Primordial black holes: constraints, potential evidence and prospects
arXiv:2601.06024 · doi:10.1007/s40766-026-00080-z
Abstract
Primordial black holes (PBHs) may have formed in the early Universe and may account for all or part of the dark matter. In this review, we summarize the current observational constraints on PBHs across the full mass range, highlight potential evidence for their existence, and outline the prospects for future searches, particularly with gravitational-wave observatories. We also discuss different PBH formation scenarios, identify the corresponding mass functions, and present the observational constraints in each case.
34 pages, 9 figures, 430 references, matches the version published in La Rivista del Nuovo Cimento
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- The Dark Side of the Moon: Listening to Scalar-Induced Gravitational Waves
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