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Ultra-deep tidal disruption events: prompt self-intersections and observables

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journal contribution
posted on 24.09.2019, 08:24 by Siva Darbha, Eric R. Coughlin, Daniel Kasen, Chris Nixon
star approaching a supermassive black hole (SMBH) can be torn apart in a tidal disruption event (TDE). We examine ultra-deep TDEs, a new regime in which the disrupted debris approaches close to the black hole’s Schwarzschild radius, and the leading part intersects the trailing part at the first pericentre passage. We calculate the range of penetration factors β versus SMBH masses M that produce these prompt self-intersections using a Newtonian analytic estimate and a general relativistic (GR) geodesic model. We find that significant self-intersection of Solar-type stars requires β ∼ 50–127 for M/M⊙ = 104, down to β ∼ 5.6–5.9 forM/M⊙ = 106. We run smoothed particle hydrodynamic (SPH) simulations to corroborate our calculations and find close agreement, with a slightly shallower dependence on M. We predict that the shock from the collision emits an X-ray flare lasting t ∼ 2 s with L ∼ 1047 erg s−1 at E ∼ 2 keV, and the debris has a prompt accretion episode lasting t ∼ several minutes. The events are rare and occur with a rate N˙≲10−7 Mpc−3 yr−1. Ultra-deep TDEs can probe the strong gravity and demographics of low-mass SMBHs.

Funding

This research used resources of the National Energy Research Scientific Computing Center, a Department of Energy Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under contract no. DE-AC02-05CH11231. This work was supported by the National Science Foundation under grant no. 1616754. ERC was supported by the National Aeronautics and Space Administration through the Einstein Fellowship Program, grant PF6-170170. CJN is supported by the Science and Technology Facilities Council (grant no. ST/M005917/1).

History

Citation

Monthly Notices of the Royal Astronomical Society, 2019, 488 (4), pp. 5267-5278 (12)

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy

Version

VoR (Version of Record)

Published in

Monthly Notices of the Royal Astronomical Society

Publisher

Oxford University Press (OUP), Royal Astronomical Society

issn

0035-8711

eissn

1365-2966

Acceptance date

09/07/2019

Copyright date

2019

Available date

24/09/2019

Publisher version

https://academic.oup.com/mnras/article/488/4/5267/5531769

Language

en