Combined effect of NSI and SFP on solar electron neutrino oscillation

Abstract

The combined effect of SFP and the non standard neutrino interaction (NSI) on the survival probability of solar electron neutrinos (assumed to be Dirac particles) is examined for various values of ${\epsilon }_{11}$, ${\epsilon }_{12}$ and $\mu B$. It is found that the neutrino survival probability curves affected by SFP and NSI effects individually for some values of the parameters (${\epsilon }_{11}$, ${\epsilon }_{12}$ and $\mu B$) get close to the standard MSW curve when both effects are combined. Therefore, the combined effect of SFP and NSI needs to be taken into account when the solar electron neutrino data obtained by low energy solar neutrino experiments is investigated.

11 pages, 3 figures, published version

References in corpus (9)

• Status of non-standard neutrino interactions
• Non standard neutrino interactions
• Search of Neutrino Magnetic Moments with a High-Purity Germanium Detector at the Kuo-Sheng Nuclear Power Station
• Loop bounds on non-standard neutrino interactions
• The Daya Bay and T2K results on ${\sin }^{2}2{\theta }_{13}$ and Non-Standard Neutrino Interactions
• Neutrino magnetic moment: a window to new physics
• Neutrino transition magnetic moments within the non-standard neutrino-nucleus interactions
• Light sterile neutrinos, spin flavour precession and the solar neutrino experiments
• Model Independent Naturalness Bounds on Magnetic Moments of Majorana Neutrinos

Cited by in corpus (1)

• Neutrino spin-flavor oscillations in solar environment