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The paper successfully models X-ray observational aspects of Quasi-Periodic Eruptions (QPEs) in galactic nuclei as due to collisions between a Tidal Disruption Event (TDE) accretion disk and a stellar mass black hole or main sequence star orbiting around a nuclear supermassive black hole (SMBH). This can have key implications in understanding EMRIs and stellar orbits in the vicinity of SMBHs.
Zhou et al. (Mon,) studied this question.