Effect of non-standard interaction for radiative neutrino mass model

Journal Article · Fri Jul 27 00:00:00 EDT 2012 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.4742110· OSTI ID:22069123

Konishi, Y; Sato, J; Shimomura, T ^[1]

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1. Department of Physics, Saitama University, Shimo-okubo, Sakura-ku, Saitama, 338-8570 (Japan)

We examined effects of non-standard interactions (NSIs) in a radiative neutrino mass model. The radiative neutrino mass model suggested by Kraus Nasri and Trodden can explain not only neutrino flavor mixing and neutrino masses, but also dark matter relic abundance. Although the NSI effects of the model are too small to be detected by present neutrino oscillation experiments, we might observe the small effects in future experiments such as neutrino factory.

• OSTI ID: 22069123
• Journal Information: AIP Conference Proceedings, Vol. 1467, Issue 1; Conference: GUT2012: International workshop on grand unified theories, Kyoto (Japan), 15-17 Mar 2012; Other Information: (c) 2012 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
FLAVOR MODEL
GRAND UNIFIED THEORY
NEUTRINO OSCILLATION
NEUTRINOS
NONLUMINOUS MATTER
REST MASS