A beam of ultrahigh energy particles of the same magnetic rigidity
G.F. Krymsky, I.Ye. Sleptsov, M.I. Pravdin, A.D. Krasilnikov

TL;DR
This paper reports the detection of three ultra-high-energy cosmic ray particles with similar magnetic rigidity, suggesting a common origin or acceleration process, based on observations from two different arrays.
Contribution
It presents evidence of a beam of particles with the same magnetic rigidity at energies above 30 EeV, indicating magnetic separation effects in their acceleration and propagation.
Findings
Three particles detected with energies above 30 EeV from the same sky region.
Particles exhibit similar magnetic rigidity despite differing energies.
Evidence suggests magnetic separation in acceleration and propagation processes.
Abstract
Two EAS arrays during a day have recorded 3 particles with energies above 30 EeV arriving from the same sky region. Two events were registered by the Yakutsk array and one - by the Telescope Array. Two Yakutsk events were estimated to be same energy and the Telescope Array shower's energy was almost 2 times higher. This indicates the same magnetic rigidity of all three particles, if the charge differs by a factor of 2. The relatively short sequence of all three events and their "monochromaticity" in rigidity can be due to the magnetic separation of particles in the acceleration process and propagation of the beam.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Solar and Space Plasma Dynamics · Gamma-ray bursts and supernovae
