Abstract
SNO+ Collaboration reports its second spectral analysis of reactor antineutrino oscillation using 286 ton-yr of new data. The measured energies of reactor antineutrino candidates were fitted to obtain the second-most precise determination of the neutrino mass-squared difference Δm212=(7.96-0.42+0.48)×10-5 eV2. Constraining Δm212 and sin2θ12 with measurements from long-baseline reactor antineutrino and solar neutrino experiments yields Δm212=(7.58-0.17+0.18)×10-5 eV2 and sin2θ12=0.308±0.013. This fit also yields a first measurement of the flux of geoneutrinos in the Western Hemisphere, with 73-43+47 TNU at SNO+.
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CITATION STYLE
Abreu, M., Albanese, V., Allega, A., Alves, R., Anderson, M. R., Andringa, S., … Zummo, A. (2025). Measurement of Reactor Antineutrino Oscillation at SNO+. Physical Review Letters, 135(12). https://doi.org/10.1103/gypt-lc9v
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