Non standard neutrino interactions: current status and future prospects

Neutrino oscillations have become well-known phenomena; the measurements of neutrino mixing angles and mass squared differences are continuously improving. Future oscillation experiments will eventually determine the remaining unknown neutrino parameters, namely, the mass ordering, normal or inverte...

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Main Authors: O G Miranda, H Nunokawa
Format: Article
Language:English
Published: IOP Publishing 2015-01-01
Series:New Journal of Physics
Subjects:
Online Access:https://doi.org/10.1088/1367-2630/17/9/095002
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author O G Miranda
H Nunokawa
author_facet O G Miranda
H Nunokawa
author_sort O G Miranda
collection DOAJ
description Neutrino oscillations have become well-known phenomena; the measurements of neutrino mixing angles and mass squared differences are continuously improving. Future oscillation experiments will eventually determine the remaining unknown neutrino parameters, namely, the mass ordering, normal or inverted, and the CP-violating phase. On the other hand, the absolute mass scale of neutrinos could be probed by cosmological observations, single beta decay as well as by neutrinoless double beta decay experiments. Furthermore, the last one may shed light on the nature of neutrinos, Dirac or Majorana, by measuring the effective Majorana mass of neutrinos. However, the neutrino mass generation mechanism remains unknown. A well-motivated phenomenological approach to search for new physics, in the neutrino sector, is that of non-standard interactions. In this short review, the current constraints in this picture, as well as the perspectives from future experiments, are discussed.
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spelling doaj.art-90bebfe37ff341ae8dbd98d6a6a2bdbd2023-08-08T14:23:53ZengIOP PublishingNew Journal of Physics1367-26302015-01-0117909500210.1088/1367-2630/17/9/095002Non standard neutrino interactions: current status and future prospectsO G Miranda0H Nunokawa1Departamento de Física, Centro de Investigación y de Estudios Avanzados del IPN , Apdo. Postal 14-740 07000 México, D F, MéxicoDepartamento de Física, Pontifícia Universidade Católica do Rio de Janeiro , C. P. 38071, 22452-970, Rio de Janeiro, BrazilNeutrino oscillations have become well-known phenomena; the measurements of neutrino mixing angles and mass squared differences are continuously improving. Future oscillation experiments will eventually determine the remaining unknown neutrino parameters, namely, the mass ordering, normal or inverted, and the CP-violating phase. On the other hand, the absolute mass scale of neutrinos could be probed by cosmological observations, single beta decay as well as by neutrinoless double beta decay experiments. Furthermore, the last one may shed light on the nature of neutrinos, Dirac or Majorana, by measuring the effective Majorana mass of neutrinos. However, the neutrino mass generation mechanism remains unknown. A well-motivated phenomenological approach to search for new physics, in the neutrino sector, is that of non-standard interactions. In this short review, the current constraints in this picture, as well as the perspectives from future experiments, are discussed.https://doi.org/10.1088/1367-2630/17/9/095002neutrino interactionsphysics beyond the standar modelneutrino mixing
spellingShingle O G Miranda
H Nunokawa
Non standard neutrino interactions: current status and future prospects
New Journal of Physics
neutrino interactions
physics beyond the standar model
neutrino mixing
title Non standard neutrino interactions: current status and future prospects
title_full Non standard neutrino interactions: current status and future prospects
title_fullStr Non standard neutrino interactions: current status and future prospects
title_full_unstemmed Non standard neutrino interactions: current status and future prospects
title_short Non standard neutrino interactions: current status and future prospects
title_sort non standard neutrino interactions current status and future prospects
topic neutrino interactions
physics beyond the standar model
neutrino mixing
url https://doi.org/10.1088/1367-2630/17/9/095002
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