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Primordial black holes captured by neutron stars: Simulations in general relativity · DOI 10.1103/physrevd.110.023021

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astro-ph.HE 1

years

2026 1

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UNVERDICTED 1

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Accretion of Primordial Black Holes in Stellar Interiors

astro-ph.HE · 2026-06-01 · unverdicted · novelty 7.0

Self-consistent spherical accretion simulations show cooling-enhanced growth of PBHs with radiative efficiency ~10^{-2} in the bremsstrahlung regime, yielding a critical seed mass of ~10^{-16} M_sun to consume a solar-mass star in a Hubble time.

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  • Accretion of Primordial Black Holes in Stellar Interiors astro-ph.HE · 2026-06-01 · unverdicted · none · ref 41

    Self-consistent spherical accretion simulations show cooling-enhanced growth of PBHs with radiative efficiency ~10^{-2} in the bremsstrahlung regime, yielding a critical seed mass of ~10^{-16} M_sun to consume a solar-mass star in a Hubble time.