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trailUltra-high-energy cosmic rays strike white dwarfs and neutron stars at astrophysically significant rates.
If TeV-scale black hole production is possible in particle collisions, cosmic rays striking white dwarfs or neutron stars would produce such black holes.
Measured flux times stellar cross-section· for
Cosmic rays with energies above 10^18 eV are observed.
atomic
Some white dwarfs have magnetic fields weak enough for ultra-high-energy cosmic rays to reach their surfaces.
atomic
Magnetic screening of neutron stars· against
Strong magnetic fields shield most neutron stars from charged ultra-high-energy cosmic rays.
atomic
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Ultra-high-energy cosmic rays strike white dwarfs and neutron stars at astrophysically significant rates.
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