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A Dark Matter Candidate with New Strong Interactions

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arxiv hep-ph/0506015 v3 pith:6EKSHJHV submitted 2005-06-02 hep-ph astro-phhep-th

T. Banks , J. D. Mason , D. O'Neil This is my paper · ORCID
classification hep-phastro-phhep-th
keywords darkmattercosmologicalparticletheoryappropriateasymmetrybaryon
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We study the possibility that dark matter is a baryon of a new strongly interacting gauge theory, which was introduced in the low energy theory of Cosmological SUSY Breaking (CSB). This particle can fit the observed dark matter density if an appropriate cosmological asymmetry is generated. The same mechanism can also explain the dark/baryonic matter ratio in the universe. The mass of the dark matter particle is in the multiple TeV range, and could be as high as 20 TeV.

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Cited by 1 Pith paper

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  1. Rich Phenomenology from Simple Ingredients: A Review of Confining Dark Sectors

    hep-ph 2026-06 unverdicted novelty 2.0 of 10

    Review of confining dark sectors summarizing dark matter candidates, abundance mechanisms, discovery channels, and applications to the abundance similarity puzzle.

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