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Cited by 1,111Dark Matter and Cosmic PhenomenaGalaxies: Formation, Evolution, PhenomenaCosmology and Gravitation Theories

Dark matter self-interactions and small scale structure

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Tulin, Sean, Yu, Hai-Bo·2018·Physics Reports
DOI 10.1016/j.physrep.2017.11.004
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  • Such models naturally predict self-interactions that can be many orders of magnitude larger than those between dark and visible matter, making the self-interaction cross section a unique window into the physics of the dark sector.

    “Such models naturally predict self-interactions that can be many orders of magnitude larger than those between dark and visible matter, making the SICS a unique window into the physics of the dark sector (S.Tulin & H. Yu 2018).”

    From A New Robust Constraint on the Self-interaction Cross Section of Dark Matter with Double Radio Relic Clusters (2026) · cites this paper as S.Tulin & H. Yu 2018

    The Summary (p. 70) says self-interactions are a general feature of hidden-sector models and that their strength depends on dark-sector scales. “From astrophysics to particle theory” (p. 12) says dark–visible coupling must be much weaker than in WIMP models and describes probes of SIDM. Neither passage establishes the claimed many-orders-of-magnitude comparison between self-interaction and dark–visible interaction cross sections. (LLM, conf=0.84)

    Experimental — accuracy not yet measured

  • Persistent discrepancies on small scales, such as the core-cusp and too-big-to-fail problems, suggest that dark matter may possess a nonzero self-interaction cross section.

    “However, persistent discrepancies on small scales, such as the core-cusp and too-big-to-fail problems, suggest that dark matter (DM) may possess a nonzero self-interaction cross section (SICS) (D.N. Spergel & P. J. Steinhardt 2000; S. Tulin & H. Yu 2018).”

    From A New Robust Constraint on the Self-interaction Cross Section of Dark Matter with Double Radio Relic Clusters (2026) · cites this paper as S. Tulin & H. Yu 2018

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Authors
Tulin, S., & Yu, H.-B.
Affiliations
  • York University (CA)
  • University of California, Riverside (US)
Corresponding author
Tulin, Sean
ORCID
Venue
Physics Reports
Publisher
Elsevier BV
Published
2018-02
Volume
730
Pages
1-57
ISSN
0370-1573 (ISSN-L)
DOI
10.1016/j.physrep.2017.11.004
OpenAlex
W2612559938
Cited by
1,111
References
10
Citations by year
2026: 130 · 2025: 149 · 2024: 124 · 2023: 120 · 2022: 130 · 2021: 126 · 2020: 111 · 2019: 128 · 2018: 81 · 2017: 9
FWCI
41.77
Type
journal article
Language
en
Open access
Licence
Locations
  • Physics Reports (acceptedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • Natural Science and Engineering Research Council of Canada
  • U.S. Department of Energy (de-sc0008541 (HBY))
  • Hellman Fellows Fund (HBY)
Topics
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
Keywords
self-interacting dark matter, small-scale structure, core-cusp problem, missing satellites problem, too big to fail, rotation curves, galaxy formation, dark matter halos, halo substructure, cluster mergers, Bullet Cluster, composite dark matter, dark matter direct detection, indirect dark matter detection, N-body simulations

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