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dc.creatorFanchi, John R.
dc.date.accessioned2019-07-12T16:01:55Z
dc.date.available2019-07-12T16:01:55Z
dc.date.issued2017-05-01
dc.identifier.urihttps://doi.org/10.1088/1742-6596/845/1/012027
dc.identifier.urihttps://repository.tcu.edu/handle/116099117/26415
dc.description.abstractMass state transitions are a key feature of parametrized relativistic dynamics (PRD). PRD is a manifestly covariant quantum theory with invariant evolution parameter. The theory has been applied to neutrino flavor oscillations between two mass states. It is generalized to transitions between three mass states and applied to the survival of electron neutrinos. The analysis shows that significant differences exist between theoretical results of the conventional model and the PRD model.en_US
dc.description.statementofresponsibilityFanchi (ENGR)
dc.language.isoen
dc.publisherIOP Publishing
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/
dc.sourceJournal of Physics: Conference Series
dc.source.urihttps://iopscience.iop.org/article/10.1088/1742-6596/845/1/012027
dc.subjectsolar neutrinos
dc.subjectexistence
dc.subjectcharge
dc.subjectparticles
dc.subjectrays
dc.titleParametrized relativistic dynamical framework for neutrino oscillations
dc.typeArticleen_US
dc.rights.holderJohn R. Fanchi et al.
dc.rights.licenseCC BY 3.0
local.collegeCollege of Science and Engineering
local.departmentEngineering


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