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| Contribution to a conference proceedings/Journal Article | PUBDB-2022-04914 |
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2022
Elsevier
Amsterdam [u.a.]
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Please use a persistent id in citations: doi:10.1016/j.jheap.2022.08.001
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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High-energy and ultra-high-energy neutrinos: A Snowmass white paper
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