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Accretion of Primordial Black Holes in Stellar Interiors

  • Authors: Matteo Cantiello, Ore Gottlieb, Cameron Norton, Matthew Kleban, Ken Van Tilburg

Matteo Cantiello et al 2026 The Astrophysical Journal 1010 .

  • Provider: AAS Journals

Caption: Figure B1.

Schematic of the recycling and pileup geometry inside the collisionless region. The flow is hydrodynamic near rB and becomes collisionless below rcoll. Most particles miss the GR loss cone on a single inward pass, return to rcoll, rethermalize, and either are recaptured or circularize after losing orbital energy to bremsstrahlung. Direct GR capture (loss cone) accounts for ∼0.2% of entrants; ∼33% are reflected at the centrifugal barrier, and ∼67% enter the recycling + circularization population.

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