A strongly interacting massive particle (SIMP) is a hypothetical particle that
interacts strongly between themselves and
weakly with ordinary matter, but could form the inferred
dark matter despite this.[1][2][3]
^
Wandelt, Benjamin D; Dave, Romeel; Farrar, Glennys R; McGuire, Patrick C; Spergel, David N; Steinhardt, Paul J (2000), "Self-Interacting Dark Matter", in Cline, David B (ed.), Sources and Detection of Dark Matter and Dark Energy in the Universe, Springer-Verlag, p. 263,
arXiv:astro-ph/0006344,
Bibcode:
2001sddm.symp..263W,
ISBN978-3-540-41216-8
^
Massey, Richard; et al. (2017), "Dark matter dynamics in Abell 3827: new data consistent with standard Cold Dark Matter", Monthly Notices of the Royal Astronomical Society, 477 (1): 669–677,
arXiv:1708.04245,
Bibcode:
2018MNRAS.477..669M,
doi:
10.1093/mnras/sty630
^
McGuire, Patrick C; Steinhardt, Paul J (2001), "Cracking Open the Window for Strongly Interacting Massive Particles as the Halo Dark Matter", Proceedings of the International Cosmic Ray Conference, vol. 4, Hamburg, Germany, p. 1566,
arXiv:astro-ph/0105567,
Bibcode:
2001ICRC....4.1566M{{
cite book}}: CS1 maint: location missing publisher (
link)
A strongly interacting massive particle (SIMP) is a hypothetical particle that
interacts strongly between themselves and
weakly with ordinary matter, but could form the inferred
dark matter despite this.[1][2][3]
^
Wandelt, Benjamin D; Dave, Romeel; Farrar, Glennys R; McGuire, Patrick C; Spergel, David N; Steinhardt, Paul J (2000), "Self-Interacting Dark Matter", in Cline, David B (ed.), Sources and Detection of Dark Matter and Dark Energy in the Universe, Springer-Verlag, p. 263,
arXiv:astro-ph/0006344,
Bibcode:
2001sddm.symp..263W,
ISBN978-3-540-41216-8
^
Massey, Richard; et al. (2017), "Dark matter dynamics in Abell 3827: new data consistent with standard Cold Dark Matter", Monthly Notices of the Royal Astronomical Society, 477 (1): 669–677,
arXiv:1708.04245,
Bibcode:
2018MNRAS.477..669M,
doi:
10.1093/mnras/sty630
^
McGuire, Patrick C; Steinhardt, Paul J (2001), "Cracking Open the Window for Strongly Interacting Massive Particles as the Halo Dark Matter", Proceedings of the International Cosmic Ray Conference, vol. 4, Hamburg, Germany, p. 1566,
arXiv:astro-ph/0105567,
Bibcode:
2001ICRC....4.1566M{{
cite book}}: CS1 maint: location missing publisher (
link)