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Self-Interacting Dark Matter

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arxiv astro-ph/0006344 v2 pith:H5H6ELR5 submitted 2000-06-24 astro-ph

classification astro-ph
keywords matterdarkdiscussaddressallowedanalysisbaryoniccollisionless
verification ladder T0 review T1 audit T2 compute T3 formal
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Spergel and Steinhardt have recently proposed the concept of dark matter with strong self-interactions as a means to address numerous discrepancies between observations of dark matter halos on subgalactic scales and the predictions of the standard collisionless dark matter picture. We review the motivations for this scenario and discuss some recent, successful numerical tests. We also discuss the possibility that the dark matter interacts strongly with ordinary baryonic matter, as well as with itself. We present a new analysis of the experimental constraints and re-evaluate the allowed range of cross-section and mass.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Search for soft unclustered energy patterns containing muons in the final state in $pp$ collisions at $\sqrt{s}$ = 13 TeV with the ATLAS detector

    hep-ex 2026-05 unverdicted novelty 6.0 of 10

    No significant excess observed in search for SUEP signatures with muons; exclusion limits set on mediator cross section times branching fraction down to 0.05 fb at 750 GeV.

  2. Searching for Dark Matter with MeVCube

    hep-ph 2025-01 conditional novelty 4.0 of 10

    Using Fisher forecasting, the author shows that a 2U to 12U MeVCube CubeSat could probe new dark matter parameter space for evaporating primordial black holes and MeV-scale decaying or annihilating dark matter.

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