Comparison of Different Tidal Disruption Event Light Curve Models with TiDE, a New Modular Open Source Code

Abstract

A tidal disruption event (TDE) occurs when a supermassive black hole disrupts a nearby passing star by tidal forces. The subsequent fallback accretion of the stellar debris results in a luminous transient outburst. Modeling the light curve of such an event may reveal important information, for example the mass of the central black hole. This paper presents the TiDE software based on semi-analytic modeling of TDEs. This object-oriented code contains different models for the accretion rate and the fallback timescale t min . We compare the resulting accretion rates to each other and with hydrodynamically simulated ones and find convincing agreement for full disruptions. We present a set of parameters estimated with TiDE for the well-observed TDE candidate AT2019qiz, and compare our results with those given by the MOSFiT code. Most of the parameters are in reasonable agreement, except for the mass and the radiative efficiency of the black hole, both of which depend heavily on the adopted fallback accretion rate.

Detectability of Strongly Gravitationally Lensed Tidal Disruption Events

“…Here we also noticed that compared with the mock mass distribution of disrupted stars in this paper, the available measurements of the disrupted star masses for the observed TDEs may vary by a factor of ∼0.1-10 or more due to different settings of the LC models. For example, as for the TDE source PS1-10jh, the star mass estimated by different LC fitting codes, i.e., MOSFiT, TDEmass, and TiDE (e.g., Mockler et al 2019;Ryu et al 2020;Kovács-Stermeczky & Vinkó 2023a), can be very different, which is ∼0.41/1.80/27.12 M e respectively. A more detailed comparison of these three codes can be seen in Kovács-Stermeczky & Vinkó (2023b).…”

“…Below we only summarize the main equations for predicting TDE LCs. For more details, please read Strubbe & Quataert (2009), Lodato &Rossi (2011), andVinkó (2023a).…”