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Quantum-mechanical Suppression of Accretion by Primordial Black Holes

The Schwarzschild radii of primordial black holes (PBHs) in the mass range of 6 × 10 ^14 –4 × 10 ^19 g match the sizes of nuclei to atoms. I discuss the resulting quantum-mechanical suppression in the accretion of matter by PBHs in dense astrophysical environments, such as planets or stars.

Furkejuvvon:
Bibliográfalaš dieđut
Váldodahkki: Abraham Loeb
Materiálatiipa: Artigo
Giella:Inglês
Almmustuhtton: IOP Publishing 2024-01-01
Ráidu:The Astrophysical Journal Letters
Fáttát:
Liŋkkat:https://doi.org/10.3847/2041-8213/ad887d
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