First Evidence of Solar Neutrino Interactions on <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mmultiscripts> <mml:mrow> <mml:mi mathvariant="normal">C</mml:mi> </mml:mrow> <mml:mprescripts/> <mml:none/> <

The SNO+ Collaboration reports the first evidence of ^{8}B solar neutrinos interacting on ^{13}C nuclei. The charged current interaction proceeds through ^{13}C+ν_{e}→^{13}N+e^{-} which is followed, with a 10 minute half life, by ^{13}N→^{13}C+e^{+}+ν_{e}. The detection strategy is based on the delayed coincidence between the electron and the positron. Evidence for the charged current signal is presented with a significance of 4.2σ. Using the natural abundance of ^{13}C present in the scintillator, 5.7 metric tons of ^{13}C over 231 days of data were used in this analysis. The 5.6_{-2.3}^{+3.0} observed events in the data set are consistent with the expectation of 4.7_{-1.3}^{+0.6} events. This result is the second real-time measurement of CC interactions of ^{8}B neutrinos with nuclei and constitutes the lowest energy observation of neutrino interactions on ^{13}C generally. This enables the first direct measurement of the CC ν_{e} reaction to the ground state of ^{13}N, yielding an average cross section of (16.1_{-6.7}^{+8.5}(stat.)_{-2.7}^{+1.6}(syst.))×10^{-43} cm^{2} over the relevant ^{8}B solar neutrino energies.

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Journal
Physical Review Letters
Published
2025-10-27
DOI
https://doi.org/10.1103/1frl-95gj
Citations
1
Primary Topic
Neutrino Physics Research
Type
article
Field-Weighted Citation Impact
1.87
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article

First Evidence of Solar Neutrino Interactions on <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mmultiscripts> <mml:mrow> <mml:mi mathvariant="normal">C</mml:mi> </mml:mrow> <mml:mprescripts/> <mml:none/> <

M. Yeh, J. Rose, R. Rosero, R. Dehghani et al.
1 citations
Physical Review Letters
Neutrino Physics Research
1.87
article

First Evidence of Solar Neutrino Interactions on <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mmultiscripts> <mml:mrow> <mml:mi mathvariant="normal">C</mml:mi> </mml:mrow> <mml:mprescripts/> <mml:none/> <

M. Yeh, J. Rose, R. Rosero, R. Dehghani, D. M. Asner, S. Maguire, J. Deloye, A. Gaur, J. Corning, N. McCauley, E. Vázquez-Jáuregui, D. J. Auty, A. S. Inácio, E. Caden, S. Riccetto, C. J. Virtue, F. Di Lodovico, D. Gooding, B. Krar, C. Kraus, W. J. Heintzelman, R. Hunt-Stokes, S. H. Cheng, M. Chen, C. Raymond Lake, Muhammad Mubasher, J. D. Wilson, S. Yang, M. M. Depatie, B. Tam, F. Barão, Tânia Baltazar, S. S. Yu, P. Ravi, J. Dittmer, C. Lefebvre, John Simms, H. M. O’Keeffe, C. Grant, A. Allega, K. H. Dixon, L. Lebanowski, C. J. Jillings, M.C. Abreu, B. Hreljac, A. Bacon, N. Barros, J. Maneira, S. Andringa, D. Cookman, A. Zummo, G. D. Orebi Gann, L. L. Kormos, Sanjoy Kumar Pal, S. Kaluzienski, Daniel A. Morris, A. Białek, M. R. Anderson, Y. Zhang, G.M. Milton, O. I. González-Reina, V. Lozza, D. Hallman, C. B. Krauss, Jianfeng Shen, M. Smiley, Tereza Kroupova, B. Quenallata, K. Paleshi, C. Dima, M. S. Esmaeilian, J. Kladnik, Fang Wang, M. Luo, Z. Ye, John R. Klein, A. Reichold, S. Manecki, Reda Tafirout, M. Hebert, R. Bayes, N. Fatemighomi, W. Parker, A. L. Hallin, J. C-L. Tseng, J. R. Wilson, P. Skensved, L. J. Nolan, L. Pickard, S. Ouyang, R. D. Martín, S. D. Biller, T. Kaptanoglu, S. Naugle, Ping Huang, M. Ward, B. T. Cleveland, A. Wright, R. L. Helmer, R. Bayes, J. E. Grove, C. Hewitt, A. B. McDonald, K. Zuber, R. Ford, S. Hall, E. Falk, J. Page, E. E. Khoda, S. DeGraw, S. Gadamsetty
article en
1 citations

Abstract

The SNO+ Collaboration reports the first evidence of ^{8}B solar neutrinos interacting on ^{13}C nuclei. The charged current interaction proceeds through ^{13}C+ν_{e}→^{13}N+e^{-} which is followed, with a 10 minute half life, by ^{13}N→^{13}C+e^{+}+ν_{e}. The detection strategy is based on the delayed coincidence between the electron and the positron. Evidence for the charged current signal is presented with a significance of 4.2σ. Using the natural abundance of ^{13}C present in the scintillator, 5.7 metric tons of ^{13}C over 231 days of data were used in this analysis. The 5.6_{-2.3}^{+3.0} observed events in the data set are consistent with the expectation of 4.7_{-1.3}^{+0.6} events. This result is the second real-time measurement of CC interactions of ^{8}B neutrinos with nuclei and constitutes the lowest energy observation of neutrino interactions on ^{13}C generally. This enables the first direct measurement of the CC ν_{e} reaction to the ground state of ^{13}N, yielding an average cross section of (16.1_{-6.7}^{+8.5}(stat.)_{-2.7}^{+1.6}(syst.))×10^{-43} cm^{2} over the relevant ^{8}B solar neutrino energies.

Physical Review LettersVol. 135(24)
Boston University (US), TRIUMF (CA), University of Lisbon (PT), University of Liverpool (GB), Lawrence Berkeley National Laboratory (US), Shandong University (CN), University of Alberta (CA), University of Sussex (GB), King's College London (GB), Brookhaven National Laboratory (US), Queen's University (CA), LIP - Laboratory of Instrumentation and Experimental Particle Physics (PT), California University of Pennsylvania (US), University of Oxford (GB), Laurentian University (CA), Lancaster University (GB), University of Coimbra (PT), Technische Universität Dresden (DE), University of Pennsylvania (US), Shandong University of Science and Technology (CN), Universidad Nacional Autónoma de México (MX), Philadelphia University (US), University of California, Berkeley (US), University of Minho (PT)
Openalex Percentile: Top 10%
Neutrino Physics Research
1.87
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