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24 results on '"Cookman D"'

1. Initial measurement of reactor antineutrino oscillation at SNO+

Author

Allega, A, Anderson, MR, Andringa, S, Askins, M, Auty, DJ, Bacon, A, Baker, J, Barão, F, Barros, N, Bayes, R, Beier, EW, Bezerra, TS, Bialek, A, Biller, SD, Blucher, E, Caden, E, Callaghan, EJ, Chen, M, Cheng, S, Cleveland, B, Cookman, D, Corning, J, Cox, MA, Dehghani, R, Deloye, J, Depatie, MM, Di Lodovico, F, Dima, C, Dittmer, J, Dixon, KH, Esmaeilian, MS, Falk, E, Fatemighomi, N, Ford, R, Gaur, A, González-Reina, OI, Gooding, D, Grant, C, Grove, J, Hall, S, Hallin, AL, Hallman, D, Heintzelman, WJ, Helmer, RL, Hewitt, C, Howard, V, Hreljac, B, Hu, J, Huang, P, Hunt-Stokes, R, Hussain, SMA, Inácio, AS, Jillings, CJ, Kaluzienski, S, Kaptanoglu, T, Khan, H, Kladnik, J, Klein, JR, Kormos, LL, Krar, B, Kraus, C, Krauss, CB, Kroupová, T, Lake, C, Lebanowski, L, Lefebvre, C, Lozza, V, Luo, M, Maio, A, Manecki, S, Maneira, J, Martin, RD, McCauley, N, McDonald, AB, Mills, C, Milton, G, Colina, A Molina, Morris, D, Morton-Blake, I, Mubasher, M, Naugle, S, Nolan, LJ, O’Keeffe, HM, Gann, GD Orebi, Page, J, Paleshi, K, Parker, W, Paton, J, Peeters, SJM, Pickard, L, Quenallata, B, Ravi, P, Reichold, A, Riccetto, S, Rose, J, Rosero, R, Semenec, I, Simms, J, Skensved, P, and Smiley, M

Subjects
Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Astronomical sciences, Atomic, molecular and optical physics, Particle and high energy physics
Abstract

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 $$\Delta m^2_{21}$$ Δ m 21 2 . In the ranges allowed by previous measurements, the best-fit $$\Delta m^2_{21}$$ Δ m 21 2 is ($$8.85^{+1.10}_{-1.33}$$ 8 . 85 - 1.33 + 1.10 ) $$\times $$ × $$10^{-5}$$ 10 - 5 $$\hbox {eV}^2$$ eV 2 . This measurement is continuing in the next phases of SNO+ and is expected to surpass the present global precision on $$\Delta m^2_{21}$$ Δ m 21 2 with about three years of data.

Published
2025

2. Measurement of the B8 solar neutrino flux using the full SNO+ water phase dataset

Author

Allega, A, Anderson, MR, Andringa, S, Askins, M, Asner, DM, Auty, DJ, Bacon, A, Barão, F, Barros, N, Bayes, R, Beier, EW, Bialek, A, Biller, SD, Blucher, E, Caden, E, Callaghan, EJ, Chen, M, Cheng, S, Cleveland, B, Cookman, D, Corning, J, Cox, MA, Dehghani, R, Deloye, J, Depatie, MM, Di Lodovico, F, Dima, C, Dittmer, J, Dixon, KH, Esmaeilian, MS, Falk, E, Fatemighomi, N, Ford, R, Gaur, A, González-Reina, OI, Gooding, D, Grant, C, Grove, J, Hall, S, Hallin, AL, Hallman, D, Heintzelman, WJ, Helmer, RL, Hewitt, C, Hreljac, B, Hu, J, Huang, P, Hunt-Stokes, R, Hussain, SMA, Inácio, AS, Jillings, CJ, Kaluzienski, S, Kaptanoglu, T, Kladnik, J, Klein, JR, Kormos, LL, Krar, B, Kraus, C, Krauss, CB, Kroupová, T, Lake, C, Lebanowski, L, Lefebvre, C, Lozza, V, Luo, M, Maio, A, Manecki, S, Maneira, J, Martin, RD, McCauley, N, McDonald, AB, Milton, G, Morris, D, Mubasher, M, Naugle, S, Nolan, LJ, O’Keeffe, HM, Gann, GD Orebi, Page, J, Paleshi, K, Parker, W, Paton, J, Peeters, SJM, Pickard, L, Quenallata, B, Ravi, P, Reichold, A, Riccetto, S, Rose, J, Rosero, R, Semenec, I, Simms, J, Skensved, P, Smiley, M, Svoboda, R, Tam, B, Tseng, J, Vázquez-Jáuregui, E, Virtue, CJ, and Ward, M

Subjects
Particle and High Energy Physics, Mathematical Physics, Mathematical Sciences, Physical Sciences, Astronomical Sciences
Abstract

The SNO+ detector operated initially as a water Cherenkov detector. The implementation of a sealed cover gas system midway through water data taking resulted in a significant reduction in the activity of Rn222 daughters in the detector and allowed the lowest background to the solar electron scattering signal above 5 MeV achieved to date. This paper reports an updated SNO+ water phase B8 solar neutrino analysis with a total livetime of 282.4 days and an analysis threshold of 3.5 MeV. The B8 solar neutrino flux is found to be (2.32-0.17+0.18(stat)-0.05+0.07(syst))×106 cm-2 s-1 assuming no neutrino oscillations, or (5.36-0.39+0.41(stat)-0.16+0.17(syst))×106 cm-2 s-1 assuming standard neutrino oscillation parameters, in good agreement with both previous measurements and standard solar model calculations. The electron recoil spectrum is presented above 3.5 MeV.

Published
2024

3. Measurement of the $^8$B Solar Neutrino Flux Using the Full SNO+ Water Phase Dataset

Author

Collaboration, SNO, Allega, A., Anderson, M. R., Andringa, S., Askins, M., Asner, D. M., Auty, D. J., Bacon, A., Barão, F., Barros, N., Bayes, R., Beier, E. W., Bialek, A., Biller, S. D., Blucher, E., Caden, E., Callaghan, E. J., Chen, M., Cheng, S., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Dehghani, R., Deloye, J., Depatie, M. M., Di Lodovico, F., Dima, C., Dittmer, J., Dixon, K. H., Esmaeilian, M. S., Falk, E., Fatemighomi, N., Ford, R., Gaur, A., González-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hall, S., Hallin, A. L., Hallman, D., Heintzelman, W. J., Helmer, R. L., Hewitt, C., Hreljac, B., Hu, J., Huang, P., Hunt-Stokes, R., Hussain, S. M. A., Inácio, A. S., Jillings, C. J., Kaluzienski, S., Kaptanoglu, T., Kladnik, J., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupová, T., Lake, C., Lebanowski, L., Lefebvre, C., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Milton, G., Morris, D., Mubasher, M., Naugle, S., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Paleshi, K., Parker, W., Paton, J., Peeters, S. J. M., Pickard, L., Quenallata, B., Ravi, P., Reichold, A., Riccetto, S., Rose, J., Rosero, R., Semenec, I., Simms, J., Skensved, P., Smiley, M., Svoboda, R., Tam, B., Tseng, J., Vázquez-Jáuregui, E., Virtue, C. J., Ward, M., Wilson, J. R., Wilson, J. D., Wright, A., Yang, S., Yeh, M., Ye, Z., Yu, S., Zhang, Y., Zuber, K., and Zummo, A.

