Dirac Neutrinos, Dark Energy and Baryon Asymmetry
arXiv:0705.3736 · doi:10.1088/1475-7516/2007/11/016
Abstract
We explore a new origin of neutrino dark energy and baryon asymmetry in the universe. The neutrinos acquire small masses through the Dirac seesaw mechanism. The pseudo-Nambu-Goldstone boson associated with neutrino mass-generation provides a candidate for dark energy. The puzzle of cosmological baryon asymmetry is resolved via neutrinogenesis.
arXiv comment6 pages, 1 figure. Accepted by JCAP (only minor rewordings, refs added)
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Cited by in corpus (22)
- Radiative Neutrino Mass, Dark Matter and Leptogenesis
- Naturally Small Dirac Neutrino Mass with Intermediate Multiplet Fields
- Extended Zee model for Neutrino Mass, Leptogenesis and Sterile Neutrino like Dark Matter
- Alternative formulation of left-right symmetry with conservation and purely Dirac neutrinos
- Realistic Neutrinogenesis with Radiative Vertex Correction
- Neutrinoless Double- Decay with Nonstandard Majoron Emission
- Neutrino Condensate as Origin of Dark Energy
- Peccei-Quinn symmetry for Dirac seesaw and leptogenesis
- Dirac neutrinos and anomaly-free discrete gauge symmetries
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- Majorana Neutrino Superfluidity and Stability of Neutrino Dark Energy
- Precise predictions for Dirac neutrino mixing
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- Left-Right Symmetric Model of Neutrino Dark Energy
- Baryogenesis from Hierarchical Dirac Neutrinos
- False Vacuum in the Supersymmetric Mass Varying Neutrinos Model
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- Avoiding parameter fine-tuning in mass varying neutrino models of DE?
- Neutrino Dark Energy in Grand Unified Theories
- Oscillation in Orbifold GUT