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Question

Accepted Answer

Diffusive shock acceleration in supernova shocks expanding into stellar wind cavities can accelerate cosmic-ray particles to energies of ≥10^15 eV and potentially explain elemental and isotopic anomalies in cosmic rays. Novelty: ClaimNovelty.INCREMENTAL. Consensus alignment: ConsensusAlignment.NEUTRAL.

Maximum energy of cosmic-ray particles accelerated by supernova remnant shocks in stellar wind cavities

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