mcfacts.physics

Underlying methods used to create and/or evolve physical systems in McFACTS simulations.

Modules

accretion	Module for calculating change of mass, spin magnitude, and spin angle due to accretion.
analytical_velocity	Module for calculating the recoil (kick) velocity of a remnant BH.
binary	Module for handling the evolution, formation, and merging of binaries.
disk_capture_stars
dynamics	Module for handling dynamical interactions.
eccentricity	Module for calculating the orbital and binary eccentricity damping.
emri	Module for EMRI specific calculations.
feedback	Module for calculating corrections to migration due to feedback models.
gw	Module for calculating the gw strain and freq of a binary.
lum	Module for calculating bolometric luminosities from a merger remnant interacting with gas via shocks or jets.
migration	Module for calculating the timescale of migrations.
point_masses	Module for handling simple GR orbital evolution (Peters 1964)
star_interactions	Module for calculating the final variables of two merging stars.
stellar_interpolation	Module for interpolating stellar radius, luminosity, and effective temperature from a grid.
tde	Module for TDE specific calculations.