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arxiv: 1809.06003 · v1 · submitted 2018-09-17 · ✦ hep-ph · astro-ph.CO

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Dibaryons cannot be the dark matter

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classification ✦ hep-ph astro-ph.CO
keywords darkmattercannotdibaryondibaryonshadronabundanceabundances
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The hypothetical $SU(3)$ flavor-singlet dibaryon state $S$ with strangeness $-2$ has been discussed as a dark-matter candidate capable of explaining the curious 5-to-1 ratio of the mass density of dark matter to that of baryons. We study the early-universe production of dibaryons and find that irrespective of the hadron abundances produced by the QCD quark/hadron transition, rapid particle reactions thermalized the $S$ abundance, and it tracked equilibrium until it "froze out" at a tiny value. For the plausible range of dibaryon masses (1860 - 1890 MeV) and generous assumptions about its interaction cross sections, $S$'s account for at most $10^{-11}$ of the baryon number, and thus cannot be the dark matter. Although it is not the dark matter, if the $S$ exists it might be an interesting relic.

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Cited by 1 Pith paper

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