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Why is it that we think ultra high energy cosmic rays are emitted from supernovae.
Ultra-high energy (UHE) cosmic rays, defined as those exceeding approximately 1018 eV, are primarily believed to originate from gamma-ray bursts (GRBs) rather than supernovae. Research from the University of Utah's Hi-Res group indicates that supernovae lack the necessary energy to accelerate particles to UHE levels. However, a connection has been established between long-duration GRBs and supernovae, suggesting a complex relationship in cosmic ray origins. Current studies continue to explore these dynamics and the implications for astrophysics.
PREREQUISITESAstronomers, astrophysicists, and researchers interested in cosmic ray origins and the dynamics of high-energy astrophysical phenomena.