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Leptogenesis origin of Dirac gaugino dark matter

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arxiv 1009.0983 v3 pith:ORE5RSQN submitted 2010-09-06 hep-ph astro-ph.CO

Leptogenesis origin of Dirac gaugino dark matter

classification hep-ph astro-ph.CO
keywords diracdarkmattercouplingsgauginoheavyhiggshiggsinos
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The Dirac nature of the gauginos (and also the Higgsinos) can be realized in $R$-symmetric supersymmetry models. In this class of models, the Dirac bino (or wino) with a small mixture of the Dirac Higgsinos is a good dark matter candidate. When the seesaw mechanism with Higgs triplet superfields is implemented to account for the neutrino masses and mixing, the leptogenesis driven by the heavy triplet decay is shown to produce not only the matter-antimatter asymmetry but also the asymmetric relic density of the Dirac gaugino dark matter. The dark matter mass turns out to be controlled by the Yukawa couplings of the heavy Higgs triplets, and it can be naturally at the weak scale for a mild hierarchy of the Yukawa couplings.

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Cited by 2 Pith papers

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    A gauged SO(3) flavour symmetry broken at multiple scales generates SM fermion masses, redistributes a lepton asymmetry into baryon and dark matter asymmetries via sphalerons, and yields dark matter as bound states of...

  2. Gauged Flavour for Asymmetric Dark Matter

    hep-ph 2026-05 unverdicted novelty 5.0

    A gauged SO(3) flavour symmetry spontaneously broken at multiple scales links SM flavour hierarchies to asymmetric dark matter via leptogenesis and sphaleron redistribution, with DM as bound states of a confining SU(3).