The DOI matches its Crossref record; 5 of the 5 references it cites were found in a registry or an index.
The clustering of massive Primordial Black Holes as Dark Matter: Measuring their mass distribution with advanced LIGO
Open accessAbstract
The recent detection by Advanced LIGO of gravitational waves (GW) from the merging of a binary black hole system sets new limits on the merging rates of massive primordial black holes (PBH) that could be a significant fraction or even the totality of the dark matter in the Universe. aLIGO opens the way to the determination of the distribution and clustering of such massive PBH. If PBH clusters have a similar density to the one observed in ultra-faint dwarf galaxies, we find merging rates comparable to aLIGO expectations. Massive PBH dark matter predicts the existence of thousands of those dwarf galaxies where star formation is unlikely because of gas accretion onto PBH, which would possibly provide a solution to the missing satellite and too-big-to-fail problems. Finally, we study the possibility of using aLIGO and future GW antennas to measure the abundance and mass distribution of PBH in the range [5 - 200] Msun to 10\% accuracy.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Black Holes in the Early Universe
Carr, B. J., & Hawking, S. W. (1974) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/168.2.399 · Cited by 1,827
The primordial black hole mass spectrum
Carr, B. J. (1975) · The Astrophysical Journal · doi:10.1086/153853 · Cited by 1,460
New cosmological constraints on primordial black holes
Carr, B. J., Kohri, K., Sendouda, Y., & Yokoyama, J. (2010) · Physical Review D · doi:10.1103/physrevd.81.104019 · Cited by 1,166
Khlopov, M. Y. (2010) · Research in Astronomy and Astrophysics · doi:10.1088/1674-4527/10/6/001 · Cited by 681
Massive primordial black holes from hybrid inflation as dark matter and the seeds of galaxies
Clesse, S., & García-Bellido, J. (2015) · Physical Review D · doi:10.1103/physrevd.92.023524 · Cited by 471
Self-citation
Cited by
Constraints on primordial black holes
Carr, B., Kohri, K., Sendouda, Y., & Yokoyama, J. (2021) · Reports on Progress in Physics · doi:10.1088/1361-6633/ac1e31 · Cited by 1,156
Abbott, B. P., Abbott, R., Abbott, T. D., Abraham, S., Acernese, F., Ackley, K., Adams, C., Adhikari, R. X., Adya, V. B., Affeldt, C., et al. (2019) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ab3800 · Cited by 895
Primordial black holes—perspectives in gravitational wave astronomy
Sasaki, M., Suyama, T., Tanaka, T., & Yokoyama, S. (2018) · Classical and Quantum Gravity · doi:10.1088/1361-6382/aaa7b4 · Cited by 894
Primordial black hole constraints for extended mass functions
Carr, B., Raidal, M., Tenkanen, T., Vaskonen, V., & Veermäe, H. (2017) · Physical Review D · doi:10.1103/physrevd.96.023514 · Cited by 452
Gravitational Waves Induced by Non-Gaussian Scalar Perturbations
Cai, R.-G., Pi, S., & Sasaki, M. (2019) · Physical Review Letters · doi:10.1103/physrevlett.122.201101 · Cited by 435
Metadata
- Authors
- Clesse, S., & García-Bellido, J.
- Venue
- Physics of the Dark Universe
- Publisher
- Elsevier BV
- Published
- 2017-03
- Volume
- 15
- Pages
- 142-147
- ISSN
- 2212-6864 (ISSN-L)
- OpenAlex
- W2299686716
- Cited by
- 583
- References
- 5
- FWCI
- 26.40
- Type
- journal article
- Language
- en
- Open access
- green
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: The clustering of massive Primordial Black Holes as Dark Matter: Measuring their mass distribution with advanced LIGO. https://app.cochat.ai/papers/10.1016/j.dark.2016.10.002
- The paper
- Clesse, S., & García-Bellido, J. (2017). The clustering of massive Primordial Black Holes as Dark Matter: Measuring their mass distribution with advanced LIGO. Physics of the Dark Universe. https://doi.org/10.1016/j.dark.2016.10.002
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