Subjects
High Energy Physics - Experiment
Abstract

The SNO+ detector operated initially as a water Cherenkov detector. The implementation of a sealed covergas system midway through water data taking resulted in a significant reduction in the activity of $^{222}$Rn daughters in the detector and allowed the lowest background to the solar electron scattering signal above 5 MeV achieved to date. This paper reports an updated SNO+ water phase $^8$B solar neutrino analysis with a total livetime of 282.4 days and an analysis threshold of 3.5 MeV. The $^8$B solar neutrino flux is found to be $\left(2.32^{+0.18}_{-0.17}\text{(stat.)}^{+0.07}_{-0.05}\text{(syst.)}\right)\times10^{6}$ cm$^{-2}$s$^{-1}$ assuming no neutrino oscillations, or $\left(5.36^{+0.41}_{-0.39}\text{(stat.)}^{+0.17}_{-0.16}\text{(syst.)} \right)\times10^{6}$ cm$^{-2}$s$^{-1}$ assuming standard neutrino oscillation parameters, in good agreement with both previous measurements and Standard Solar Model Calculations. The electron recoil spectrum is presented above 3.5 MeV., Comment: 9 pages, 10 figures, v2: minor updates to match PRD publication

Published
2024
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4. Initial measurement of reactor antineutrino oscillation at SNO+

Author

Collaboration, SNO, Allega, A., Anderson, M. R., Andringa, S., Askins, M., Asner, D. M., Auty, D. J., Bacon, A., Baker, J., Barão, F., Barros, N., Bayes, R., Beier, E. W., Bezerra, T. S., Bialek, A., Biller, S. D., Blucher, E., Caden, E., Callaghan, E. J., Chen, M., Cheng, S., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Dehghani, R., Deloye, J., Depatie, M. M., Di Lodovico, F., Dima, C., Dittmer, J., Dixon, K. H., Esmaeilian, M. S., Falk, E., Fatemighomi, N., Ford, R., Gaur, A., González-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hall, S., Hallin, A. L., Hallman, D., Heintzelman, W. J., Helmer, R. L., Hewitt, C., Howard, V., Hreljac, B., Hu, J., Huang, P., Hunt-Stokes, R., Hussain, S. M. A., Inácio, A. S., Jillings, C. J., Kaluzienski, S., Kaptanoglu, T., Khan, H., Kladnik, J., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupová, T., Lake, C., Lebanowski, L., Lefebvre, C., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Mills, C., Milton, G., Colina, A. Molina, Morris, D., Morton-Blake, I., Mubasher, M., Naugle, S., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Paleshi, K., Parker, W., Paton, J., Peeters, S. J. M., Pickard, L., Quenallata, B., Ravi, P., Reichold, A., Riccetto, S., Rose, J., Rosero, R., Semenec, I., Simms, J., Skensved, P., Smiley, M., Smith, J., Svoboda, R., Tam, B., Tseng, J., Vázquez-Jáuregui, E., Veinot, J. G. C., Virtue, C. J., Ward, M., Weigand, J. J., Wilson, J. R., Wilson, J. D., Wright, A., Yang, S., Yeh, M., Ye, Z., Yu, S., Zhang, Y., Zuber, K., and Zummo, A.

Subjects
High Energy Physics - Experiment, Nuclear Experiment
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.

Published
2024
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5. Event-by-event direction reconstruction of solar neutrinos in a high light-yield liquid scintillator

Author

Allega, A, Anderson, MR, Andringa, S, Antunes, J, Askins, M, Auty, DJ, Bacon, A, Baker, J, Barros, N, Barão, F, Bayes, R, Beier, EW, Bezerra, TS, Bialek, A, Biller, SD, Blucher, E, Caden, E, Callaghan, EJ, Chen, M, Cheng, S, Cleveland, B, Cookman, D, Corning, J, Cox, MA, Dehghani, R, Deloye, J, Depatie, MM, Di Lodovico, F, Dittmer, J, Dixon, KH, Falk, E, Fatemighomi, N, Ford, R, Gaur, A, González-Reina, OI, Gooding, D, Grant, C, Grove, J, Hall, S, Hallin, AL, Heintzelman, WJ, Helmer, RL, Hewitt, C, Hreljac, B, Howard, V, Hu, J, Hunt-Stokes, R, Hussain, SMA, Inácio, AS, Jillings, CJ, Kaluzienski, S, Kaptanoglu, T, Khaghani, P, Khan, H, Klein, JR, Kormos, LL, Krar, B, Kraus, C, Krauss, CB, Kroupová, T, Lake, C, Lebanowski, L, Lee, J, Lefebvre, C, Lin, YH, Lozza, V, Luo, M, Maio, A, Manecki, S, Maneira, J, Martin, RD, McCauley, N, McDonald, AB, Mills, C, Milton, G, Morton-Blake, I, Mubasher, M, Colina, A Molina, Morris, D, Naugle, S, Nolan, LJ, O’Keeffe, HM, Gann, GD Orebi, Page, J, Paleshi, K, Parker, W, Paton, J, Peeters, SJM, Pickard, L, Ravi, P, Reichold, A, Riccetto, S, Rigan, M, Rose, J, Rosero, R, Rumleskie, J, Semenec, I, Skensved, P, Smiley, M, and Smith, J

Subjects
Nuclear and Plasma Physics, Physical Sciences
Abstract

The direction of individual B8 solar neutrinos has been reconstructed using the SNO+ liquid scintillator detector. Prompt, directional Cherenkov light was separated from the slower, isotropic scintillation light using time information, and a maximum likelihood method was used to reconstruct the direction of individual scattered electrons. A clear directional signal was observed, correlated with the solar angle. The observation was aided by a period of low primary fluor concentration that resulted in a slower scintillator decay time. This is the first time that event-by-event direction reconstruction in high light-yield liquid scintillator has been demonstrated in a large-scale detector.

Published
2024

6. Event-by-Event Direction Reconstruction of Solar Neutrinos in a High Light-Yield Liquid Scintillator

Author

Allega, A., Anderson, M. R., Andringa, S., Antunes, J., Askins, M., Auty, D. J., Bacon, A., Baker, J., Barros, N., Barão, F., Bayes, R., Beier, E. W., Bezerra, T. S., Bialek, A., Biller, S. D., Blucher, E., Caden, E., Callaghan, E. J., Chen, M., Cheng, S., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Dehghani, R., Deloye, J., Depatie, M. M., Di Lodovico, F., Dittmer, J., Dixon, K. H., Falk, E., Fatemighomi, N., Ford, R., Gaur, A., Ganzálaz-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hall, S., Hallin, A. L., Heintzelman, W. J., Helmer, R. L., Hewitt, C., Hreljac, B., Howard, V., Hu, J., Hunt-Stokes, R., Hussain, S. M. A., Inácio, A. S., Jillings, C. J., Kaluzienski, S., Kaptanoglu, T., Khaghani, P., Khan, H., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupová, T., Lake, C., Lebanowski, L., Lee, J., Lefebvra, C., Lin, Y. H., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Mills, C., Milton, G., Morton-Blake, I., Mubasher, M., Colina, A. Molina, Morris, D., Naugle, S., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Paleshi, K., Parker, W., Paton, J., Peeters, S. J. M., Pickard, L., Ravi, P., Reichold, A., Riccetto, S., Rigan, M., Rose, J., Rosero, R., Rumleskie, J., Semenec, I., Skensvard, P., Smiley, M., Smith, J., Svoboda, R., Tam, B., Tseng, J., Valder, S., Vázquez-Jáuregui, E., Virtue, C. J., Wang, J., Ward, M., Wilson, J. R., Wilson, J. D., Wright, A., Yanez, J. P., Yang, S., Yeh, M., Ye, Z., Yu, S., Zhang, Y., Zuber, K., and Zummo, A.

Subjects
High Energy Physics - Experiment, Physics - Instrumentation and Detectors
Abstract

The direction of individual $^8$B solar neutrinos has been reconstructed using the SNO+ liquid scintillator detector. Prompt, directional Cherenkov light was separated from the slower, isotropic scintillation light using time information, and a maximum likelihood method was used to reconstruct the direction of individual scattered electrons. A clear directional signal was observed, correlated with the solar angle. The observation was aided by a period of low primary fluor concentration that resulted in a slower scintillator decay time. This is the first time that event-by-event direction reconstruction in high light-yield liquid scintillator has been demonstrated in a large-scale detector., Comment: 6 pages, 6 figures. Accepted manuscript by PRD

Published
2023
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7. Evidence of Antineutrinos from Distant Reactors using Pure Water at SNO+

Author

Collaboration, SNO, Allega, A., Anderson, M. R., Andringa, S., Antunes, J., Askins, M., Auty, D. J., Bacon, A., Barros, N., Barao, F., Bayes, R., Beier, E. W., Bezerra, T. S., Bialek, A., Biller, S. D., Blucher, E., Caden, E., Callaghan, E. J., Cheng, S., Chen, M., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Dehghani, R., Deloye, J., Deluce, C., Depatie, M. M., Dittmer, J., Dixon, K. H., Di Lodovico, F., Falk, E., Fatemighomi, N., Ford, R., Frankiewicz, K., Gaur, A., Gonzalez-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hallin, A. L., Hallman, D., Heintzelman, W. J., Helmer, R. L., Hu, J., Hunt-Stokes, R., Hussain, S. M. A., Inacio, A. S., Jillings, C. J., Kaluzienski, S., Kaptanoglu, T., Khaghani, P., Khan, H., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupova, T., Lam, I., Land, B. J., Lawson, I., Lebanowski, L., Lee, J., Lefebvre, C., Lidgard, J., Lin, Y. H., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Mills, C., Morton-Blake, I., Naugle, S., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Parker, W., Paton, J., Peeters, S. J. M., Pickard, L., Ravi, P., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Rose, J., Rosero, R., Rumleskie, J., Semenec, I., Skensved, P., Smiley, M., Svoboda, R., Tam, B., Tseng, J., Turner, E., Valder, S., Virtue, C. J., Vazquez-Jauregui, E., Wang, J., Ward, M., Wilson, J. R., Wilson, J. D., Wright, A., Yanez, J. P., Yang, S., Yeh, M., Yu, S., Zhang, Y., Zuber, K., and Zummo, A.

