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

Space Sciences

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

D. R. Pasham, M. Zajaček, et al.

This groundbreaking research reveals the presence of strong, quasi-periodic X-ray flux and temperature modulations in the tidal disruption event AT2020ocn/ZTF18aakelin, suggesting insights into black hole dynamics, led by Dheeraj R. Pasham and his colleagues.

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Playback language: English
Abstract
This paper reports the discovery of strong, quasi-periodic X-ray flux and temperature modulations in a tidal disruption event (TDE), AT2020ocn/ZTF18aakelin. These modulations, separated by roughly 15 days and lasting about 130 days, are consistent with Lense-Thirring precession of the accretion flow. While other mechanisms cannot be ruled out, the authors constrain the black hole's dimensionless spin parameter (a) to be between 0.05 and 0.5, assuming typical TDE parameters and rigid body precession of the disk.
Publisher
Nature
Published On
May 22, 2024
Authors
Dheeraj R. Pasham, Michal Zajaček, C. J. Nixon, Eric R. Coughlin, Marzena Śniegowska, Agnieszka Janiuk, Bożena Czerny, Thomas Wevers, Muryel Guolo, Yukta Ajay, Michael Loewenstein
Tags
X-ray flux
temperature modulations
tidal disruption event
black hole spin
Lense-Thirring precession
accretion flow
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