Journal Article PUBDB-2021-03170

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Publisher Correction: A concordance scenario for the observed neutrino from a tidal disruption event

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2021
Nature Publishing Group London

Nature astronomy 5(6), 621 () [10.1038/s41550-021-01343-x]
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Report No.: DESY-20-088; arXiv:2005.06097

Abstract: During a tidal disruption event, a star is torn apart by the tidal forces of a supermassive black hole, with about 50% of the star’s mass eventually accreted by the black hole. The resulting flare can, in extreme cases of super-Eddington mass accretion, result in a relativistic jet1,2,3,4. While tidal disruption events have been theoretically proposed as sources of high-energy cosmic rays5,6 and neutrinos7,8,9,10,11,12,13,14, stacking searches indicate that their contribution to the diffuse extragalactic neutrino flux is very low15. However, a recent association of a track-like astrophysical neutrino (IceCube-191001A16) with a tidal disruption event (AT2019dsg17) indicates that some tidal disruption events can accelerate cosmic rays to petaelectronvolt energies. Here we introduce a phenomenological concordance scenario with a relativistic jet to explain this association: an expanding cocoon progressively obscures the X-rays emitted by the accretion disk, while at the same time providing a sufficiently intense external target of backscattered X-rays for the production of neutrinos via proton–photon interactions. We also reproduce the delay (relative to the peak) of the neutrino emission by scaling the production radius with the black-body radius. Our energetics and assumptions for the jet and the cocoon are compatible with expectations from numerical simulations of tidal disruption events.

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Contributing Institute(s):
  1. Theoretische Astroteilchenphysik (Z_THAT)
Research Program(s):
  1. 613 - Matter and Radiation from the Universe (POF4-613) (POF4-613)
  2. NEUCOS - Neutrinos and the origin of the cosmic rays (646623) (646623)
Experiment(s):
  1. No specific instrument

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A concordance scenario for the observed neutrino from a tidal disruption event
Nature astronomy 5, 472 - 477 () [10.1038/s41550-021-01305-3]  GO Embargoed OpenAccess  Download fulltext Files  Download fulltextFulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS


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