redback.transient_models.general_synchrotron_models.synchrotron_pldensity

redback.transient_models.general_synchrotron_models.synchrotron_pldensity(time, redshift, v_s, logA, s, logepsb, logepse, p, **kwargs)[source]
Parameters:

  • time – time in observer frame in days

  • redshift – redshift

  • v_s – velocity of the shock (km/s)

  • logA – log10 of the circumstellar material density at R=1e15 cm (cm^-3)

  • s – power law index of the circumstellar material density profile

  • logepse – log10 epsilon_e; electron thermalisation efficiency

  • logepsb – log10 epsilon_b; magnetic field amplification efficiency

  • p – electron power law slope

  • kwargs – extra parameters to change physics/settings

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

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

Returns:

flux density