Neutrino masses and mixing: Entering the era of subpercent precision
Abstract
We perform an updated global analysis of the known and unknown parameters of the standard 3 framework as of 2025. The known oscillation parameters include three mixing angles (θ12,\,θ23,\,θ13) and two squared mass gaps, chosen as δ m2=m22-m21>0 and m2=m23-12(m21+m22), where α=sign( m2) distinguishes normal ordering (NO, α=+1) from inverted ordering (IO, α=-1). With respect to our previous 2021 update, the combination of oscillation data leads to appreciably reduced uncertainties for θ23, θ13 and | m2|. In particular, | m2| is the first 3 parameter to enter the domain of subpercent precision (0.8\% at 1σ). We underline some issues about systematics, that might affect this error estimate. Concerning oscillation unknowns, we find a relatively weak preference for NO versus IO (at 2.2σ), for CP violation versus conservation in NO (1.3σ) and for the first θ23 octant versus the second in NO (1.1σ). We discuss the status and qualitative prospects of the mass ordering hint in the plane (δ m2,\, m2ee), where m2ee=| m2|+12α(2θ12-2θ12)δ m2, to be measured by the JUNO experiment with subpercent precision. We also discuss upper bounds on nonoscillation observables. We report mβ<0.50~eV and mββ<0.086~eV (2σ). Concerning the sum of neutrino masses , we discuss representative combinations of data, with or without augmenting the model with extra parameters accounting for possible systematics or new physics. The resulting 2σ upper limits are roughly spread around the bound < 0.2~eV within a factor of three. [Abridged]
Turn this paper into a full lesson
ArcXiv compiles a staged curriculum from this paper: 8-12 lessons across beginner → advanced, synthesised section guides, visuals, flashcards, a quiz, exercises, and on-demand deep dives per section. Grounded in the abstract, never invented.