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Yes, it stands for SIMP haha funny, but the other article (Weakly interacting massive particles) also has the abbreviation of WIMPs so SIMPs should stay for consistency reasons
Rescuing 1 sources and tagging 0 as dead.) #IABot (v2.0.9.5
 
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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''') is area hypothetical particlesparticle that [[strong interaction|interactinteracts strongly]] between themselves [looks like they scatter off each other - observation of colliding galaxies in theand [[AbellWeak 3827interaction|weakly]] cluster, where it seemed that dark matter lagged behind the ordinary matter] and 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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|journal=Monthly Notices of the Royal Astronomical Society
|volume=477
|issue=1
|pages=669–677
|arxiv=1708.04245
|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
|url=https://www.sciencenews.org/article/dark-matter-isnt-interacting-itself-after-all
|work=ScienceNews
|accessdateaccess-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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|bibcode=1998PhRvD..57.4606C
|doi=10.1103/PhysRevD.57.4606
|s2cid=44780458
|mode=cs2
}}</ref><ref name="albq">
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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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|doi=10.1103/PhysRevLett.87.061301
|pmid=11497819
|s2cid=13510283
|mode=cs2
}}</ref><ref name="chuz">
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|bibcode=2006ApJ...645..950C
|doi=10.1086/504505
|s2cid=16131656
|mode=cs2
}}</ref>
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|title=Opening the window on strongly interacting dark matter
|journal=Physical Review D
|volume=41 |issue=12 |pages=35943594–3603
|bibcode=1990PhRvD..41.3594S
|doi=10.1103/PhysRevD.41.3594
|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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|bibcode=2002PhRvD..65l3503C
|doi=10.1103/PhysRevD.65.123503
|s2cid=14926247
|mode=cs2
}}.</ref><ref name="zahar">
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|bibcode=2005PhRvD..72h3502Z
|doi=10.1103/PhysRevD.72.083502
|s2cid=39245145
|mode=cs2
}}</ref><ref name="wdn">
{{cite journal
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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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|bibcode=2004PhRvD..70j3517M
|doi=10.1103/PhysRevD.70.103517
|s2cid=53396770
|mode=cs2
}}</ref> Earth's heat flow significantly constrains any cross section.<ref>
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|bibcode=2007PhRvD..76d3523M
|doi=10.1103/PhysRevD.76.043523
|s2cid=119710504
|mode=cs2
}}</ref>
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