Subjects
Nuclear Experiment, High Energy Physics - Experiment
Abstract

The SNO+ Collaboration reports the first evidence of reactor antineutrinos in a Cherenkov detector. The nearest nuclear reactors are located 240~km away in Ontario, Canada. This analysis uses events with energies lower than in any previous analysis with a large water Cherenkov detector. Two analytical methods are used to distinguish reactor antineutrinos from background events in 190 days of data and yield consistent evidence for antineutrinos with a combined significance of 3.5$\sigma$., Comment: v2: add missing author, add link to supplemental material v3: minor updates to match PRL publication

Published
2022
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8. Evidence of Antineutrinos from Distant Reactors Using Pure Water at SNO+

Author

Allega, A, Anderson, MR, Andringa, S, Antunes, J, Askins, M, Auty, DJ, Bacon, A, Barros, N, Barão, F, Bayes, R, Beier, EW, Bezerra, TS, Bialek, A, Biller, SD, Blucher, E, Caden, E, Callaghan, EJ, Cheng, S, Chen, M, Cleveland, B, Cookman, D, Corning, J, Cox, MA, Dehghani, R, Deloye, J, Deluce, C, Depatie, MM, Dittmer, J, Dixon, KH, Di Lodovico, F, Falk, E, Fatemighomi, N, Ford, R, Frankiewicz, K, Gaur, A, González-Reina, OI, Gooding, D, Grant, C, Grove, J, Hallin, AL, Hallman, D, Heintzelman, WJ, Helmer, RL, Hu, J, Hunt-Stokes, R, Hussain, SMA, Inácio, AS, Jillings, CJ, Kaluzienski, S, Kaptanoglu, T, Khaghani, P, Khan, H, Klein, JR, Kormos, LL, Krar, B, Kraus, C, Krauss, CB, Kroupová, T, Lam, I, Land, BJ, Lawson, I, Lebanowski, L, Lee, J, Lefebvre, C, Lidgard, J, Lin, YH, Lozza, V, Luo, M, Maio, A, Manecki, S, Maneira, J, Martin, RD, McCauley, N, McDonald, AB, Mills, C, Morton-Blake, I, Naugle, S, Nolan, LJ, O’Keeffe, HM, Gann, GD Orebi, Page, J, Parker, W, Paton, J, Peeters, SJM, Pickard, L, Ravi, P, Reichold, A, Riccetto, S, Richardson, R, Rigan, M, Rose, J, Rosero, R, Rumleskie, J, Semenec, I, Skensved, P, Smiley, M, Svoboda, R, Tam, B, Tseng, J, and Turner, E

Subjects
Nuclear and Plasma Physics, Physical Sciences, SNO+ Collaboration, Mathematical Sciences, Engineering, General Physics, Mathematical sciences, Physical sciences
Abstract

The SNO+ Collaboration reports the first evidence of reactor antineutrinos in a Cherenkov detector. The nearest nuclear reactors are located 240 km away in Ontario, Canada. This analysis uses events with energies lower than in any previous analysis with a large water Cherenkov detector. Two analytical methods are used to distinguish reactor antineutrinos from background events in 190 days of data and yield consistent evidence for antineutrinos with a combined significance of 3.5σ.

Published
2023

9. Improved search for invisible modes of nucleon decay in water with the SNO+ detector

Author

Collaboration, SNO, Allega, A., Anderson, M. R., Andringa, S., Askins, M., Auty, D. J., Bacon, A., Barros, N., Barão, F., Bayes, R., Beier, E. W., Bezerra, T. S., Bialek, A., Biller, S. D., Blucher, E., Caden, E., Callaghan, E. J., Cheng, S., Chen, M., Chkvorets, O., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Dehghani, R., Deluce, C., Depatie, M. M., Dittmer, J., Dixon, K. H., Di Lodovico, F., Falk, E., Fatemighomi, N., Ford, R., Frankiewicz, K., Gaur, A., González-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hallin, A. L., Hallman, D., Hartnell, J., Heintzelman, W. J., Helmer, R. L., Hu, J., Hunt-Stokes, R., Hussain, S. M. A., Inácio, A. S., Jillings, C. J., Kaptanoglu, T., Khaghani, P., Khan, H., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupová, T., Lam, I., Land, B. J., Lawson, I., Lebanowski, L., Lee, J., Lefebvre, C., Lidgard, J., Lin, Y. H., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Meyer, M., Mills, C., Morton-Blake, I., Naugle, S., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Parker, W., Paton, J., Peeters, S. J. M., Pickard, L., Ravi, P., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Rose, J., Rumleskie, J., Semenec, I., Skensved, P., Smiley, M., Svoboda, R., Tam, B., Tseng, J., Turner, E., Valder, S., Veinot, J. G. C., Virtue, C. J., Vázquez-Jáuregui, E., Wang, J., Ward, M., Weigand, J. J., Wilson, J. D., Wilson, J. R., Wright, A., Yanez, J. P., Yang, S., Yeh, M., Yu, S., Zhang, T., Zhang, Y., Zuber, K., and Zummo, A.

Subjects
High Energy Physics - Experiment
Abstract

This paper reports results from a search for single and multi-nucleon disappearance from the $^{16}$O nucleus in water within the \snoplus{} detector using all of the available data. These so-called "invisible" decays do not directly deposit energy within the detector but are instead detected through their subsequent nuclear de-excitation and gamma-ray emission. New limits are given for the partial lifetimes: $\tau(n\rightarrow inv) > 9.0\times10^{29}$ years, $\tau(p\rightarrow inv) > 9.6\times10^{29}$ years, $\tau(nn\rightarrow inv) > 1.5\times10^{28}$ years, $\tau(np\rightarrow inv) > 6.0\times10^{28}$ years, and $\tau(pp\rightarrow inv) > 1.1\times10^{29}$ years at 90\% Bayesian credibility level (with a prior uniform in rate). All but the ($nn\rightarrow inv$) results improve on existing limits by a factor of about 3.

Published
2022
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10. Improved search for invisible modes of nucleon decay in water with the SNO+detector

Author

Allega, A, Anderson, MR, Andringa, S, Askins, M, Auty, DJ, Bacon, A, Barros, N, Barão, F, Bayes, R, Beier, EW, Bezerra, TS, Bialek, A, Biller, SD, Blucher, E, Caden, E, Callaghan, EJ, Cheng, S, Chen, M, Chkvorets, O, Cleveland, B, Cookman, D, Corning, J, Cox, MA, Dehghani, R, Deluce, C, Depatie, MM, Dittmer, J, Dixon, KH, Di Lodovico, F, Falk, E, Fatemighomi, N, Ford, R, Frankiewicz, K, Gaur, A, González-Reina, OI, Gooding, D, Grant, C, Grove, J, Hallin, AL, Hallman, D, Hartnell, J, Heintzelman, WJ, Helmer, RL, Hu, J, Hunt-Stokes, R, Hussain, SMA, Inácio, AS, Jillings, CJ, Kaptanoglu, T, Khaghani, P, Khan, H, Klein, JR, Kormos, LL, Krar, B, Kraus, C, Krauss, CB, Kroupová, T, Lam, I, Land, BJ, Lawson, I, Lebanowski, L, Lee, J, Lefebvre, C, Lidgard, J, Lin, YH, Lozza, V, Luo, M, Maio, A, Manecki, S, Maneira, J, Martin, RD, McCauley, N, McDonald, AB, Meyer, M, Mills, C, Morton-Blake, I, Naugle, S, Nolan, LJ, O’Keeffe, HM, Gann, GD Orebi, Page, J, Parker, W, Paton, J, Peeters, SJM, Pickard, L, Ravi, P, Reichold, A, Riccetto, S, Richardson, R, Rigan, M, Rose, J, Rumleskie, J, Semenec, I, Skensved, P, Smiley, M, Svoboda, R, Tam, B, Tseng, J, Turner, E, and Valder, S

Subjects
Nuclear and Plasma Physics, Particle and High Energy Physics, Synchrotrons and Accelerators, Physical Sciences
Abstract

This paper reports results from a search for single and multinucleon disappearance from the O16 nucleus in water within the SNO+ detector using all of the available data. These so-called "invisible"decays do not directly deposit energy within the detector but are instead detected through their subsequent nuclear deexcitation and gamma-ray emission. New limits are given for the partial lifetimes: τ(n→inv)>9.0×1029 years, τ(p→inv)>9.6×1029 years, τ(nn→inv)>1.5×1028 years, τ(np→inv)>6.0×1028 years, and τ(pp→inv)>1.1×1029 years at 90% Bayesian credibility level (with a prior uniform in rate). All but the (nn→inv) results improve on existing limits by a factor of about 3.

