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trailBlack holes capable of Eddington-limited accretion and radiation are also subject to astrophysical retention bounds.
Astrophysical bounds from stellar survival do not exclude metastable collider-produced black holes.
Catastrophic growth does not occur in Plaga's metastable micro black hole scenario.
Same-physics coverage (Giddings–Mangano)· 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 black hole accreting hazardously fast on Earth would accrete faster inside white dwarfs or neutron stars.
White dwarf and neutron star interiors are vastly denser than terrestrial matter.
Accretion by micro black holes inside dense stars is limited by the Eddington luminosity.
Plaga's metastable black-hole risk scenario applies Hawking-radiation and accretion formulas inconsistently.
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Plaga's observational-evasion counter· against
Eddington-limited accretion by metastable micro black holes would evade existing astrophysical observations.
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Black holes capable of Eddington-limited accretion and radiation are also subject to astrophysical retention bounds.
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