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Neutrino Masses and Leptogenesis with Heavy Higgs Triplets

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arxiv hep-ph/9802445 v2 pith:UGUK6HUQ submitted 1998-02-27 hep-ph

classification hep-ph
keywords electroweakheavyhiggsleptogenesismassesneutrinotripletsaddition
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A simple and economical extension of the minimal standard electroweak gauge model (without right-handed neutrinos) by the addition of two heavy Higgs scalar triplets would have two significant advantages. \underline {Naturally} small Majorana neutrino masses would become possible, as well as leptogenesis in the early universe which gets converted at the electroweak phase transition into the present observed baryon asymmetry.

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Cited by 4 Pith papers

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

  1. Thermal Leptogenesis in the BNT Model of Neutrino Mass

    hep-ph 2026-08 conditional novelty 6.0 of 10

    In the BNT neutrino-mass model, thermal leptogenesis can explain the observed baryon asymmetry with triplet masses above roughly 3.5e7 GeV in the hierarchical case and as low as 1.7 TeV with resonant enhancement.

  2. The mass-coupling effect in leptogenesis

    hep-ph 2025-09 conditional novelty 6.0 of 10

    In weak-washout heavy-particle decay leptogenesis, the lepton asymmetry is approximately independent of the decaying particle mass and the couplings of thermalized decay products, because the nonthermal distribution s...

  3. Gravitational Wave Probe of Singlet-Doublet Dark Matter Induced Radiative Neutrino Mass

    hep-ph 2025-11 conditional novelty 5.0 of 10

    A radiative-seesaw model with singlet-doublet dark matter can satisfy neutrino, muon, flavor, relic, and direct-detection constraints while producing a first-order electroweak phase transition with gravitational waves...

  4. Type II Seesaw Leptogenesis in a Majoron background

    hep-ph 2025-06 unverdicted novelty 5.0 of 10

    Spontaneous wash-in leptogenesis in Type II Seesaw with Majoron pNGB background enables baryon asymmetry generation alongside dark matter cogenesis for specific v_T, v_sigma and m_j ranges.

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