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Lepto-axiogenesis with light right-handed neutrinos

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arxiv 2402.10263 v1 pith:3DNXFSPW submitted 2024-02-15 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords lepto-axiogenesisbaryonmassneutrinoright-handedasymmetrydownequilibrium
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We study lepto-axiogenesis in theories where the right-handed neutrino is light enough that its dynamics affect the determination of the baryon asymmetry. When compared with theories of high-scale lepto-axiogenesis where the Majorana neutrino mass may be treated as an effective dimension-five operator, we find that the predicted saxion mass is lower. Two distinct scenarios emerge. In the first, processes that generate the baryon asymmetry are in equilibrium down to the mass of the right-handed neutrino. In the second, the relevant processes never reach equilibrium; the baryon number freezes in. We comment on implications for supersymmetric spectra and discuss constraints on late decays of supersymmetric relics and from dark radiation. In contrast to high-scale lepto-axiogenesis, which predicts superpartners with masses of 10-100 TeV or more, we find this scenario is consistent with a wider range of superpartner masses, all the way down to current direct search bounds.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Dark Matter and Baryon Asymmetry from Monopole-Axion Interactions

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    A rotating QCD axion dissipates kinetic energy via dark monopole dyon transitions, explaining dark matter and baryon asymmetry with a predicted axion decay constant below 10^9 GeV.

  2. Flipped Rotating Axion Non-minimally Coupled to Gravity: Baryogenesis and Dark Matter

    hep-ph 2025-02 conditional novelty 4.0 of 10

    A rotating axion, kicked into motion by a sign flip in its gravitational effective potential during kination, can co-generate baryon asymmetry and dark matter in a Majoron seesaw model.

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