Published
2022

11. Optical calibration of the SNO+ detector in the water phase with deployed sources

Author

Collaboration, SNO, Anderson, M. R., Andringa, S., Askins, M., Auty, D. J., Barão, F., Barros, N., Bayes, R., Beier, E. W., Bialek, A., Biller, S. D., Blucher, E., Boulay, M., Caden, E., Callaghan, E. J., Caravaca, J., Chen, M., Chkvorets, O., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Deluce, C., Depatie, M. M., Di Lodovico, F., Dittmer, J., Falk, E., Fatemighomi, N., Fischer, V., Ford, R., Frankiewicz, K., Gaur, A., Gilje, K., González-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hallin, A. L., Hallman, D., Hartnell, J., Heintzelman, W. J., Helmer, R. L., Hu, J., Hunt-Stokes, R., Hussain, S. M. A., Inácio, A. S., Jillings, C. J., Kaptanoglu, T., Khaghani, P., Khan, H., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupová, T., Lam, I., Land, B. J., LaTorre, A., Lawson, I., Lebanowski, L., Lefebvre, C., Li, A., Lidgard, J., Lin, Y. H., Liu, Y., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Meyer, M., Mills, C., Morton-Blake, I., Nae, S., Nirkko, M., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Parker, W., Paton, J., Peeters, S. J. M., Pershing, T., Pickard, L., Prior, G., Ravi, P., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Rose, J., Rumleskie, J., Semenec, I., Shaker, F., Sharma, M. K., Skensved, P., Smiley, M., Stainforth, R., Svoboda, R., Tam, B., Tseng, J., Turner, E., Valder, S., Vázquez-Jáuregui, E., Veinot, J. G. C., Virtue, C. J., Wang, J., Ward, M., Weigand, J. J., Wilson, J. R., Wright, A., Yanez, J. P., Yeh, M., Yu, S., Zhang, T., Zhang, Y., Zuber, K., and Zummo, A.

Subjects
Physics - Instrumentation and Detectors, High Energy Physics - Experiment, Nuclear Experiment
Abstract

SNO+ is a large-scale liquid scintillator experiment with the primary goal of searching for neutrinoless double beta decay, and is located approximately 2 km underground in SNOLAB, Sudbury, Canada. The detector acquired data for two years as a pure water Cherenkov detector, starting in May 2017. During this period, the optical properties of the detector were measured in situ using a deployed light diffusing sphere, with the goal of improving the detector model and the energy response systematic uncertainties. The measured parameters included the water attenuation coefficients, effective attenuation coefficients for the acrylic vessel, and the angular response of the photomultiplier tubes and their surrounding light concentrators, all across different wavelengths. The calibrated detector model was validated using a deployed tagged gamma source, which showed a 0.6% variation in energy scale across the primary target volume., Comment: Accepted by JINST (30 pages, 19 figures)

Published
2021
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12. The SNO+ Experiment

Author

Collaboration, SNO, Albanese, V., Alves, R., Anderson, M. R., Andringa, S., Anselmo, L., Arushanova, E., Asahi, S., Askins, M., Auty, D. J., Back, A. R., Back, S., Barão, F., Barnard, Z., Barr, A., Barros, N., Bartlett, D., Bayes, R., Beaudoin, C., Beier, E. W., Berardi, G., Bialek, A., Biller, S. D., Blucher, E., Bonventre, R., Boulay, M., Braid, D., Caden, E., Callaghan, E. J., Caravaca, J., Carvalho, J., Cavalli, L., Chauhan, D., Chen, M., Chkvorets, O., Clark, K. J., Cleveland, B., Connors, C., Cookman, D., Coulter, I. T., Cox, M. A., Cressy, D., Dai, X., Darrach, C., Davis-Purcell, B., Deluce, C., Depatie, M. M., Descamps, F., Di Lodovico, F., Dittmer, J., Doxtator, A., Duhaime, N., Duncan, F., Dunger, J., Earle, A. D., Fabris, D., Falk, E., Farrugia, A., Fatemighomi, N., Felber, C., Fischer, V., Fletcher, E., Ford, R., Frankiewicz, K., Gagnon, N., Gaur, A., Gauthier, J., Gibson-Foster, A., Gilje, K., González-Reina, O. I., Gooding, D., Gorel, P., Graham, K., Grant, C., Grove, J., Grullon, S., Guillian, E., Hall, S., Hallin, A. L., Hallman, D., Hans, S., Hartnell, J., Harvey, P., Hedayatipour, M., Heintzelman, W. J., Heise, J., Helmer, R. L., Hodak, B., Hodak, M., Hood, M., Horne, D., Hreljac, B., Hu, J., Hussain, S. M. A., Iida, T., Inácio, A. S., Jackson, C. M., Jelley, N. A., Jillings, C. J., Jones, C., Jones, P. G., Kamdin, K., Kaptanoglu, T., Kaspar, J., Keeter, K., Kefelian, C., Khaghani, P., Kippenbrock, L., Klein, J. R., Knapik, R., Kofron, J., Kormos, L. L., Korte, S., Krar, B., Kraus, C., Krauss, C. B., Kroupová, T., Labe, K., Lafleur, F., Lam, I., Lan, C., Land, B. J., Lane, R., Langrock, S., Larochelle, P., Larose, S., LaTorre, A., Lawson, I., Lebanowski, L., Lefeuvre, G. M., Leming, E. J., Li, A., Li, O., Lidgard, J., Liggins, B., Liimatainen, P., Lin, Y. H., Liu, X., Liu, Y., Lozza, V., Luo, M., Maguire, S., Maio, A., Majumdar, K., Manecki, S., Maneira, J., Martin, R. D., Marzec, E., Mastbaum, A., Mathewson, A., McCauley, N., McDonald, A. B., McFarlane, K., Mekarski, P., Meyer, M., Miller, C., Mills, C., Mlejnek, M., Mony, E., Morissette, B., Morton-Blake, I., Mottram, M. J., Nae, S., Nirkko, M., Nolan, L. J., Novikov, V. M., O'Keeffe, H. M., O'Sullivan, E., Gann, G. D. Orebi, Parnell, M. J., Paton, J., Peeters, S. J. M., Pershing, T., Petriw, Z., Petzoldt, J., Pickard, L., Pracsovics, D., Prior, G., Prouty, J. C., Quirk, S., Read, S., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Ritchie, I., Robertson, A., Robertson, B. C., Rose, J., Rosero, R., Rost, P. M., Rumleskie, J., Schumaker, M. A., Schwendener, M. H., Scislowski, D., Secrest, J., Seddighin, M., Segui, L., Seibert, S., Semenec, I., Shaker, F., Shantz, T., Sharma, M. K., Shokair, T. M., Sibley, L., Sinclair, J. R., Singh, K., Skensved, P., Smiley, M., Sonley, T., Sörensen, A., St-Amant, M., Stainforth, R., Stankiewicz, S., Strait, M., Stringer, M. I., Stripay, A., Svoboda, R., Tacchino, S., Tam, B., Tanguay, C., Tatar, J., Tian, L., Tolich, N., Tseng, J., Tseung, H. W. C., Turner, E., Van Berg, R., Vázquez-Jáuregui, E., Veinot, J. G. C., Virtue, C. J., von Krosigk, B., Walker, J. M. G., Walker, M., Wallig, J., Walton, S. C., Wang, J., Ward, M., Wasalski, O., Waterfield, J., Weigand, J. J., White, R. F., Wilson, J. R., Winchester, T. J., Woosaree, P., Wright, A., Yanez, J. P., Yeh, M., Zhang, T., Zhang, Y., Zhao, T., Zuber, K., and Zummo, A.

