Primordial black holes: constraints, potential evidence and prospects
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.
Authors
- B. Carr
- Hardi Veermäe (ORCID: https://orcid.org/0000-0003-1845-1355)
- Ville Vaskonen
- Antonio J. Iovino
- Gabriele Perna
Institutions
- New York University Abu Dhabi (AE)
- University of Padua (IT)
- Queen Mary University of London (GB)
- National Institute of Chemical Physics and Biophysics (EE)
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova (IT)
Publication Details
- Journal
- Rivista Del Nuovo Cimento
- Published
- 2026-03-31
- DOI
- https://doi.org/10.1007/s40766-026-00080-z
- Primary Topic
- Pulsars and Gravitational Waves Research
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- European Commission
- Eesti Teadusagentuur
- Università degli Studi di Padova
- HORIZON EUROPE Framework Programme