Repeating Partial Tidal Encounters of Sun-like Stars Leading to their Complete Disruption

TL;DR

This study uses 3D hydrodynamic simulations to explore how Sun-like stars undergo multiple partial tidal disruptions by supermassive black holes, leading to eventual complete destruction and complex flare patterns.

Contribution

It provides new insights into the evolution of stars under repeated tidal encounters, highlighting the role of stellar structure and the implications for observing and interpreting TDEs.

Findings

Stars become less concentrated after tidal encounters.

Mass loss correlates with the ratio of central to average density.

Repeated encounters lead to complete stellar disruption.

Abstract

Stars grazing supermassive black holes on bound orbits may produce periodic flares over many passages, known as repeating partial tidal disruption events (TDEs). Here, we present 3D hydrodynamic simulations of sun-like stars over multiple tidal encounters. The star is significantly restructured and becomes less concentrated as a result of mass loss and tidal heating. The vulnerability to mass loss depends sensitively on the stellar density structure, and the strong correlation between the fractional mass loss $\Delta M/M_*$ and the ratio of the central and average density $\rho_{\mathrm{c}}/\bar\rho$, which was initially derived in disruption simulations of main-sequence stars, also applies for stars strongly reshaped by tides. Over multiple orbits, the star loses progressively more mass in each encounter and is doomed to a complete disruption. Throughout its lifetime, the star may produce numerous weak flares (depending on the initial impact parameter), followed by a couple of luminous flares whose brightness increases exponentially. Flux-limited surveys are heavily biased toward the brightest flares, which may appear similar to the flare produced by the same star undergoing a full disruption on its first tidal encounter. This places new challenges on constraining the intrinsic TDE rates, which need to take repeating TDEs into account. Other types of stars with different initial density structures (e.g., evolved stars with massive cores) follow distinct evolution tracks, which might explain the diversity of the long-term luminosity evolution seen in recently uncovered repeaters.