“…Bonnerot, Rossi, Lodato, & Price 2016). Even though TDEs are facilitated by the large tidal radius of massive BHs, the large number of stellar-mass BBHs in the Galaxy (Lamberts et al, 2018) could be an asset to expect TDEs from stellar-mass BBHs in young stellar clusters (Kremer et al 2020, see also Ryu, Perna, & Wang 2022). Up to now, stellar-mass BBHs harboring a post-TDE disk may not be distinguishable from a low-mass X-ray binary system, i.e.…”