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How heavy can dark matter be? Constraining colourful unitarity with SARAH

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arxiv 2012.09022 v2 pith:EF4PYPKX submitted 2020-12-16 hep-ph

Mark D. Goodsell , Rhea Moutafis This is my paper · ORCID
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keywords darkmattercolourfulconstraintssarahunitarityalongapply
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We describe the automation of the calculation of perturbative unitarity constraints including scalars that have colour charges, and its release in SARAH 4.14.4. We apply this, along with vacuum stability constraints, to a simple dark matter model with colourful mediators and interesting decays, and show how it leads to a bound on a thermal relic dark matter mass well below the classic Griest-Kamionkowski limit.

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  1. Unveiling the inert Triplet desert region with a pNGB Dark Matter and its Gravitational Wave signatures

    hep-ph 2025-05 conditional novelty 6.0 of 10

    A two-component dark matter model combining an inert scalar triplet with a pseudo-Goldstone singlet revives the sub-TeV triplet desert region and predicts gravitational waves detectable by LISA, BBO, and DECIGO.

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