Self-Interacting Dark Matter

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dc.creatorWandelt, Benjamin D.
dc.creatorDave, Romeel
dc.creatorFarrar, Glennys R.
dc.creatorMcGuire, Patrick C.
dc.creatorSpergel, David N.
dc.creatorSteinhardt, Paul J.
dc.date2000-06-24
dc.date2000-06-28
dc.date.accessioned2026-07-07T01:54:07Z
dc.date.available2026-07-07T01:54:07Z
dc.descriptionSpergel 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.
dc.description12 pages, 3 figures; minor typos corrected. To appear in Proceedings of Dark Matter 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0006344
dc.identifierhttp://arxiv.org/abs/astro-ph/0006344
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1222
dc.subjectAstrophysics
dc.titleSelf-Interacting Dark Matter
dc.typetext

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