redback.transient_models.supernova_models.shock_cooling_and_arnett

redback.transient_models.supernova_models.shock_cooling_and_arnett(time, redshift, log10_mass, log10_radius, log10_energy, f_nickel, mej, **kwargs)[source]
Parameters:

  • time – time in days

  • redshift – source redshift

  • log10_mass – log10 mass of extended material in solar masses

  • log10_radius – log10 radius of extended material in cm

  • log10_energy – log10 energy of extended material in ergs

  • f_nickel – fraction of nickel mass

  • mej – total ejecta mass in solar masses

  • kwargs – Must be all the kwargs required by the specific interaction_process, photosphere, sed methods used e.g., for Diffusion and TemperatureFloor: kappa, kappa_gamma, vej (km/s), temperature_floor

  • nn – density power law slope

  • delta – inner density power law slope

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

  • photosphere – Default is TemperatureFloor. kwargs must have vej or relevant parameters if using different photosphere model

  • sed – Default is blackbody.

  • frequency – Required if output_format is ‘flux_density’. frequency to calculate - Must be same length as time array or a single number).

  • bands – Required if output_format is ‘magnitude’ or ‘flux’.

  • output_format – ‘flux_density’, ‘magnitude’, ‘spectra’, ‘flux’, ‘sncosmo_source’

  • lambda_array – Optional argument to set your desired wavelength array (in Angstroms) to evaluate the SED on.

  • cosmology – Cosmology to use for luminosity distance calculation. Defaults to Planck18. Must be a astropy.cosmology object.

Returns:

set by output format - ‘flux_density’, ‘magnitude’, ‘spectra’, ‘flux’, ‘sncosmo_source’