

Documentation: NULL

"""

# Packages
import torch


[docs] def mass1_mass2_to_mchirp_q(m1, m2): """ Convert component masses to chirp mass and mass ratio. Parameters ---------- m1 : float or torch.Tensor Primary mass (must be >= m2). m2 : float or torch.Tensor Secondary mass. Returns ------- mchirp : same type as input Chirp mass ``(m1*m2)^(3/5) / (m1+m2)^(1/5)``. q : same type as input Mass ratio ``m1 / m2`` (>= 1 when m1 >= m2). """ q = m1 / m2 mchirp = (m1 * m2) ** (3 / 5) / (m1 + m2) ** (1 / 5) return mchirp, q
[docs] def chirp_distance_to_distance(chirp_distance, mchirp): """ Convert chirp distance to luminosity distance. Uses the standard relation ``d_L = d_chirp * (Mc / 1.2 Msun)^(5/6)`` where 1.2 Msun is the chirp mass of a 1.4+1.4 Msun binary. Parameters ---------- chirp_distance : float or torch.Tensor Chirp distance in Mpc. mchirp : float or torch.Tensor Chirp mass in solar masses. Returns ------- float or torch.Tensor Luminosity distance in Mpc. """ return chirp_distance * (mchirp / 1.2) ** (5 / 6)