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Astrophysics Uniquely Enabled by Observations of High-Energy Cosmic Neutrinos

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arxiv 1903.04334 v2 pith:3S3YPJUP submitted 2019-03-11 astro-ph.HE astro-ph.COhep-ph

Astrophysics Uniquely Enabled by Observations of High-Energy Cosmic Neutrinos

Markus Ackermann , Markus Ahlers , Luis Anchordoqui , Mauricio Bustamante , Amy Connolly , Cosmin Deaconu , Darren Grant , Peter Gorham
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Francis Halzen Albrecht Karle Kumiko Kotera Marek Kowalski Miguel A. Mostafa Kohta Murase Anna Nelles Angela Olinto Andres Romero-Wolf Abigail Vieregg Stephanie Wissel
This is my paper
classification astro-ph.HE astro-ph.COhep-ph
keywords neutrinoscosmicsourcesaddressastrophysicsenergetichigh-energymeasurements
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High-energy cosmic neutrinos carry unique information about the most energetic non-thermal sources in the Universe. This white paper describes the outstanding astrophysics questions that neutrino astronomy can address in the coming decade. A companion white paper discusses how the observation of cosmic neutrinos can address open questions in fundamental physics. Detailed measurements of the diffuse neutrino flux, measurements of neutrinos from point sources, and multi-messenger observations with neutrinos will enable the discovery and characterization of the most energetic sources in the Universe.

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Cited by 4 Pith papers

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

  1. Are neutrinos Majorana? Fixed-target and high-energy astrophysical searches decide

    hep-ph 2026-06 unverdicted novelty 6.0

    Correlated HNL discovery at SHiP and flavor ratio shifts in astrophysical neutrinos at telescopes would establish neutrinos as Majorana fermions.

  2. Astrophysical bounds on the high-energy evolution of neutrino mixing

    hep-ph 2026-04 unverdicted novelty 5.0

    High-energy astrophysical neutrinos can constrain the running of neutrino mixing parameters with energy, with future multi-detector setups forecast to set strong bounds despite astrophysical uncertainties.

  3. Trinity: An Air-Shower Imaging Instrument to detect Ultrahigh Energy Neutrinos

    astro-ph.IM 2019-07 unverdicted novelty 5.0

    Proposes the Trinity air-shower imaging system for detecting ultrahigh energy tau neutrinos between 10^7 and 10^10 GeV to address IceCube neutrino sources, UHECR origins, and high-energy neutrino physics.

  4. POEMMA (Probe of Extreme Multi-Messenger Astrophysics) design

    astro-ph.HE 2019-07 unverdicted novelty 3.0

    POEMMA is a proposed NASA probe-class mission designed to observe ultra-high energy cosmic rays and cosmic neutrinos from space.