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- W4377029481 abstract "We consider the prospects for future ultrahigh energy cosmic ray and neutrino observations to constrain the evolution of sources producing a proton flux above 10 EeV ($1text{ }text{ }mathrm{EeV}={10}^{18}text{ }text{ }mathrm{eV}$). We find that strong constraints on the source evolution can be obtained by combining measurements of the cosmic ray proton fraction above 30 EeV with measurement of the neutrino flux at 1 EeV, if neutrinos are predominantly of cosmogenic origin. In the case that interactions in the source environment produce a significant astrophysical neutrino flux, constraints on the source evolution may require measurement of the observed proton fraction, as well as, the neutrino flux at multiple energies, such as 1 EeV and 10 EeV. Finally, we show that fits to current UHECR data favor models which result in a $>30text{ }text{ }mathrm{EeV}$ proton fraction and 1 EeV neutrino flux that could realistically be discovered by the next generation of experiments." @default.
- W4377029481 created "2023-05-19" @default.
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- W4377029481 date "2023-05-18" @default.
- W4377029481 modified "2023-10-18" @default.
- W4377029481 title "Prospects for joint cosmic ray and neutrino constraints on the evolution of trans-Greisen-Zatsepin-Kuzmin proton sources" @default.
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- W4377029481 doi "https://doi.org/10.1103/physrevd.107.103030" @default.
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