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6533b859fe1ef96bd12b6f6c

RESEARCH PRODUCT

Dirac neutrinos from Peccei-Quinn symmetry: a fresh look at the axion

Mario ReigMario ReigEduardo PeinadoRahul SrivastavaRahul SrivastavaJosé W. F. Valle

subject

High Energy Physics - TheoryJob creationPhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyLibrary scienceFOS: Physical sciencesAstronomy and Astrophysics01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)0103 physical sciencesChristian ministryHigh Energy Physics::Experiment010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics

description

We show that a very simple solution to the strong CP problem naturally leads to Dirac neutrinos. Small effective neutrino masses emerge from a type-I Dirac seesaw mechanism. Neutrino mass limits probe the axion parameters in regions currently inaccessible to conventional searches.

yearjournalcountryeditionlanguage
2019-10-07
https://dx.doi.org/10.48550/arxiv.1910.02961
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