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- W2079396771 endingPage "1433" @default.
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- W2079396771 abstract "Some of the proposed explanations for the origin of ultrahigh-energy cosmic rays invoke new sources of energetic photons (e.g., topological defects, relic particles, etc.). At high redshift, when the cosmic microwave background has a higher temperature but the radio background is low, the ultrahigh-energy photons can generate neutrinos through pair production of muons and pions. The resulting diffuse background of 10(17) eV neutrinos can be detected by future experiments." @default.
- W2079396771 created "2016-06-24" @default.
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- W2079396771 date "2001-02-19" @default.
- W2079396771 modified "2023-09-25" @default.
- W2079396771 title "Neutrinos Produced by Ultrahigh-Energy Photons at High Redshift" @default.
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- W2079396771 doi "https://doi.org/10.1103/physrevlett.86.1430" @default.
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