trailMicro black holes captured inside neutron stars or white dwarfs accrete at approximately the Bondi rate
Accretion by micro black holes inside dense stars is limited by the Eddington luminosity.
A rapidly accreting captured black hole would destroy its host star on timescales shorter than observed stellar ages.
Radiation trapping defeats feedback· for
For micro black holes accreting in white-dwarf or neutron-star matter, the photon trapping radius far exceeds the Bondi radius
atomic
Radiation from a micro black hole accreting inside dense stellar matter is trapped and advected inward with the accretion flow
Accretion flow onto a black hole embedded inside a star is quasi-spherical rather than disk-like
Black holes inside neutron stars accrete at the Bondi rate without radiative feedback halting the accretion
Relativistic solutions and simulations· for
General-relativistic simulations of black holes accreting inside neutron stars find Bondi-type accretion rates proportional to the horizon area
atomic
Stellar rotation imparts enough angular momentum to slow a captured black hole's accretion well below the Bondi rate
atomic
claim · empirical · derivedA factual claim that rests on inference from other evidence rather than direct observation.constitution →claim page ↗︎
Micro black holes captured inside neutron stars or white dwarfs accrete at approximately the Bondi rate
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