The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.
Asymmetric Dark Matter: Theories, signatures, and constraints
Open accessAbstract
We review theories of Asymmetric Dark Matter (ADM), their cosmological implications and detection. While there are many models of ADM in the literature, our review of existing models will center on highlighting the few common features and important mechanisms for generation and transfer of the matter–anti-matter asymmetry between dark and visible sectors. We also survey ADM hidden sectors, the calculation of the relic abundance for ADM, and how the DM asymmetry may be erased at late times through oscillations. We consider cosmological constraints on ADM from the cosmic microwave background, neutron stars, the Sun, and brown and white dwarves. Lastly, we review indirect and direct detection methods for ADM, collider signatures, and constraints.
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
Barygenesis without grand unification
Fukugita, M., & Yanagida, T. (1986) · Physics Letters B · doi:10.1016/0370-2693(86)91126-3 · Cited by 3,879
Observational Evidence for Self-Interacting Cold Dark Matter
Spergel, D. N., & Steinhardt, P. J. (2000) · Physical Review Letters · doi:10.1103/physrevlett.84.3760 · Cited by 2,097
Beyond collisionless dark matter: Particle physics dynamics for dark matter halo structure
Tulin, S., Yu, H.-B., & Zurek, K. M. (2013) · Physical Review D · doi:10.1103/physrevd.87.115007 · Cited by 516
Self-citation
Cited by
Dark matter self-interactions and small scale structure
Tulin, S., & Yu, H.-B. (2018) · Physics Reports · doi:10.1016/j.physrep.2017.11.004 · Cited by 1,111
Search for Low-Mass Weakly Interacting Massive Particles with SuperCDMS
Agnese, R., Anderson, A. J., Asai, M., Balakishiyeva, D., Basu Thakur, R., Bauer, D. A., Beaty, J., Billard, J., Borgland, A., Bowles, M. A., et al. (2014) · Physical Review Letters · doi:10.1103/physrevlett.112.241302 · Cited by 517
Cosmic microwave background limits on accreting primordial black holes
Ali-Haïmoud, Y., & Kamionkowski, M. (2017) · Physical Review D · doi:10.1103/physrevd.95.043534 · Cited by 454
Long-lived particles at the energy frontier: the MATHUSLA physics case
Curtin, D., Drewes, M., McCullough, M., Meade, P., Mohapatra, R. N., Shelton, J., Shuve, B., Accomando, E., Alpigiani, C., Antusch, S., et al. (2019) · Reports on Progress in Physics · doi:10.1088/1361-6633/ab28d6 · Cited by 384
Self-citationLight dark matter: Models and constraints
Knapen, S., Lin, T., & Zurek, K. M. (2017) · Physical Review D · doi:10.1103/physrevd.96.115021 · Cited by 371
Self-citation
Metadata
- Authors
- Zurek, K. M.
- Venue
- Physics Reports
- Publisher
- Elsevier BV
- Published
- 2014-04
- Volume
- 537
- Issue
- 3
- Pages
- 91-121
- ISSN
- 0370-1573 (ISSN-L)
- OpenAlex
- W2114165334
- Cited by
- 541
- References
- 3
- FWCI
- 17.79
- 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: Asymmetric Dark Matter: Theories, signatures, and constraints. https://app.cochat.ai/papers/10.1016/j.physrep.2013.12.001
- The paper
- Zurek, K. M. (2014). Asymmetric Dark Matter: Theories, signatures, and constraints. Physics Reports. https://doi.org/10.1016/j.physrep.2013.12.001
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.
