2025/11/26 by Francesco Capozzi, Capozzi, Francesco, E. Lisi +7 · 7 citations
Physics and Astronomy · #Neutrino Physics Research #Particle physics theoretical and experimental studies #Quantum Chromodynamics and Particle Interactions
paper · pdf · doi:10.48550/arxiv.2511.21650
Within the standard 3ν framework, we discuss updated bounds on the leading oscillation parameters related to the (ν1, ν2) states, namely, the squared mass difference δm2=m22-m21 and the mixing parameter sin2θ12. A previous global analysis of 2024 oscillation data estimated δm2 and sin2θ12 with fractional 1σ errors of about 2.3% and 4.5%, respectively. First we update the analysis by applying the latest SNO+ constraints, that slightly shift the (δm2, sin2θ12) best fits. Then we apply the constraints placed by the first JUNO results, that significantly reduce the uncertainties of both parameters. Our updated global bounds (as of 2025) can be summarized as: δm2/10-5\rm eV2 = 7.48± 0.10 and sin2θ12=0.3085±0.0073 (with correlation ρ=-0.20), corresponding to 1σ uncertainties as small as 1.3% and 2.4%, respectively. We also comment on minor physical and statistical effects that, in the future, may contribute to lift the current mass-ordering degeneracy of (δm2, θ12) estimates.