Hint of non-standard dynamics in solar neutrino conversion
arXiv:1101.3875 · doi:10.1103/PhysRevD.83.101701
Abstract
Motivated by the recent low-threshold measurements of the solar 8B neutrino spectrum performed by Borexino, Super-Kamiokande and the Sudbury Neutrino Observatory -- all now monitoring the transition regime between low-energy (vacuum-like) and high-energy (matter-dominated) flavor conversions -- we consider the role of sub-dominant dynamical terms induced by new flavor-changing interactions. We find that the presence of such perturbations with strength ~ 0.1 G_F is now favored, offering a better description of the anomalous behavior suggested by the new results, whose spectrum shows no sign of the typical low-energy upturn predicted by the standard MSW mechanism. Our findings, if interpreted in a 2-flavor scheme, provide a hint of such new interactions at the ~ 2 sigma level, which is rather robust with respect to 3-flavor effects possibly induced by non-zero theta_13.
5 pages, 4 figures; one figure added; minor changes in the text; references added; matches version published in PRD (Rapid Communications)
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Cited by in corpus (9)
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- Degeneracy between octant and neutrino non-standard interactions at DUNE
- Neutrino oscillations: the rise of the PMNS paradigm
- Testing the very-short-baseline neutrino anomalies at the solar sector
- Solar neutrino physics with low-threshold dark matter detectors
- Neutrino oscillations and Non-Standard Interactions
- Searching for Axial Neutral Current Non-Standard Interactions of neutrinos by DUNE-like experiments
- Non-standard interactions from the future neutrino solar sector