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August 23, 2025SymmetryOpen Access

Ultra High-Energy Cosmic Ray Particle Trajectory Bending in Galactic Magnetic Fields

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This analysis reveals trajectory changes of UHECR in galaxy magnetic fields, indicating model impacts.

Trajectory changes of ultra high-energy cosmic rays were significantly influenced by galactic magnetic fields, showing varied results across models.
Using multiple galactic field models, the research found differences in UHECR trajectory outcomes, demonstrating their dependence on the magnetic field structure.
The calculations involved detailed models of magnetic fields, capturing the complexity of cosmic ray movement across the galaxy and uncertain source locations.
This research highlights the need for improved knowledge of galactic magnetic fields to enhance cosmic ray astronomy and its findings.

Tadeusz Wibig (2025) studied this question.

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