English

Reshuffled Strongly Interacting Massive Particle Dark Matter

High Energy Physics - Phenomenology 2022-06-14 v2 Cosmology and Nongalactic Astrophysics High Energy Physics - Theory

Abstract

In this work, we reanalyze the multi-component strongly interacting massive particle (mSIMP) scenario using an effective operator approach. As in the single-component SIMP case, the total relic abundance of mSIMP dark matter (DM) is determined by the coupling strengths of 323 \to 2 processes achieved by a five-point effective operator. Intriguingly, we notice that there is an irreducible 222 \to 2 process induced by the corresponding five-point interaction in the dark sector, which would reshuffle the mass densities of SIMP DM after the chemical freeze-out. We dub this DM scenario as reshuffled SIMP (rrSIMP). Given this observation, we then numerically solve the coupled Boltzmann equations including the 323 \to 2 and 222 \to 2 processes to get the correct yields of rrSIMP DM. It turns out that the masses of rrSIMP DM must be nearly degenerate for them to contribute sizable abundances. On the other hand, we also introduce effective operators to bridge the dark sector and visible sector via a vector portal coupling. Notably, we find that the reshuffled mechanism in the rrSIMP scenario is sensitive to the size of the DM self-interacting cross section.

Cite

@article{arxiv.2107.04375,
  title  = {Reshuffled Strongly Interacting Massive Particle Dark Matter},
  author = {Shu-Yu Ho and Pyungwon Ko and Chih-Ting Lu},
  journal= {arXiv preprint arXiv:2107.04375},
  year   = {2022}
}

Comments

8 pages, 3 figures, 3 tables, the title changed. Matches the version published in Phys.Dark Univ

R2 v1 2026-06-24T04:02:20.040Z