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From the Dawn of Neutrino Astronomy to A New View of the Extreme Universe

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arxiv 2405.17623 v2 pith:BFVC6Z7Q submitted 2024-05-27 hep-ex astro-ph.HEhep-ph

classification hep-exastro-ph.HEhep-ph
keywords neutrinoextremeuniverseastronomyastrophysicsauthorsdiscoverynext
verification ladder T0 review T1 audit T2 compute T3 formal
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Over the past decade, neutrino astronomy has emerged as a new window into the extreme and hidden universe. Current-generation experiments have detected high-energy neutrinos of astrophysical origin and identified the first sources, opening the field to discovery. Looking ahead, the authors of this Perspective identify seven major open questions in neutrino astrophysics and particle physics that could lead to transformative discoveries over the next 20 years. These multidisciplinary questions range from understanding the vicinity of a black hole to unveiling the nature of neutrino mass, among other topics. Additionally, we critically review the current experimental capabilities and their limitations and, from there, discuss the interplay between different proposed neutrino telescope technologies and analysis techniques. The authors firmly believe that achieving the immense discovery potential over the next two decades demands a model of global partnership and specialized, complementary detectors. This collaborative neutrino telescope network will pave the way for a thriving multimessenger era, transforming our understanding of neutrino physics, astrophysics, and the extreme universe.

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Cited by 2 Pith papers

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

  1. Astrophysical Neutrino Sources as Colliders

    hep-ph 2026-07 conditional novelty 7.0 of 10

    Neutrino point-source observations (IceCube, KM3NeT) can bound inelastic pp and pγ cross sections from √s ≈ 1 GeV to ~10^5 GeV, extending beyond LHC/HERA and sometimes below unitarity limits.

  2. Four, One, and None: Quantifying the Ultra-High-Energy Neutrino Anomaly Across ANITA-IV, KM3NeT, and IceCube

    astro-ph.HE 2026-07 conditional novelty 6.0 of 10

    A joint three-detector analysis finds that ANITA-IV's four events and KM3NeT's 220 PeV event cannot be reconciled with IceCube's silence under any Standard Model diffuse or transient flux, leaving a 5.9-7.9σ anomaly.

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