Ultraheavy Cosmic Rays May Solve 60-Year Mystery of Their Origins
High-energy cosmic rays, possessing energy levels over ten million times greater than particles accelerated in Earth's Large Hadron Collider, have long puzzled scientists regarding their origins. A prominent example, the Amaterasu particle detected in 2021, exhibited energy forty million times greater than LHC collisions yet appeared to originate from an empty region of space. New research led by Kohta Murase at Penn State suggests a breakthrough in this sixty-year-old mystery. The study proposes that these ultra-high-energy cosmic rays are actually atomic nuclei of elements heavier than iron. This superheavy composition could explain how such particles are accelerated by the universe's most violent events and why their trajectories appear misleading. By identifying these particles as heavy nuclei rather than protons, researchers may finally unlock the mechanisms behind their acceleration and pinpoint their mysterious sources. This finding represents a potential key to understanding the extreme astrophysical processes capable of flinging such intensely powerful particles toward Earth, marking a significant step forward in particle physics and astrophysics.
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