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2025

Bright Cosmic-Ray Source as a Solution to Auger-TA Tensions

Korochkin, Alexander, Semikoz, Dmitri, Tinyakov, Peter

Understand

The ultra-high-energy cosmic ray (UHECR) spectra measured by the Pierre Auger Observatory (Auger) and the Telescope Array (TA) agree very well below $10^{19.5}$ eV but differ significantly at higher energies.

We show that these differences can be explained by a single nearby source superimposed on a nearly isotropic background.
Taking into account deflections in Galactic and extragalactic magnetic fields, such a source can account for the excess in the TA spectrum without producing excessive anisotropy.
The required hard spectrum of the source and intermediate-mass composition are consistent with previous fits of the Auger-only spectrum and composition.