redback.transient_models.supernova_models.general_magnetar_driven_supernova

redback.transient_models.supernova_models.general_magnetar_driven_supernova(time, redshift, mej, E_sn, kappa, l0, tau_sd, nn, kappa_gamma, **kwargs)[source]
Parameters:

  • time – time in observer frame in days

  • redshift – redshift

  • mej – ejecta mass in solar units

  • E_sn – supernova explosion energy

  • ejecta_radius – initial ejecta radius

  • kappa – opacity

  • n_ism – ism number density

  • l0 – initial magnetar spin-down luminosity (in erg/s)

  • tau_sd – magnetar spin down damping timescale (in seconds)

  • nn – braking index

  • kappa_gamma – gamma-ray opacity used to calculate magnetar thermalisation efficiency

  • kwargs – Additional parameters - 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 and CutoffBlackbody: cutoff_wavelength, default is 3000 Angstrom

  • pair_cascade_switch – whether to account for pair cascade losses, default is False

  • albedo (ejecta) – ejecta albedo; default is 0.5

  • pair_cascade_fraction – fraction of magnetar luminosity lost to pair cascades; default is 0.05

  • output_format – whether to output flux density or AB magnitude

  • frequency – (frequency to calculate - Must be same length as time array or a single number)

  • f_nickel – Ni^56 mass as a fraction of ejecta mass

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

  • sed – Default is CutoffBlackbody.

Returns:

flux density or AB magnitude or dynamics output