redback.transient_models.tde_models.smooth_exponential_powerlaw_cooling_envelope_bolometric

redback.transient_models.tde_models.smooth_exponential_powerlaw_cooling_envelope_bolometric(time, peak_time, alpha_1, alpha_2, smoothing_factor, mbh_6, stellar_mass, eta, alpha, beta, **kwargs)[source]

Full lightcurve, with smoothed exponential power law rise till xi * fallback time and then the metzger tde model, bolometric version for fitting the bolometric lightcurve

Parameters:

  • time – time in source frame in days

  • peak_time – peak time in days

  • alpha_1 – power law index before peak

  • alpha_2 – power law index after peak

  • smoothing_factor – controls transition smoothness at peak (higher = smoother)

  • mbh_6 – mass of supermassive black hole in units of 10^6 solar mass

  • stellar_mass – stellar mass in units of solar masses

  • eta – SMBH feedback efficiency (typical range: etamin - 0.1)

  • alpha – disk viscosity

  • beta – TDE penetration factor (typical range: 1 - beta_max)

  • xi – Optional transition factor - smooth exponential power law transitions to cooling envelope at xi * tfb

  • kwargs – Additional parameters, check _cooling_envelope for more information

:return luminosity in ergs/s