Subjects
Physics - Instrumentation and Detectors, High Energy Physics - Experiment, Nuclear Experiment
Abstract

The SNO+ experiment is located 2 km underground at SNOLAB in Sudbury, Canada. A low background search for neutrinoless double beta ($0\nu\beta\beta$) decay will be conducted using 780 tonnes of liquid scintillator loaded with 3.9 tonnes of natural tellurium, corresponding to 1.3 tonnes of $^{130}$Te. This paper provides a general overview of the SNO+ experiment, including detector design, construction of process plants, commissioning efforts, electronics upgrades, data acquisition systems, and calibration techniques. The SNO+ collaboration is reusing the acrylic vessel, PMT array, and electronics of the SNO detector, having made a number of experimental upgrades and essential adaptations for use with the liquid scintillator. With low backgrounds and a low energy threshold, the SNO+ collaboration will also pursue a rich physics program beyond the search for $0\nu\beta\beta$ decay, including studies of geo- and reactor antineutrinos, supernova and solar neutrinos, and exotic physics such as the search for invisible nucleon decay. The SNO+ approach to the search for $0\nu\beta\beta$ decay is scalable: a future phase with high $^{130}$Te-loading is envisioned to probe an effective Majorana mass in the inverted mass ordering region., Comment: 61 pages, 23 figures, 4 tables

Published
2021
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13. Development, characterisation, and deployment of the SNO+ liquid scintillator

Author

Collaboration, SNO, Anderson, M. R., Andringa, S., Anselmo, L., Arushanova, E., Asahi, S., Askins, M., Auty, D. J., Back, A. R., Barnard, Z., Barros, N., Bartlett, D., Barão, F., Bayes, R., Beier, E. W., Bialek, A., Biller, S. D., Blucher, E., Bonventre, R., Boulay, M., Braid, D., Caden, E., Callaghan, E. J., Caravaca, J., Carvalho, J., Cavalli, L., Chauhan, D., Chen, M., Chkvorets, O., Clark, K. J., Cleveland, B., Cookman, D., Connors, C., Coulter, I. T., Cox, M. A., Cressy, D., Dai, X., Darrach, C., Davis-Purcell, B., Deluce, C., Depatie, M. M., Descamps, F., Dittmer, J., Di Lodovico, F., Duhaime, N., Duncan, F., Dunger, J., Earle, A. D., Fabris, D., Falk, E., Farrugia, A., Fatemighomi, N., Fischer, V., Fletcher, E., Ford, R., Frankiewicz, K., Gagnon, N., Gaur, A., Gilje, K., González-Reina, O. I., Gooding, D., Gorel, P., Graham, K., Grant, C., Grove, J., Grullon, S., Guillian, E., Hall, S., Hallin, A. L., Hallman, D., Hans, S., Hartnell, J., Harvey, P., Hedayatipour, M., Heintzelman, W. J., Heise, J., Helmer, R. L., Horne, D., Hreljac, B., Hu, J., Hussain, A. S. M., Iida, T., Inácio, A. S., Jackson, M., Jelley, N. A., Jillings, C. J., Jones, C., Jones, P. G., Kamdin, K., Kaptanoglu, T., Kaspar, J., Keeter, K., Kefelian, C., Khaghani, P., Kippenbrock, L., Klein, J. R., Knapik, R., Kofron, J., Kormos, L. L., Korte, S., Krar, B., Kraus, C., Krauss, C. B., Kroupova, T., Labe, K., Lafleur, F., Lam, I., Lan, C., Land, B. J., Lane, R., Langrock, S., LaTorre, A., Lawson, I., Lebanowski, L., Lefeuvre, G. M., Leming, E. J., Li, A., Lidgard, J., Liggins, B., Lin, Y. H., Liu, X., Liu, Y., Lozza, V., Luo, M., Maguire, S., Maio, A., Majumdar, K., Manecki, S., Maneira, J., Martin, R. D., Marzec, E., Mastbaum, A., Mauel, J., McCauley, N., McDonald, A. B., Mekarski, P., Meyer, M., Miller, C., Mills, C., Mlejnek, M., Mony, E., Morton-Blake, I., Mottram, M. J., Nae, S., Nirkko, M., Nolan, L. J., Novikov, V. M., O'Keeffe, H. M., O'Sullivan, E., Gann, G. D. Orebi, Parnell, M. J., Paton, J., Peeters, S. J. M., Pershing, T., Petriw, Z., Petzoldt, J., Pickard, L., Pracsovics, D., Prior, G., Prouty, J. C., Quirk, S., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Robertson, A., Rose, J., Rosero, R., Rost, P. M., Rumleskie, J., Schumaker, M. A., Schwendener, M. H., Scislowski, D., Secrest, J., Seddighin, M., Segui, L., Seibert, S., Semenec, I., Shaker, F., Shantz, T., Sharma, M. K., Shokair, T. M., Sibley, L., Sinclair, J. R., Singh, K., Skensved, P., Smiley, M., Sonley, T., Stainforth, R., Strait, M., Stringer, M. I., Svoboda, R., Sörensen, A., Tam, B., Tatar, J., Tian, L., Tolich, N., Tseng, J., Tseung, H. W. C., Turner, E., Van Berg, R., Veinot, J. G. C., Virtue, C. J., von Krosigk, B., Vázquez-Jáuregui, E., Walker, J. M. G., Walker, M., Walton, S. C., Wang, J., Ward, M., Wasalski, O., Waterfield, J., Weigand, J. J., White, R. F., Wilson, J. R., Winchester, T. J., Woosaree, P., Wright, A., Yanez, J. P., Yeh, M., Zhang, T., Zhang, Y., Zhao, T., Zuber, K., and Zummo, A.

Subjects
Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract

A liquid scintillator consisting of linear alkylbenzene as the solvent and 2,5-diphenyloxazole as the fluor was developed for the SNO+ experiment. This mixture was chosen as it is compatible with acrylic and has a competitive light yield to pre-existing liquid scintillators while conferring other advantages including longer attenuation lengths, superior safety characteristics, chemical simplicity, ease of handling, and logistical availability. Its properties have been extensively characterized and are presented here. This liquid scintillator is now used in several neutrino physics experiments in addition to SNO+., Comment: 21 pages, 10 figures

Published
2020
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14. Optical calibration of the SNO+ detector in the water phase with deployed sources

Author

Anderson, MR, Andringa, S, Askins, M, Auty, DJ, Barão, F, Barros, N, Bayes, R, Beier, EW, Bialek, A, Biller, SD, Blucher, E, Boulay, M, Caden, E, Callaghan, EJ, Caravaca, J, Chen, M, Chkvorets, O, Cleveland, B, Cookman, D, Corning, J, Cox, MA, Deluce, C, Depatie, MM, Di Lodovico, F, Dittmer, J, Falk, E, Fatemighomi, N, Fischer, V, Ford, R, Frankiewicz, K, Gaur, A, Gilje, K, González-Reina, OI, Gooding, D, Grant, C, Grove, J, Hallin, AL, Hallman, D, Hartnell, J, Heintzelman, WJ, Helmer, RL, Hu, J, Hunt-Stokes, R, Hussain, SMA, Inácio, AS, Jillings, CJ, Kaptanoglu, T, Khaghani, P, Khan, H, Klein, JR, Kormos, LL, Krar, B, Kraus, C, Krauss, CB, Kroupová, T, Lam, I, Land, BJ, LaTorre, A, Lawson, I, Lebanowski, L, Lefebvre, C, Li, A, Lidgard, J, Lin, YH, Liu, Y, Lozza, V, Luo, M, Maio, A, Manecki, S, Maneira, J, Martin, RD, McCauley, N, McDonald, AB, Meyer, M, Mills, C, Morton-Blake, I, Nae, S, Nirkko, M, Nolan, LJ, O'Keeffe, HM, Gann, GD Orebi, Page, J, Parker, W, Paton, J, Peeters, SJM, Pershing, T, Pickard, L, Prior, G, Ravi, P, Reichold, A, Riccetto, S, Richardson, R, Rigan, M, Rose, J, Rumleskie, J, Semenec, I, Shaker, F, Sharma, MK, Skensved, P, and Smiley, M

Subjects
Nuclear and Plasma Physics, Particle and High Energy Physics, Synchrotrons and Accelerators, Physical Sciences, Analysis and statistical methods, Cherenkov detectors, Detector alignment and calibration methods, Neutrino detectors, Engineering, Nuclear & Particles Physics, Physical sciences
Abstract

SNO+ is a large-scale liquid scintillator experiment with the primary goal of searching for neutrinoless double beta decay, and is located approximately 2 km underground in SNOLAB, Sudbury, Canada. The detector acquired data for two years as a pure water Cherenkov detector, starting in May 2017. During this period, the optical properties of the detector were measured in situ using a deployed light diffusing sphere, with the goal of improving the detector model and the energy response systematic uncertainties. The measured parameters included the water attenuation coefficients, effective attenuation coefficients for the acrylic vessel, and the angular response of the photomultiplier tubes and their surrounding light concentrators, all across different wavelengths. The calibrated detector model was validated using a deployed tagged gamma source, which showed a 0.6% variation in energy scale across the primary target volume.

