redback.transient_models.supernova_models.nickelmixing_bolometric

redback.transient_models.supernova_models.nickelmixing_bolometric(time, mej, esn, kappa, kappa_gamma, f_nickel, f_mixing, temperature_floor, **kwargs)[source]

A model for the bolometric light curve of a supernova with nickel mixing

Parameters:

  • time – time in source frame in days

  • mej – ejecta mass in solar masses

  • esn – energy of explosion in foe

  • kappa – gray opacity

  • kappa_gamma – gamma-ray opacity

  • f_nickel – fraction of nickel mass

  • f_mixing – fraction of nickel mass that is mixed, a low value puts all the nickel in the first shell.

  • kwargs – bolometric luminosity in erg/s

  • beta – power law slope for mass distribution; m = m_0 * (v/v_min)^(-beta)

  • stop_time – time to stop ODE at, default is 300 days

  • mass_len – number of mass shells, defaults to 200

  • vmax – maximum velocity in km/s, defaults to 100000

  • dense_resolution – resolution of dense time array, default is 1000

Returns:

bolometric luminosity