Multi-epoch Modeling of TXS 0506+056 and Implications for Long-term High-energy Neutrino Emission

@article{Petropoulou2019MultiepochMO,
  title={Multi-epoch Modeling of TXS 0506+056 and Implications for Long-term High-energy Neutrino Emission},
  author={M. Petropoulou and K. Murase and M. Santander and S. Buson and A. Tohuvavohu and T. Kawamuro and G. Vasilopoulos and Hiroshi Negoro and Y. Ueda and M. Siegel and A. Keivani and N. Kawai and A. Mastichiadis and S. Dimitrakoudis},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2019}
}
Blazars have been proposed as efficient particle accelerators and promising neutrino sources long before the discovery of astrophysical high-energy neutrinos. The recent report by the IceCube Collaboration of a $\sim 3.5\sigma$ excess of $13\pm5$ neutrino events in the direction of the blazar TXS 0506+056 during a six month-long period in 2014-2015 as well as the detection of a single high-energy neutrino, IceCube-170922A, during a major gamma-ray flare from the same blazar in 2017, have… Expand
A Neutral Beam Model for High-energy Neutrino Emission from the Blazar TXS 0506+056
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