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trailThe highest-energy cosmic rays include a substantial proton fraction.
If TeV-scale black hole production is possible in particle collisions, cosmic rays striking white dwarfs or neutron stars would produce such black holes.
Telescope Array light-composition data· for
Telescope Array shower-maximum measurements are consistent with a predominantly protonic composition up to about 10^19 eV
atomic
Auger heavier-composition trend· against
Pierre Auger Observatory shower-maximum measurements indicate cosmic-ray composition becomes heavier above about 2×10^18 eV
The mean shower-maximum depth measured by the Pierre Auger Observatory increases more slowly with energy above about 2×10^18 eV than expected for constant composition
Shower-to-shower fluctuations of shower-maximum depth measured by the Pierre Auger Observatory decrease with energy above about 2×10^18 eV
assumed
Hadronic interaction models reliably predict the air-shower observables used to infer cosmic-ray composition
A factual claim that rests on inference from other evidence rather than direct observation.constitutionclaim page ↗︎
The highest-energy cosmic rays include a substantial proton fraction.
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