redback.transient_models.tde_models.stream_stream_tde_bolometric

redback.transient_models.tde_models.stream_stream_tde_bolometric(time, mbh_6, mstar, c1, f, h_r, inc_tcool, del_omega, sigma_t, peak_time, **kwargs)

A bolometric TDE model based on stream-stream collisions. The early emission follows a gaussian rise.

Parameters:

• time – observer frame time in days

• mbh_6 – black hole mass (10^6 solar masses)

• mstar – mass of the disrupted star (solar masses)

• c1 – characteristic distance scale of the emission region in units of the apocenter distance of the most tightly bound debris

• f – fraction of the bound mass within the semimajor axis of the most tightly bound debris at peak mass return time

• h_r – aspect ratio used to calculate t_cool. This is only used when include_tcool_tdyn_ratio = 1

• inc_tcool – if include_tcool_tdyn_ratio = 1, the luminosity is limited by the Eddington luminosity if t_cool / t_dyn < 1.0

• del_omega – solid angle (in units of pi) of radiation from the emission region

• peak_time – peak time in days

• sigma_t – the sharpness of the Gaussian in days

Returns:

bolometric luminosity