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Initial measurement of reactor antineutrino oscillation at SNO+

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Initial measurement of reactor antineutrino oscillation at SNO+. / SNO+ Collaboration ; Kormos, L. L.; O'Keeffe, H. M.
In: European Physical Journal C, Vol. 85, No. 1, 17, 31.01.2025.

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SNO+ Collaboration, Kormos LL, O'Keeffe HM. Initial measurement of reactor antineutrino oscillation at SNO+. European Physical Journal C. 2025 Jan 31;85(1):17. Epub 2025 Jan 10. doi: 10.1140/epjc/s10052-024-13687-5

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SNO+ Collaboration ; Kormos, L. L. ; O'Keeffe, H. M. / Initial measurement of reactor antineutrino oscillation at SNO+. In: European Physical Journal C. 2025 ; Vol. 85, No. 1.

Bibtex

@article{951aa769637946729750826039951bbf,
title = "Initial measurement of reactor antineutrino oscillation at SNO+",
abstract = " The SNO+ collaboration reports its first spectral analysis of long-baseline reactor antineutrino oscillation using 114 tonne-years of data. Fitting the neutrino oscillation probability to the observed energy spectrum yields constraints on the neutrino mass-squared difference $\Delta m^2_{21}$. In the ranges allowed by previous measurements, the best-fit $\Delta m^2_{21}$ is (8.85$^{+1.10}_{-1.33}$) $\times$ 10$^{-5}$ eV$^2$. This measurement is continuing in the next phases of SNO+ and is expected to surpass the present global precision on $\Delta m^2_{21}$ with about three years of data. ",
keywords = "hep-ex, nucl-ex",
author = "{SNO+ Collaboration} and A. Allega and S. Andringa and M. Askins and Auty, {D. J.} and A. Bacon and F. Bar{\~a}o and N. Barros and R. Bayes and Beier, {E. W.} and Bezerra, {T. S.} and A. Bialek and Biller, {S. D.} and E. Blucher and E. Caden and Callaghan, {E. J.} and B. Cleveland and D. Cookman and J. Corning and R. Dehghani and J. Deloye and Depatie, {M. M.} and Lodovico, {F. Di} and C. Dima and J. Dittmer and Dixon, {K. H.} and Esmaeilian, {M. S.} and E. Falk and N. Fatemighomi and R. Ford and A. Gaur and Gonz{\'a}lez-Reina, {O. I.} and D. Gooding and C. Grant and Hallin, {A. L.} and D. Hallman and Heintzelman, {W. J.} and Helmer, {R. L.} and B. Hreljac and P. Huang and R. Hunt-Stokes and In{\'a}cio, {A. S.} and Jillings, {C. J.} and S. Kaluzienski and T. Kaptanoglu and J. Kladnik and Klein, {J. R.} and Kormos, {L. L.} and O'Keeffe, {H. M.}",
year = "2025",
month = jan,
day = "31",
doi = "10.1140/epjc/s10052-024-13687-5",
language = "English",
volume = "85",
journal = "European Physical Journal C",
number = "1",

}

RIS

TY - JOUR

T1 - Initial measurement of reactor antineutrino oscillation at SNO+

AU - SNO+ Collaboration

AU - Allega, A.

AU - Andringa, S.

AU - Askins, M.

AU - Auty, D. J.

AU - Bacon, A.

AU - Barão, F.

AU - Barros, N.

AU - Bayes, R.

AU - Beier, E. W.

AU - Bezerra, T. S.

AU - Bialek, A.

AU - Biller, S. D.

AU - Blucher, E.

AU - Caden, E.

AU - Callaghan, E. J.

AU - Cleveland, B.

AU - Cookman, D.

AU - Corning, J.

AU - Dehghani, R.

AU - Deloye, J.

AU - Depatie, M. M.

AU - Lodovico, F. Di

AU - Dima, C.

AU - Dittmer, J.

AU - Dixon, K. H.

AU - Esmaeilian, M. S.

AU - Falk, E.

AU - Fatemighomi, N.

AU - Ford, R.

AU - Gaur, A.

AU - González-Reina, O. I.

AU - Gooding, D.

AU - Grant, C.

AU - Hallin, A. L.

AU - Hallman, D.

AU - Heintzelman, W. J.

AU - Helmer, R. L.

AU - Hreljac, B.

AU - Huang, P.

AU - Hunt-Stokes, R.

AU - Inácio, A. S.

AU - Jillings, C. J.

AU - Kaluzienski, S.

AU - Kaptanoglu, T.

AU - Kladnik, J.

AU - Klein, J. R.

AU - Kormos, L. L.

AU - O'Keeffe, H. M.

PY - 2025/1/31

Y1 - 2025/1/31

N2 - The SNO+ collaboration reports its first spectral analysis of long-baseline reactor antineutrino oscillation using 114 tonne-years of data. Fitting the neutrino oscillation probability to the observed energy spectrum yields constraints on the neutrino mass-squared difference $\Delta m^2_{21}$. In the ranges allowed by previous measurements, the best-fit $\Delta m^2_{21}$ is (8.85$^{+1.10}_{-1.33}$) $\times$ 10$^{-5}$ eV$^2$. This measurement is continuing in the next phases of SNO+ and is expected to surpass the present global precision on $\Delta m^2_{21}$ with about three years of data.

AB - The SNO+ collaboration reports its first spectral analysis of long-baseline reactor antineutrino oscillation using 114 tonne-years of data. Fitting the neutrino oscillation probability to the observed energy spectrum yields constraints on the neutrino mass-squared difference $\Delta m^2_{21}$. In the ranges allowed by previous measurements, the best-fit $\Delta m^2_{21}$ is (8.85$^{+1.10}_{-1.33}$) $\times$ 10$^{-5}$ eV$^2$. This measurement is continuing in the next phases of SNO+ and is expected to surpass the present global precision on $\Delta m^2_{21}$ with about three years of data.

KW - hep-ex

KW - nucl-ex

U2 - 10.1140/epjc/s10052-024-13687-5

DO - 10.1140/epjc/s10052-024-13687-5

M3 - Journal article

VL - 85

JO - European Physical Journal C

JF - European Physical Journal C

IS - 1

M1 - 17

ER -