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| Preprint | PUBDB-2022-04968 |
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2022
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Report No.: arXiv:2203.08096
Abstract: Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With energies far beyond solar, supernovae, atmospheric, and accelerator neutrinos, high-energy and ultra-high-energy neutrinos probe fundamental physics from the TeV scale to the EeV scale and beyond. They are sensitive to physics both within and beyond the Standard Model through their production mechanisms and in their propagation over cosmological distances. They carry unique information about their extreme non-thermal sources by giving insight into regions that are opaque to electromagnetic radiation. This white paper describes the opportunities astrophysical neutrino observations offer for astrophysics and high-energy physics, today and in coming years.
Keyword(s): neutrino: energy ; neutrino: energy: high ; neutrino: UHE ; neutrino: detector ; neutrino: propagation ; neutrino: decay ; neutrino: flux ; WIMP: dark matter ; neutrino: supernova ; ANITA ; IceCube ; KM3NeT ; Baikal ; numerical calculations ; new physics ; neutrino, UHE
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Contribution to a conference proceedings/Journal Article
High-energy and ultra-high-energy neutrinos: A Snowmass white paper
2022 Snowmass Summer Study, SeattleSeattle, United States, 17 Jul 2022 - 26 Jul 2022
Journal of high energy astrophysics 36, 55 - 110 (2022) [10.1016/j.jheap.2022.08.001]
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