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RESEARCH PRODUCT
Resurrection of large lepton number asymmetries from neutrino flavor oscillations
William H. KinneyWan-il ParkGabriela Barenboimsubject
PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and Detectors010308 nuclear & particles physicsHigh Energy Physics::LatticeAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciences01 natural sciencesLepton numberNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesis0103 physical sciencesMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationFlavorAstrophysics - Cosmology and Nongalactic Astrophysicsdescription
We numerically solve the evolution equations of neutrino three-flavor density matrices, and show that, even if neutrino oscillations mix neutrino flavors, large lepton number asymmetries are still allowed in certain limits by Big Bang Nucleosynthesis (BBN).
year | journal | country | edition | language |
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2016-09-06 | Physical Review D |