Published
2021

15. Development, characterisation, and deployment of the SNO+ liquid scintillator

Author

Anderson, MR, Andringa, S, Anselmo, L, Arushanova, E, Asahi, S, Askins, M, Auty, DJ, Back, AR, Barnard, Z, Barros, N, Bartlett, D, Barão, F, Bayes, R, Beier, EW, Bialek, A, Biller, SD, Blucher, E, Bonventre, R, Boulay, M, Braid, D, Caden, E, Callaghan, EJ, Caravaca, J, Carvalho, J, Cavalli, L, Chauhan, D, Chen, M, Chkvorets, O, Clark, KJ, Cleveland, B, Cookman, D, Connors, C, Coulter, IT, Cox, MA, Cressy, D, Dai, X, Darrach, C, Davis-Purcell, B, Deluce, C, Depatie, MM, Descamps, F, Dittmer, J, Di Lodovico, F, Duhaime, N, Duncan, F, Dunger, J, Earle, AD, Fabris, D, Falk, E, Farrugia, A, Fatemighomi, N, Fischer, V, Fletcher, E, Ford, R, Frankiewicz, K, Gagnon, N, Gaur, A, Gilje, K, González-Reina, OI, Gooding, D, Gorel, P, Graham, K, Grant, C, Grove, J, Grullon, S, Guillian, E, Hall, S, Hallin, AL, Hallman, D, Hans, S, Hartnell, J, Harvey, P, Hedayatipour, M, Heintzelman, WJ, Heise, J, Helmer, RL, Horne, D, Hreljac, B, Hu, J, Hussain, SMA, Iida, T, Inácio, AS, Jackson, CM, Jelley, NA, Jillings, CJ, Jones, C, Jones, PG, Kamdin, K, Kaptanoglu, T, Kaspar, J, Keeter, K, Kefelian, C, Khaghani, P, Kippenbrock, L, Klein, JR, Knapik, R, Kofron, J, Kormos, LL, Korte, S, and Krar, B

Subjects
Nuclear and Plasma Physics, Physical Sciences, Double-beta decay detectors, Neutrino detectors, Scintillators, scintillation and light emission processes (solid, gas and liquid scintillators), Engineering, Nuclear & Particles Physics, Physical sciences
Abstract

A liquid scintillator consisting of linear alkylbenzene as the solvent and 2,5-diphenyloxazole as the fluor was developed for the SNO+ experiment. This mixture was chosen as it is compatible with acrylic and has a competitive light yield to pre-existing liquid scintillators while conferring other advantages including longer attenuation lengths, superior safety characteristics, chemical simplicity, ease of handling, and logistical availability. Its properties have been extensively characterized and are presented here. This liquid scintillator is now used in several neutrino physics experiments in addition to SNO+.

Published
2021

16. Initial measurement of reactor antineutrino oscillation at SNO+

Author

Collaboration, SNO+, Allega, A., Anderson, M. R., Andringa, S., Askins, M., Auty, D. J., Bacon, A., Baker, J., Barão, F., Barros, N., Bayes, R., Beier, E. W., Bezerra, T. S., Bialek, A., Biller, S. D., Blucher, E., Caden, E., Callaghan, E. J., Chen, M., Cheng, S., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Dehghani, R., Deloye, J., Depatie, M. M., Di Lodovico, F., Dima, C., Dittmer, J., Dixon, K. H., Esmaeilian, M. S., Falk, E., Fatemighomi, N., Ford, R., Gaur, A., González-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hall, S., Hallin, A. L., Hallman, D., Heintzelman, W. J., Helmer, R. L., Hewitt, C., Howard, V., Hreljac, B., Hu, J., Huang, P., Hunt-Stokes, R., Hussain, S. M. A., Inácio, A. S., Jillings, C. J., Kaluzienski, S., Kaptanoglu, T., Khan, H., Kladnik, J., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupová, T., Lake, C., Lebanowski, L., Lefebvre, C., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Mills, C., Milton, G., Colina, A. Molina, Morris, D., Morton-Blake, I., Mubasher, M., Naugle, S., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Paleshi, K., Parker, W., Paton, J., Peeters, S. J. M., Pickard, L., Quenallata, B., Ravi, P., Reichold, A., Riccetto, S., Rose, J., Rosero, R., Semenec, I., Simms, J., Skensved, P., Smiley, M., Smith, J., Svoboda, R., Tam, B., Tseng, J., Vázquez-Jáuregui, E., Veinot, J. G. C., Virtue, C. J., Ward, M., Weigand, J. J., Wilson, J. R., Wilson, J. D., Wright, A., Yang, S., Yeh, M., Ye, Z., Yu, S., Zhang, Y., Zuber, K., Zummo, A., Collaboration, SNO+, Allega, A., Anderson, M. R., Andringa, S., Askins, M., Auty, D. J., Bacon, A., Baker, J., Barão, F., Barros, N., Bayes, R., Beier, E. W., Bezerra, T. S., Bialek, A., Biller, S. D., Blucher, E., Caden, E., Callaghan, E. J., Chen, M., Cheng, S., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Dehghani, R., Deloye, J., Depatie, M. M., Di Lodovico, F., Dima, C., Dittmer, J., Dixon, K. H., Esmaeilian, M. S., Falk, E., Fatemighomi, N., Ford, R., Gaur, A., González-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hall, S., Hallin, A. L., Hallman, D., Heintzelman, W. J., Helmer, R. L., Hewitt, C., Howard, V., Hreljac, B., Hu, J., Huang, P., Hunt-Stokes, R., Hussain, S. M. A., Inácio, A. S., Jillings, C. J., Kaluzienski, S., Kaptanoglu, T., Khan, H., Kladnik, J., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupová, T., Lake, C., Lebanowski, L., Lefebvre, C., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Mills, C., Milton, G., Colina, A. Molina, Morris, D., Morton-Blake, I., Mubasher, M., Naugle, S., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Paleshi, K., Parker, W., Paton, J., Peeters, S. J. M., Pickard, L., Quenallata, B., Ravi, P., Reichold, A., Riccetto, S., Rose, J., Rosero, R., Semenec, I., Simms, J., Skensved, P., Smiley, M., Smith, J., Svoboda, R., Tam, B., Tseng, J., Vázquez-Jáuregui, E., Veinot, J. G. C., Virtue, C. J., Ward, M., Weigand, J. J., Wilson, J. R., Wilson, J. D., Wright, A., Yang, S., Yeh, M., Ye, Z., Yu, S., Zhang, Y., Zuber, K., and Zummo, A.

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.

Published
2024

17. Evidence of antineutrinos from distant reactors using pure water at SNO

Author

Collaboration, SNO+, Allega, A., Anderson, M. R., Andringa, S., Antunes, J., Askins, M., Auty, D. J., Bacon, A., Barros, N., Barao, F., Bayes, R., Beier, E. W., Bezerra, T. S., Bialek, A., Biller, S. D., Blucher, E., Caden, E., Callaghan, E. J., Cheng, S., Chen, M., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Dehghani, R., Deloye, J., Deluce, C., Depatie, M. M., Dittmer, J., Dixon, K. H., Di Lodovico, F., Falk, E., Fatemighomi, N., Ford, R., Frankiewicz, K., Gaur, A., Gonzalez-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hallin, A. L., Hallman, D., Heintzelman, W. J., Helmer, R. L., Hu, J., Hunt-Stokes, R., Hussain, S. M. A., Inacio, A. S., Jillings, C. J., Kaluzienski, S., Kaptanoglu, T., Khaghani, P., Khan, H., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupova, T., Lam, I., Land, B. J., Lawson, I., Lebanowski, L., Lee, J., Lefebvre, C., Lidgard, J., Lin, Y. H., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Mills, C., Morton-Blake, I., Naugle, S., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Parker, W., Paton, J., Peeters, S. J. M., Pickard, L., Ravi, P., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Rose, J., Rosero, R., Rumleskie, J., Semenec, I., Skensved, P., Smiley, M., Svoboda, R., Tam, B., Tseng, J., Turner, E., Valder, S., Virtue, C. J., Vazquez-Jauregui, E., Wang, J., Ward, M., Wilson, J. R., Wilson, J. D., Wright, A., Yanez, J. P., Yang, S., Yeh, M., Yu, S., Zhang, Y., Zuber, K., Zummo, A., and Collaboration, The SNO +

Subjects
High Energy Physics - Experiment (hep-ex), FOS: Physical sciences, General Physics and Astronomy, Nuclear Experiment (nucl-ex), Nuclear Experiment, High Energy Physics - Experiment
Abstract

The SNO+ Collaboration reports the first evidence of reactor antineutrinos in a Cherenkov detector. The nearest nuclear reactors are located 240~km away in Ontario, Canada. This analysis uses events with energies lower than in any previous analysis with a large water Cherenkov detector. Two analytical methods are used to distinguish reactor antineutrinos from background events in 190 days of data and yield consistent evidence for antineutrinos with a combined significance of 3.5$\sigma$., Comment: v2: add missing author, add link to supplemental material v3: minor updates to match PRL publication

