Simulated optical light curves of super-Eddington tidal disruption events with ZEBRA flows

We present simulated optical light curves of super-Eddington tidal disruption events (TDEs) using the zero-Bernoulli accretion (ZEBRA) flow model, which proposes that during phase, disc is quasi-spherical, radiation-pressure dominated, and accompanied by production strong jets. construct for both on- off-axis (with respect to jet) observers account anisotropic nature jetted emission. find at wavelengths, emission from orders magnitude brighter than produced jet, even with boosting synchrotron self-Compton. Comparing observed TDE Swift J2058.4+0516, we ZEBRA model accurately captures timescale remains reproduces luminosity transient. However, shape deviate early times radius temperature our modelled are $\sim2.7 - 4.1$ smaller $\sim1.4 2.3$ larger, respectively, observed. suggest this indicates inflates more, more rapidly, currently predicted discuss possible extensions this. Such refinements, coupled valuable new data upcoming large scale surveys, could help resolve TDEs how they powered.