A Simple Parameterization of Matter Effects on Neutrino Oscillations

Abstract

We present simple analytical approximations to matter-effect corrected effective neutrino mixing-angles and effective mass-squared-differences. The expressions clarify the dependence of oscillation probabilities in matter to the mixing angles and mass-squared-differences in vacuum, and are useful for analyzing long-baseline neutrino oscillation experiments.

73 pages REVTeX4, 84 eps figures

Cited by in corpus (9)

• Analytical Approximation of the Neutrino Oscillation Matter Effects at large ${\theta }_{13}$
• Solving the degeneracy of the lepton-flavor mixing angle theta_atm by the T2KK two detector neutrino oscillation experiment
• Why Is The Neutrino Oscillation Formula Expanded In $\Delta m_{21}^2/\Delta m_{31}^2$ Still Accurate Near The Solar Resonance In Matter?
• A compact analytical approximation for a light sterile neutrino oscillation in matter
• Constraints on New Physics from Long Baseline Neutrino Oscillation Experiments
• Fibonacci Fast Convergence for Neutrino Oscillations in Matter
• Probing the sensitivity to leptonic ${\delta }_{CP}$ in presence of invisible decay of ${\nu }_3$ using atmospheric neutrinos
• Hierarchy independent sensitivity to leptonic δ_CP with atmospheric neutrinos
• Could Geoneutrinos Interact With the Geomagnetic Field?