Evolution of Neutrino Mass-Mixing Parameters in Matter with Non-Standard Interactions
arXiv:2103.13431 · doi:10.1007/JHEP11(2021)094
Abstract
We explore the role of matter effect in the evolution of neutrino oscillation parameters in the presence of lepton-flavor-conserving and lepton-flavor-violating neutral-current non-standard interactions (NSI) of the neutrino. We derive simple approximate analytical expressions showing the evolution/running of mass-mixing parameters in matter with energy in the presence of standard interactions (SI) and SI+NSI (considering both positive and negative values of real NSI parameters). We observe that only the NSI parameters in the (2,3) block, namely and affect the running of . Though all the NSI parameters influence the evolution of , and show a stronger impact at the energies relevant for DUNE. quickly approaches to with increasing energy in both SI and SI+NSI cases. The change in is quite significant as compared to both in SI and SI+NSI frameworks. Flipping the signs of the NSI parameters alters the way in which mass-mixing parameters run with energy. We demonstrate the utility of our approach in addressing several important features related to neutrino oscillation such as: a) unraveling interesting degeneracies between and NSI parameters, b) estimating the resonance energy in presence of NSI when in matter becomes maximal, c) figuring out the required baselines and energies to have maximal matter effect in transition in the presence of different NSI parameters, and d) studying the impact of NSI parameters and on the survival probability.
arXiv comment37 pages, 13 figures, 2 tables. Comments are welcome
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