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@ARTICLE{Winter:461913,
      author       = {Winter, Walter and Lunardini, Cecilia},
      title        = {{P}ublisher {C}orrection: {A} concordance scenario for the
                      observed neutrino from a tidal disruption event},
      journal      = {Nature astronomy},
      volume       = {5},
      number       = {6},
      issn         = {2397-3366},
      address      = {London},
      publisher    = {Nature Publishing Group},
      reportid     = {PUBDB-2021-03170, arXiv:2005.06097. DESY-20-088},
      pages        = {621},
      year         = {2021},
      note         = {Waiting for fulltext},
      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.},
      cin          = {$Z_THAT$},
      ddc          = {520},
      cid          = {$I:(DE-H253)Z_THAT-20210408$},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613) /
                      NEUCOS - Neutrinos and the origin of the cosmic rays
                      (646623)},
      pid          = {G:(DE-HGF)POF4-613 / G:(EU-Grant)646623},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)16},
      eprint       = {2005.06097},
      howpublished = {arXiv:2005.06097},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2005.06097;\%\%$},
      UT           = {WOS:000628085700001},
      doi          = {10.1038/s41550-021-01343-x},
      url          = {https://bib-pubdb1.desy.de/record/461913},
}