The Daya Bay and T2K results on $\sin^2 2 \theta_{13}$ and Non-Standard Neutrino Interactions

TL;DR

This paper demonstrates that discrepancies in measured 3 values from T2K and Daya Bay can be explained by non-standard neutrino interactions affecting oscillation probabilities.

Contribution

It introduces a framework where non-standard neutrino interactions reconcile differing 3 measurements from T2K and Daya Bay experiments.

Findings

NSI effects can align T2K and Daya Bay 3 results

Reconciliation depends on specific NSI parameters

Standard oscillation models cannot fully explain the data

Abstract

We show that the relatively large best fit value of $\sin^2 2 \theta_{13} = 0.14 \, (0.17)$ measured in the T2K experiment for fixed values of i) the Dirac CP violation phase $\delta = 0$, and ii) the atmospheric neutrino mixing parameters $\theta_{23} = \pi/4$, $|\Delta m^2_{32}| = 2.4 \times 10^{-3} \; {\rm eV}^2$, can be reconciled with the Daya Bay result $\sin^2 2 \theta_{13} = 0.090 \pm 0.009$ if the effects of non-standard neutrino interactions (NSI) in the relevant $\bar \nu_e \to \bar \nu_e$ and $\nu_\mu \to \nu_e$ oscillation probabilities are taken into account.