redback.transient_models.supernova_models.csm_interaction_bolometric

redback.transient_models.supernova_models.csm_interaction_bolometric(time, mej, csm_mass, vej, eta, rho, kappa, r0, **kwargs)[source]
Parameters:

  • time – time in days in source frame

  • mej – ejecta mass in solar masses

  • csm_mass – csm mass in solar masses

  • vej – ejecta velocity in km/s

  • eta – csm density profile exponent

  • rho – csm density profile amplitude

  • kappa – opacity

  • r0 – radius of csm shell in AU

  • kwargs –

    Additional keyword arguments: efficiency: in converting between kinetic energy and luminosity, default 0.5 delta: default 1, nn: default 12, dense_resolution: resolution of dense engine time array, default 1000 dense_time_min: minimum dense engine time in days, default min(0.1, min(time)) stop_time: maximum dense engine time in days, default max(time) + 100 csm_diffusion_method: CSM diffusion integral method. Default is “cumulative”.

    Use “quadrature” for the legacy per-time integral.

    If interaction process is different kwargs must include other keyword arguments that are required.

  • interaction_process – Default is CSMDiffusion. Can also be None in which case the output is just the raw engine luminosity, or another interaction process.

Returns:

bolometric_luminosity