Self-generated magnetic turbulence in cosmic filaments suppresses low-rigidity UHECR escape for cluster-scale sources, photodisintegrates heavy nuclei into secondary protons below the ankle, and yields neutrino and gamma-ray fluxes compatible with or constrained by current limits.
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Magnetized cosmic web filaments suppress UHECR proton flux below 3×10^19 eV, producing magnetic horizon radii of ~50 Mpc at 10^18 eV and ~150 Mpc at 10^19 eV.
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Self-confinement of ultra-high-energy nuclei in cosmic filaments: implications for the UHECR spectrum and composition
Self-generated magnetic turbulence in cosmic filaments suppresses low-rigidity UHECR escape for cluster-scale sources, photodisintegrates heavy nuclei into secondary protons below the ankle, and yields neutrino and gamma-ray fluxes compatible with or constrained by current limits.
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The Impact of the Magnetised Cosmic Web on Ultra High Energy Cosmic Ray Propagation
Magnetized cosmic web filaments suppress UHECR proton flux below 3×10^19 eV, producing magnetic horizon radii of ~50 Mpc at 10^18 eV and ~150 Mpc at 10^19 eV.