History of Dark Matter
Open accessAbstract
The standard model of modern cosmology is unthinkable without dark matter, although direct detections are still missing. A broad perspective of how dark matter was postulated and became accepted is presented, from prehistory, over observations of galaxy clusters, galaxy rotation curves, the search for baryonic dark matter, possible alternative explanations via modified gravity, up to the hunt for dark matter particles. The interplay is described between observational discoveries and theoretical arguments which led finally to the adoption of this paradigm.
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For wimp ≃ 0 outside the bounce window, the imprint field's background and linear perturbation behavior is indistinguishable from cold dark matter (CDM).
“For wimp≃0 outside the bounce window, its background and linear perturbation behavior is indistinguishable from cold dark matter (CDM) [58].”
From Counting Cosmic Cycles: Past Big Crunches, Future Recurrence Limits, and the Age of the Quantum Memory Matrix Universe (2025) · cites this paper as [58]
The WIMP paradigm and Cosmology sections discuss cold dark matter and the growth of its density fluctuations, but do not address an imprint field. Searches for a bounce window, wimp ≃ 0, and matching background and linear perturbation behavior found no passage supporting the attributed comparison. (LLM, conf=0.76)
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“For w imp ≃ 0 outside the bounce window, its background and linear perturbation behavior is indistinguishable from cold dark matter (CDM) [58].”
- Authors
- Bertone, G., & Hooper, D.
- Affiliations
- University of Amsterdam (NL)
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- Reviews of Modern Physics
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- American Physical Society (APS)
- Published
- 2018-10-15
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- 90
- Issue
- 4
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- 1539-0756
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- en
- Open access
- bronze
- doi.org
- Licence
- Locations
- Reviews of Modern Physics (publishedVersion)
- UvA-DARE (University of Amsterdam) (publishedVersion, other-oa)
- arXiv (Cornell University) (submittedVersion)
- OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) (submittedVersion)
- Data Archiving and Networked Services (DANS) (submittedVersion, other-oa)
- Funders
- H2020 European Research Council (WIMPs Kairos)
- U.S. Department of Energy
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Keywords
- dark matter, galaxy rotation curves, galaxy clusters, baryonic dark matter, modified gravity
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 ›
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