Published
2023
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18. Improved search for invisible modes of nucleon decay in water with the SNO+ detector

Author

Collaboration, SNO+, Allega, A., Anderson, M. R., Andringa, S., Askins, M., Auty, D. J., Bacon, A., Barros, N., Barão, F., Bayes, R., Beier, E. W., Bezerra, T. S., Bialek, A., Biller, S. D., Blucher, E., Caden, E., Callaghan, E. J., Cheng, S., Chen, M., Chkvorets, O., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Dehghani, R., Deluce, C., Depatie, M. M., Dittmer, J., Dixon, K. H., Di Lodovico, F., Falk, E., Fatemighomi, N., Ford, R., Frankiewicz, K., Gaur, A., González-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hallin, A. L., Hallman, D., Hartnell, J., Heintzelman, W. J., Helmer, R. L., Hu, J., Hunt-Stokes, R., Hussain, S. M. A., Inácio, A. S., Jillings, C. J., Kaptanoglu, T., Khaghani, P., Khan, H., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupová, T., Lam, I., Land, B. J., Lawson, I., Lebanowski, L., Lee, J., Lefebvre, C., Lidgard, J., Lin, Y. H., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Meyer, M., Mills, C., Morton-Blake, I., Naugle, S., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Parker, W., Paton, J., Peeters, S. J. M., Pickard, L., Ravi, P., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Rose, J., Rumleskie, J., Semenec, I., Skensved, P., Smiley, M., Svoboda, R., Tam, B., Tseng, J., Turner, E., Valder, S., Veinot, J. G. C., Virtue, C. J., Vázquez-Jáuregui, E., Wang, J., Ward, M., Weigand, J. J., Wilson, J. D., Wilson, J. R., Wright, A., Yanez, J. P., Yang, S., Yeh, M., Yu, S., Zhang, T., Zhang, Y., Zuber, K., Zummo, A., Collaboration, SNO+, Allega, A., Anderson, M. R., Andringa, S., Askins, M., Auty, D. J., Bacon, A., Barros, N., Barão, F., Bayes, R., Beier, E. W., Bezerra, T. S., Bialek, A., Biller, S. D., Blucher, E., Caden, E., Callaghan, E. J., Cheng, S., Chen, M., Chkvorets, O., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Dehghani, R., Deluce, C., Depatie, M. M., Dittmer, J., Dixon, K. H., Di Lodovico, F., Falk, E., Fatemighomi, N., Ford, R., Frankiewicz, K., Gaur, A., González-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hallin, A. L., Hallman, D., Hartnell, J., Heintzelman, W. J., Helmer, R. L., Hu, J., Hunt-Stokes, R., Hussain, S. M. A., Inácio, A. S., Jillings, C. J., Kaptanoglu, T., Khaghani, P., Khan, H., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupová, T., Lam, I., Land, B. J., Lawson, I., Lebanowski, L., Lee, J., Lefebvre, C., Lidgard, J., Lin, Y. H., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Meyer, M., Mills, C., Morton-Blake, I., Naugle, S., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Parker, W., Paton, J., Peeters, S. J. M., Pickard, L., Ravi, P., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Rose, J., Rumleskie, J., Semenec, I., Skensved, P., Smiley, M., Svoboda, R., Tam, B., Tseng, J., Turner, E., Valder, S., Veinot, J. G. C., Virtue, C. J., Vázquez-Jáuregui, E., Wang, J., Ward, M., Weigand, J. J., Wilson, J. D., Wilson, J. R., Wright, A., Yanez, J. P., Yang, S., Yeh, M., Yu, S., Zhang, T., Zhang, Y., Zuber, K., and Zummo, A.

Abstract

This paper reports results from a search for single and multi-nucleon disappearance from the $^{16}$O nucleus in water within the \snoplus{} detector using all of the available data. These so-called "invisible" decays do not directly deposit energy within the detector but are instead detected through their subsequent nuclear de-excitation and gamma-ray emission. New limits are given for the partial lifetimes: $\tau(n\rightarrow inv) > 9.0\times10^{29}$ years, $\tau(p\rightarrow inv) > 9.6\times10^{29}$ years, $\tau(nn\rightarrow inv) > 1.5\times10^{28}$ years, $\tau(np\rightarrow inv) > 6.0\times10^{28}$ years, and $\tau(pp\rightarrow inv) > 1.1\times10^{29}$ years at 90\% Bayesian credibility level (with a prior uniform in rate). All but the ($nn\rightarrow inv$) results improve on existing limits by a factor of about 3.

Published
2022
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19. Evidence of Antineutrinos from Distant Reactors using Pure Water at SNO+

Author

Collaboration, SNO+, Allega, A., Anderson, M. R., Andringa, S., Antunes, J., Askins, M., Auty, D. J., Bacon, A., Barros, N., Barao, F., Bayes, R., Beier, E. W., Bezerra, T. S., Bialek, A., Biller, S. D., Blucher, E., Caden, E., Callaghan, E. J., Cheng, S., Chen, M., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Dehghani, R., Deloye, J., Deluce, C., Depatie, M. M., Dittmer, J., Dixon, K. H., Di Lodovico, F., Falk, E., Fatemighomi, N., Ford, R., Frankiewicz, K., Gaur, A., Gonzalez-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hallin, A. L., Hallman, D., Heintzelman, W. J., Helmer, R. L., Hu, J., Hunt-Stokes, R., Hussain, S. M. A., Inacio, A. S., Jillings, C. J., Kaluzienski, S., Kaptanoglu, T., Khaghani, P., Khan, H., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupova, T., Lam, I., Land, B. J., Lawson, I., Lebanowski, L., Lee, J., Lefebvre, C., Lidgard, J., Lin, Y. H., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Mills, C., Morton-Blake, I., Naugle, S., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Parker, W., Paton, J., Peeters, S. J. M., Pickard, L., Ravi, P., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Rose, J., Rosero, R., Rumleskie, J., Semenec, I., Skensved, P., Smiley, M., Svoboda, R., Tam, B., Tseng, J., Turner, E., Valder, S., Virtue, C. J., Vazquez-Jauregui, E., Wang, J., Ward, M., Wilson, J. R., Wilson, J. D., Wright, A., Yanez, J. P., Yang, S., Yeh, M., Yu, S., Zhang, Y., Zuber, K., Zummo, A., Collaboration, SNO+, Allega, A., Anderson, M. R., Andringa, S., Antunes, J., Askins, M., Auty, D. J., Bacon, A., Barros, N., Barao, F., Bayes, R., Beier, E. W., Bezerra, T. S., Bialek, A., Biller, S. D., Blucher, E., Caden, E., Callaghan, E. J., Cheng, S., Chen, M., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Dehghani, R., Deloye, J., Deluce, C., Depatie, M. M., Dittmer, J., Dixon, K. H., Di Lodovico, F., Falk, E., Fatemighomi, N., Ford, R., Frankiewicz, K., Gaur, A., Gonzalez-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hallin, A. L., Hallman, D., Heintzelman, W. J., Helmer, R. L., Hu, J., Hunt-Stokes, R., Hussain, S. M. A., Inacio, A. S., Jillings, C. J., Kaluzienski, S., Kaptanoglu, T., Khaghani, P., Khan, H., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupova, T., Lam, I., Land, B. J., Lawson, I., Lebanowski, L., Lee, J., Lefebvre, C., Lidgard, J., Lin, Y. H., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Mills, C., Morton-Blake, I., Naugle, S., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Parker, W., Paton, J., Peeters, S. J. M., Pickard, L., Ravi, P., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Rose, J., Rosero, R., Rumleskie, J., Semenec, I., Skensved, P., Smiley, M., Svoboda, R., Tam, B., Tseng, J., Turner, E., Valder, S., Virtue, C. J., Vazquez-Jauregui, E., Wang, J., Ward, M., Wilson, J. R., Wilson, J. D., Wright, A., Yanez, J. P., Yang, S., Yeh, M., Yu, S., Zhang, Y., Zuber, K., and Zummo, A.

