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trailIf TeV-scale black hole production is possible in particle collisions, cosmic rays striking white dwarfs or neutron stars would produce such black holes.
TeV-scale black holes produced at the LHC pose no significant risk.
Black holes capable of Eddington-limited accretion and radiation are also subject to astrophysical retention bounds.
Survival of white dwarfs and neutron stars constrains TeV-scale black hole accretion rates.
Kinematic and flux argument· for
Cosmic rays with energies above 10^18 eV are observed.
atomic
Cosmic ray collisions with Earth's atmosphere reach energies exceeding LHC collision energies.
The center-of-mass energy of the highest-energy cosmic-ray atmospheric collisions exceeds the LHC's collision energy.
Ultra-high-energy cosmic rays strike white dwarfs and neutron stars at astrophysically significant rates.
Some white dwarfs have magnetic fields weak enough for ultra-high-energy cosmic rays to reach their surfaces.
Strong magnetic fields shield most neutron stars from charged ultra-high-energy cosmic rays.
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If TeV-scale black hole production is possible in particle collisions, cosmic rays striking white dwarfs or neutron stars would produce such black holes.
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