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trailA rapidly accreting captured black hole would destroy its host star on timescales shorter than observed stellar ages.
Survival of white dwarfs and neutron stars constrains TeV-scale black hole accretion rates.
Bondi-rate consumption in dense matter· for
Micro black holes captured inside neutron stars or white dwarfs accrete at approximately the Bondi rate
For micro black holes accreting in white-dwarf or neutron-star matter, the photon trapping radius far exceeds the Bondi radius
Radiation from a micro black hole accreting inside dense stellar matter is trapped and advected inward with the accretion flow
General-relativistic simulations of black holes accreting inside neutron stars find Bondi-type accretion rates proportional to the horizon area
Stellar rotation imparts enough angular momentum to slow a captured black hole's accretion well below the Bondi rate
Old white dwarfs and neutron stars are observed to survive for billions of years
atomic
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.
Plaga's metastable black-hole risk scenario applies Hawking-radiation and accretion formulas inconsistently.
Eddington throttling objection· against
Accretion by micro black holes inside dense stars is limited by the Eddington luminosity.
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A rapidly accreting captured black hole would destroy its host star on timescales shorter than observed stellar ages.
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