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- W4384808229 abstract "The origin of the TeV--PeV astrophysical neutrinos seen by the IceCube telescope is unknown. If they are made in proton-photon interactions in astrophysical sources, their spectrum may show bump-like features. We search for such features in the 7.5-years High-Energy Starting Events (HESE), and forecast the power of such searches using larger data samples expected from upcoming telescopes. Present-day data reveals no evidence of bump-like features, which allows us to constrain candidate populations of photohadronic neutrino sources. Near-future forecasts show promising potential for stringent constraints or decisive discovery of bump-like features. Our results provide new insight into the origins of high-energy astrophysical neutrinos, complementing those from point-source searches." @default.
- W4384808229 created "2023-07-20" @default.
- W4384808229 creator A5046213613 @default.
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- W4384808229 date "2023-07-18" @default.
- W4384808229 modified "2023-09-27" @default.
- W4384808229 title "Hunting for bumps in the diffuse high-energy neutrino flux" @default.
- W4384808229 doi "https://doi.org/10.48550/arxiv.2307.09170" @default.
- W4384808229 hasPublicationYear "2023" @default.
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