trailRadiation from a micro black hole accreting inside dense stellar matter is trapped and advected inward with the accretion flow
Accretion by micro black holes inside dense stars is limited by the Eddington luminosity.
Micro black holes captured inside neutron stars or white dwarfs accrete at approximately the Bondi rate
Photon trapping condition· for
For micro black holes accreting in white-dwarf or neutron-star matter, the photon trapping radius far exceeds the Bondi radius
atomic
Simulation evidence· for
Black holes inside neutron stars accrete at the Bondi rate without radiative feedback halting the accretion
atomic
assumed
Accretion flow onto a black hole embedded inside a star is quasi-spherical rather than disk-like
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Radiation from a micro black hole accreting inside dense stellar matter is trapped and advected inward with the accretion flow
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2depended on by
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