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引用次数: 0
摘要
质量范围在 6 × 1014-4 × 1019 g 的原始黑洞（PBHs）的施瓦兹柴尔德半径与原子核到原子的大小相匹配。我将讨论在致密天体物理环境（如行星或恒星）中，原始黑洞对物质吸积所产生的量子力学抑制。
Quantum-mechanical Suppression of Accretion by Primordial Black Holes
The Schwarzschild radii of primordial black holes (PBHs) in the mass range of 6 × 1014–4 × 1019 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.
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