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.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
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.