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- W3174647119 abstract "The origin of the cosmic neutrino signal measured by IceCube is still unknown. A general correlation between the sources of high-energy $gamma$-ray sources with IceCube neutrinos is expected since hadronic interactions are the crucial precursors of both messengers at such high energies. Blazars dominate the extragalactic $gamma$-ray sky. However, neutrinos originating from inside the blazar jets cannot account for more than $sim30%$ of the diffuse flux. We study ultrahigh-energy cosmic-ray contribution to the diffuse flux through photopion interactions on cosmic background photons. The extragalactic background light, consisting of IR/UV/optical photons require a proton energy threshold of $E_{rm th}^{p,pi} approx 10^{17}$ eV for pion production. The latter can yield PeV neutrinos. We analyze the total contribution from resolved and unresolved blazars by using a luminosity-dependent density evolution of blazars. The latest Fermi-LAT 4LAC catalog sheds light on the redshift distribution of the diffuse neutrino flux for resolved $gamma$-ray blazars." @default.
- W3174647119 created "2021-07-05" @default.
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- W3174647119 date "2021-06-28" @default.
- W3174647119 modified "2023-10-16" @default.
- W3174647119 title "Diffuse neutrino flux from blazars via cosmic-ray propagation in extragalactic medium" @default.
- W3174647119 doi "https://doi.org/10.22323/1.395.1003" @default.
- W3174647119 hasPublicationYear "2021" @default.
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