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{{shortShort description|Hypothetical particles that interact strongly with ordinary matter, but could form the inferred dark matter despite thisparticle}}
A '''Stronglystrongly interacting massive particlesparticle''' (SIMPs)'''SIMP''') areis a hypothetical particlesparticle that [[strong interaction|interactinteracts strongly]] between themselves and [[Weak interaction|weakly]] with ordinary matter, but could form the inferred [[dark matter]] despite this.<ref name="wand">
{{cite book
|last1=Wandelt |first1=Benjamin D
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|bibcode=2001sddm.symp..263W
|isbn=978-3-540-41216-8
}}</ref><ref>
}}</ref> However, this finding has since been discounted based on further observations and modelling of the cluster.<ref>
{{cite journal
|last1=Massey |first1=Richard
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|mode=cs2
|doi=10.1093/mnras/sty630
|doi-access=free
|bibcode=2018MNRAS.477..669M
}}</ref><ref>{{cite web
|last1=Grossman
{{cite web
|last1=Grossman |first1=Lisa
|date=April 5, 2018
|title=Dark matter isn't interacting with itself after all
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|work=ScienceNews
|access-date=2018-04-05
|archive-date=2018-04-06
|archive-url=https://web.archive.org/web/20180406013104/https://www.sciencenews.org/article/dark-matter-isnt-interacting-itself-after-all
|url-status=live
}}</ref>
 
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|volume=59 |issue=1 |page=015021
|arxiv=hep-ph/9805288
|bibcode=1999PhRvD1998PhRvD..59a5021A
|doi=10.1103/PhysRevD.59.015021
|mode=cs2
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|pmid=10012303
|mode=cs2
|url=httphttps://cds.cern.ch/record/212913
}}</ref><ref name="cyb">
{{Cite journal
|last1=Cyburt |first1=Richard H
|last2=Fields |first2=Brian D
|last3=Pavlidou |first3=Vasiliki| authorlink3=Vasiliki Pavlidou
|last4=Wandelt |first4=Benjamin D
|year=2002
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|chapter=Cracking Open the Window for Strongly Interacting Massive Particles as the Halo Dark Matter
|title=Proceedings of the International Cosmic Ray Conference
|journal=International Cosmic Ray Conference
|volume=4
|___location=Hamburg, Germany
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