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Neutrino oscillations and non-standard Interactions

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Neutrino oscillations and non-standard Interactions

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dc.contributor.author Farzan, Yasaman
dc.contributor.author Tórtola Baixauli, María Amparo
dc.date.accessioned 2019-05-07T12:53:29Z
dc.date.available 2019-05-07T12:53:29Z
dc.date.issued 2018
dc.identifier.citation Farzan, Yasaman Tórtola Baixauli, María Amparo 2018 Neutrino oscillations and non-standard Interactions Frontiers in physics (Lausanne) 6 10 1 34
dc.identifier.uri http://hdl.handle.net/10550/70099
dc.description.abstract Current neutrino experiments are measuring the neutrino mixing parameters with an unprecedented accuracy. The upcoming generation of neutrino experiments will be sensitive to subdominant neutrino oscillation effects that can in principle give information on the yet-unknown neutrino parameters: the Dirac CP-violating phase in the PMNS mixing matrix, the neutrino mass ordering and the octant of θ23. Determining the exact values of neutrino mass and mixing parameters is crucial to test various neutrino models and flavor symmetries that are designed to predict these neutrino parameters. In the first part of this review, we summarize the current status of the neutrino oscillation parameter determination. We consider the most recent data from all solar neutrino experiments and the atmospheric neutrino data from Super-Kamiokande, IceCube, and ANTARES. We also implement the data from the reactor neutrino experiments KamLAND, Daya Bay, RENO, and Double Chooz as well as the long baseline neutrino data from MINOS, T2K, and NOνA. If in addition to the standard interactions, neutrinos have subdominant yet-unknown Non-Standard Interactions (NSI) with matter fields, extracting the values of these parameters will suffer from new degeneracies and ambiguities. We review such effects and formulate the conditions on the NSI parameters under which the precision measurement of neutrino oscillation parameters can be distorted. Like standard weak interactions, the non-standard interaction can be categorized into two groups: Charged Current (CC) NSI and Neutral Current (NC) NSI. Our focus will be mainly on neutral current NSI because it is possible to build a class of models that give rise to sizeable NC NSI with discernible effects on neutrino oscillation. These models are based on new U(1) gauge symmetry with a gauge boson of mass ≲ 10 MeV. The UV complete model should be of course electroweak invariant which in general implies that along with neutrinos, charged fermions also acquire new interactions on which there are strong bounds. We enumerate the bounds that already exist on the electroweak symmetric models and demonstrate that it is possible to build viable models avoiding all these bounds. In the end, we review methods to test these models and suggest approaches to break the degeneracies in deriving neutrino mass parameters caused by NSI.
dc.language.iso eng
dc.relation.ispartof Frontiers in physics (Lausanne), 2018, vol. 6, num. 10, p. 1-34
dc.subject Partícules (Física nuclear)
dc.subject Violació CP (Física nuclear)
dc.title Neutrino oscillations and non-standard Interactions
dc.type journal article es_ES
dc.date.updated 2019-05-07T12:53:29Z
dc.identifier.doi 10.3389/fphy.2018.00010
dc.identifier.idgrec 129980
dc.rights.accessRights open access es_ES

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