Neutrino Oscillations and Collider Test of the R-parity Violating Minimal Supergravity Model

Abstract

We study the R-parity violating minimal supergravity models accounting for the observed neutrino masses and mixing, which can be tested in future collider experiments. The bi-large mixing can be explained by allowing five dominant tri-linear couplings $ λ&#39;_{1,2,3}$ and $λ_{1,2}$. The desired ratio of the atmospheric and solar neutrino mass-squared differences can be obtained in a very limited parameter space where the tree-level contribution is tuned to be suppressed. In this allowed region, we quantify the correlation between the three neutrino mixing angles and the tri-linear R-parity violating couplings. Qualitatively, the relations $| λ&#39;_1 | < | λ&#39;_2| \sim | λ&#39;_3|$, and $|λ_1| \sim |λ_2|$ are required by the large atmospheric neutrino mixing angle $θ_{23}$ and the small angle $θ_{13}$, and the large solar neutrino mixing angle $θ_{12}$, respectively. Such a prediction on the couplings can be tested in the next linear colliders by observing the branching ratios of the lightest supersymmetric particle (LSP). For the stau or the neutralino LSP, the ratio $|λ_1|^2: |λ_2|^2: |λ_1|^2 + |λ_2|^2$ can be measured by establishing $Br(eν): Br(μν) : Br(τν)$ or $Br(νe^\pm τ^\mp ): Br(νμ^\pmτ^\mp) : Br(ντ^\pmτ^\mp)$, respectively. The information on the couplings $λ&#39;_i$ can be drawn by measuring $Br(l_i t \bar{b}) \propto |λ&#39;_i|^2$ if the neutralino LSP is heavier than the top quark.