redback.transient_models.magnetar_driven_ejecta_models.trapped_magnetar

redback.transient_models.magnetar_driven_ejecta_models.trapped_magnetar(time, redshift, mej, beta, ejecta_radius, kappa, n_ism, l0, tau_sd, nn, thermalisation_efficiency, **kwargs)[source]
Parameters:

  • time – time in source frame or observer frame depending on output format in seconds

  • redshift – redshift - not used if evaluating luminosity

  • mej – ejecta mass in solar units

  • beta – initial ejecta velocity

  • ejecta_radius – initial ejecta radius

  • kappa – opacity

  • n_ism – ism number density

  • l0 – initial magnetar X-ray luminosity

  • tau_sd – magnetar spin down damping timescale

  • nn – braking index

  • thermalisation_efficiency – magnetar thermalisation efficiency

  • kwargs – ‘output_format’ - whether to output luminosity or flux

  • kwargs – ‘frequency’ in Hertz to evaluate the mergernova emission - use a typical X-ray frequency

  • kwargs – ‘photon_index’ only used if calculating the flux lightcurve

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

Returns:

luminosity or integrated flux