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Beginning a journey across the universe: the discovery of extragalactic neutrino factories

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arxiv 2207.06314 v1 pith:KVWFIR7A submitted 2022-07-13 astro-ph.HE astro-ph.GA

Beginning a journey across the universe: the discovery of extragalactic neutrino factories

classification astro-ph.HE astro-ph.GA
keywords blazarsneutrinosastrophysicalextragalactichigh-energyneutrinosourcesacross
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Neutrinos are the most elusive particles in the Universe, capable of traveling nearly unimpeded across it. Despite the vast amount of data collected, a long standing and unsolved issue is still the association of high-energy neutrinos with the astrophysical sources that originate them. Amongst the candidate sources of neutrinos there are blazars, a class of extragalactic sources powered by supermassive black holes that feed highly relativistic jets, pointed towards the Earth. Previous studies appear controversial, with several efforts claiming a tentative link between high-energy neutrino events and individual blazars, and others putting into question such relation. In this work we show that blazars are unambiguously associated with high-energy astrophysical neutrinos at unprecedented level of confidence, i.e. chance probability of 6 x 10^{-7}. Our statistical analysis provides the observational evidence that blazars are astrophysical neutrino factories and hence, extragalactic cosmic-ray accelerators.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Active Galactic Nuclei as high-energy neutrino sources

    astro-ph.HE 2026-06 accept novelty 2.5

    AGN (jetted and non-jetted) are viable high-energy neutrino sources, with TXS 0506+056 and NGC 1068 as the only statistically significant associations so far, while gamma-ray blazars contribute only a small fraction o...

  2. Active Galactic Nuclei as high-energy neutrino sources

    astro-ph.HE 2026-06 unverdicted novelty 2.0

    Review summarizing correlations between astrophysical neutrinos and gamma-ray/radio AGN, specific source associations, proposed production mechanisms, and future prospects.