A KamLAND global fit using Daya Bay-measured antineutrino spectra instead of the Huber-Müller model lowers the best-fit Δm²₂₁ from 7.53 to 7.50 ×10^{-5} eV² and reduces tension with JUNO.
Measurement of the Electron Antineu- trino Oscillation with 1958 Days of Operation at Daya Bay
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Refined Global Fit of KamLAND Data and the Daya Bay Antineutrino Energy Spectrum
A KamLAND global fit using Daya Bay-measured antineutrino spectra instead of the Huber-Müller model lowers the best-fit Δm²₂₁ from 7.53 to 7.50 ×10^{-5} eV² and reduces tension with JUNO.