Non-thermal production via late-decaying reheatons can achieve the observed dark matter density for sexaquarks by controlling branching fractions and coalescence probabilities, unlike thermal freeze-out which underproduces them by many orders of magnitude.
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In a constituent quark model, only baryon-baryon-like configurations of the uuddss system produce near-threshold states appearing as loosely bound three-quark clusters.
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Non-Thermal Production of Sexaquark Dark Matter
Non-thermal production via late-decaying reheatons can achieve the observed dark matter density for sexaquarks by controlling branching fractions and coalescence probabilities, unlike thermal freeze-out which underproduces them by many orders of magnitude.
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Sexaquarks and $H$ dibaryons in the $uuddss$ system: a comparison within a constituent quark model
In a constituent quark model, only baryon-baryon-like configurations of the uuddss system produce near-threshold states appearing as loosely bound three-quark clusters.