Lense–Thirring precession after a supermassive black hole disrupts a star

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Publikace nespadá pod Ekonomicko-správní fakultu, ale pod Přírodovědeckou fakultu. Oficiální stránka publikace je na webu muni.cz.
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PASHAM Dheeraj R. ZAJAČEK Michal NIXON C. J. COUGHLIN Eric R. ŚNIEGOWSKA Marzena JANIUK Agnieszka CZERNY Bożena WEVERS Thomas GUOLO Muryel AJAY Yukta LOEWENSTEIN Michael

Rok publikování 2024
Druh Článek v odborném periodiku
Časopis / Zdroj Nature
Fakulta / Pracoviště MU

Přírodovědecká fakulta

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Doi http://dx.doi.org/10.1038/s41586-024-07433-w
Klíčová slova Compact astrophysical objects; General relativity and gravity; High-energy astrophysics; Transient astrophysical phenomena
Popis An accretion disk formed around a supermassive black hole after it disrupts a star is expected to be initially misaligned with respect to the equatorial plane of the black hole. This misalignment induces relativistic torques (the Lense–Thirring effect) on the disk, causing the disk to precess at early times, whereas at late times the disk aligns with the black hole and precession terminates1,2. Here we report, using high-cadence X-ray monitoring observations of a tidal disruption event (TDE), the discovery of strong, quasi-periodic X-ray flux and temperature modulations. These X-ray modulations are separated by roughly 15?days and persist for about 130?days during the early phase of the TDE. Lense–Thirring precession of the accretion flow can produce this X-ray variability, but other physical mechanisms, such as the radiation-pressure instability3,4, cannot be ruled out. Assuming typical TDE parameters, that is, a solar-like star with the resulting disk extending at most to the so-called circularization radius, and that the disk precesses as a rigid body, we constrain the disrupting dimensionless spin parameter of the black hole to be 0.05???|a|???0.5.
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