redback.transient_models.supernova_models.shockcooling_sapirwaxman_and_arnett_bolometric

redback.transient_models.supernova_models.shockcooling_sapirwaxman_and_arnett_bolometric(time, v_shock, m_env, mej, f_rho, f_nickel, radius, kappa, **kwargs)[source]

Assumes Shock cooling following Sapir and Waxman and arnett model for radioactive decay

Parameters:

  • time – time in source frame in days

  • v_shock – shock speed in km/s, also the ejecta velocity in the arnett calculation

  • m_env – envelope mass in solar masses

  • mej – ejecta mass in solar masses

  • f_rho – f_rho. Typically, of order unity

  • f_nickel – fraction of nickel mass

  • radius – star/envelope radius in units of 10^13 cm

  • kappa – opacity in cm^2/g

  • kwargs – Additional parameters required by model

  • n – index of progenitor density profile, 1.5 (default) or 3.0

  • RW – If True, use the simplified Rabinak & Waxman formulation (off by default)

Returns:

bolometric luminosity in erg/s