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trailSurvival of white dwarfs and neutron stars constrains TeV-scale black hole accretion rates.
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.
Particle collisions at the LHC pose no danger to Earth.
Stellar survival bound· for
If TeV-scale black hole production is possible in particle collisions, cosmic rays striking white dwarfs or neutron stars would produce such black holes.
Cosmic ray collisions with Earth's atmosphere reach energies exceeding LHC collision energies.
Ultra-high-energy cosmic rays strike white dwarfs and neutron stars at astrophysically significant rates.
The highest-energy cosmic rays include a substantial proton fraction.
Stable microscopic black holes produced by cosmic rays striking white dwarfs or neutron stars would be stopped inside those stars, whether charged or neutral.
Charged microscopic black holes are stopped in dense stellar matter by electromagnetic energy loss.
Gravitational and accretional energy loss stops neutral TeV-scale black holes inside white dwarfs.
A rapidly accreting captured black hole would destroy its host star on timescales shorter than observed stellar ages.
Micro black holes captured inside neutron stars or white dwarfs accrete at approximately the Bondi rate
A black hole accreting hazardously fast on Earth would accrete faster inside white dwarfs or neutron stars.
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Survival of white dwarfs and neutron stars constrains TeV-scale black hole accretion rates.
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