Abstract

The SNO+ Collaboration reports the first evidence of reactor antineutrinos in a Cherenkov detector. The nearest nuclear reactors are located 240~km away in Ontario, Canada. This analysis uses events with energies lower than in any previous analysis with a large water Cherenkov detector. Two analytical methods are used to distinguish reactor antineutrinos from background events in 190 days of data and yield consistent evidence for antineutrinos with a combined significance of 3.5$\sigma$., Comment: v2: add missing author, add link to supplemental material v3: minor updates to match PRL publication

Published
2022
Full Text
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20. The SNO+ Experiment

Author

Collaboration, SNO+, Albanese, V., Alves, R., Anderson, M. R., Andringa, S., Anselmo, L., Arushanova, E., Asahi, S., Askins, M., Auty, D. J., Back, A. R., Back, S., Bar��o, F., Barnard, Z., Barr, A., Barros, N., Bartlett, D., Bayes, R., Beaudoin, C., Beier, E. W., Berardi, G., Bialek, A., Biller, S. D., Blucher, E., Bonventre, R., Boulay, M., Braid, D., Caden, E., Callaghan, E. J., Caravaca, J., Carvalho, J., Cavalli, L., Chauhan, D., Chen, M., Chkvorets, O., Clark, K. J., Cleveland, B., Connors, C., Cookman, D., Coulter, I. T., Cox, M. A., Cressy, D., Dai, X., Darrach, C., Davis-Purcell, B., Deluce, C., Depatie, M. M., Descamps, F., Di Lodovico, F., Dittmer, J., Doxtator, A., Duhaime, N., Duncan, F., Dunger, J., Earle, A. D., Fabris, D., Falk, E., Farrugia, A., Fatemighomi, N., Felber, C., Fischer, V., Fletcher, E., Ford, R., Frankiewicz, K., Gagnon, N., Gaur, A., Gauthier, J., Gibson-Foster, A., Gilje, K., Gonz��lez-Reina, O. I., Gooding, D., Gorel, P., Graham, K., Grant, C., Grove, J., Grullon, S., Guillian, E., Hall, S., Hallin, A. L., Hallman, D., Hans, S., Hartnell, J., Harvey, P., Hedayatipour, M., Heintzelman, W. J., Heise, J., Helmer, R. L., Hodak, B., Hodak, M., Hood, M., Horne, D., Hreljac, B., Hu, J., Hussain, S. M. A., Iida, T., In��cio, A. S., Jackson, C. M., Jelley, N. A., Jillings, C. J., Jones, C., Jones, P. G., Kamdin, K., Kaptanoglu, T., Kaspar, J., Keeter, K., Kefelian, C., Khaghani, P., Kippenbrock, L., Klein, J. R., Knapik, R., Kofron, J., Kormos, L. L., Korte, S., Krar, B., Kraus, C., Krauss, C. B., Kroupov��, T., Labe, K., Lafleur, F., Lam, I., Lan, C., Land, B. J., Lane, R., Langrock, S., Larochelle, P., Larose, S., LaTorre, A., Lawson, I., Lebanowski, L., Lefeuvre, G. M., Leming, E. J., Li, A., Li, O., Lidgard, J., Liggins, B., Liimatainen, P., Lin, Y. H., Liu, X., Liu, Y., Lozza, V., Luo, M., Maguire, S., Maio, A., Majumdar, K., Manecki, S., Maneira, J., Martin, R. D., Marzec, E., Mastbaum, A., Mathewson, A., McCauley, N., McDonald, A. B., McFarlane, K., Mekarski, P., Meyer, M., Miller, C., Mills, C., Mlejnek, M., Mony, E., Morissette, B., Morton-Blake, I., Mottram, M. J., Nae, S., Nirkko, M., Nolan, L. J., Novikov, V. M., O'Keeffe, H. M., O'Sullivan, E., Gann, G. D. Orebi, Parnell, M. J., Paton, J., Peeters, S. J. M., Pershing, T., Petriw, Z., Petzoldt, J., Pickard, L., Pracsovics, D., Prior, G., Prouty, J. C., Quirk, S., Read, S., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Ritchie, I., Robertson, A., Robertson, B. C., Rose, J., Rosero, R., Rost, P. M., Rumleskie, J., Schumaker, M. A., Schwendener, M. H., Scislowski, D., Secrest, J., Seddighin, M., Segui, L., Seibert, S., Semenec, I., Shaker, F., Shantz, T., Sharma, M. K., Shokair, T. M., Sibley, L., Sinclair, J. R., Singh, K., Skensved, P., Smiley, M., Sonley, T., S��rensen, A., St-Amant, M., Stainforth, R., Stankiewicz, S., Strait, M., Stringer, M. I., Stripay, A., Svoboda, R., Tacchino, S., Tam, B., Tanguay, C., Tatar, J., Tian, L., Tolich, N., Tseng, J., Tseung, H. W. C., Turner, E., Van Berg, R., V��zquez-J��uregui, E., Veinot, J. G. C., Virtue, C. J., von Krosigk, B., Walker, J. M. G., Walker, M., Wallig, J., Walton, S. C., Wang, J., Ward, M., Wasalski, O., Waterfield, J., Weigand, J. J., White, R. F., Wilson, J. R., Winchester, T. J., Woosaree, P., Wright, A., Yanez, J. P., Yeh, M., Zhang, T., Zhang, Y., Zhao, T., Zuber, K., and Zummo, A.

Subjects
High Energy Physics - Experiment (hep-ex), Physics::Instrumentation and Detectors, FOS: Physical sciences, High Energy Physics::Experiment, Instrumentation and Detectors (physics.ins-det), Nuclear Experiment (nucl-ex), Nuclear Experiment
Abstract

The SNO+ experiment is located 2 km underground at SNOLAB in Sudbury, Canada. A low background search for neutrinoless double beta ($0������$) decay will be conducted using 780 tonnes of liquid scintillator loaded with 3.9 tonnes of natural tellurium, corresponding to 1.3 tonnes of $^{130}$Te. This paper provides a general overview of the SNO+ experiment, including detector design, construction of process plants, commissioning efforts, electronics upgrades, data acquisition systems, and calibration techniques. The SNO+ collaboration is reusing the acrylic vessel, PMT array, and electronics of the SNO detector, having made a number of experimental upgrades and essential adaptations for use with the liquid scintillator. With low backgrounds and a low energy threshold, the SNO+ collaboration will also pursue a rich physics program beyond the search for $0������$ decay, including studies of geo- and reactor antineutrinos, supernova and solar neutrinos, and exotic physics such as the search for invisible nucleon decay. The SNO+ approach to the search for $0������$ decay is scalable: a future phase with high $^{130}$Te-loading is envisioned to probe an effective Majorana mass in the inverted mass ordering region., 61 pages, 23 figures, 4 tables

Published
2021
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21. The SNO+ experiment

Author

Albanese, V., additional, Alves, R., additional, Anderson, M.R., additional, Andringa, S., additional, Anselmo, L., additional, Arushanova, E., additional, Asahi, S., additional, Askins, M., additional, Auty, D.J., additional, Back, A.R., additional, Back, S., additional, Barão, F., additional, Barnard, Z., additional, Barr, A., additional, Barros, N., additional, Bartlett, D., additional, Bayes, R., additional, Beaudoin, C., additional, Beier, E.W., additional, Berardi, G., additional, Bialek, A., additional, Biller, S.D., additional, Blucher, E., additional, Bonventre, R., additional, Boulay, M., additional, Braid, D., additional, Caden, E., additional, Callaghan, E.J., additional, Caravaca, J., additional, Carvalho, J., additional, Cavalli, L., additional, Chauhan, D., additional, Chen, M., additional, Chkvorets, O., additional, Clark, K.J., additional, Cleveland, B., additional, Connors, C., additional, Cookman, D., additional, Coulter, I.T., additional, Cox, M.A., additional, Cressy, D., additional, Dai, X., additional, Darrach, C., additional, Davis-Purcell, B., additional, Deluce, C., additional, Depatie, M.M., additional, Descamps, F., additional, Di Lodovico, F., additional, Dittmer, J., additional, Doxtator, A., additional, Duhaime, N., additional, Duncan, F., additional, Dunger, J., additional, Earle, A.D., additional, Fabris, D., additional, Falk, E., additional, Farrugia, A., additional, Fatemighomi, N., additional, Felber, C., additional, Fischer, V., additional, Fletcher, E., additional, Ford, R., additional, Frankiewicz, K., additional, Gagnon, N., additional, Gaur, A., additional, Gauthier, J., additional, Gibson-Foster, A., additional, Gilje, K., additional, González-Reina, O.I., additional, Gooding, D., additional, Gorel, P., additional, Graham, K., additional, Grant, C., additional, Grove, J., additional, Grullon, S., additional, Guillian, E., additional, Hall, S., additional, Hallin, A.L., additional, Hallman, D., additional, Hans, S., additional, Hartnell, J., additional, Harvey, P., additional, Hedayatipour, M., additional, Heintzelman, W.J., additional, Heise, J., additional, Helmer, R.L., additional, Hodak, B., additional, Hodak, M., additional, Hood, M., additional, Horne, D., additional, Hreljac, B., additional, Hu, J., additional, Hussain, S.M.A., additional, Iida, T., additional, Inácio, A.S., additional, Jackson, C.M., additional, Jelley, N.A., additional, Jillings, C.J., additional, Jones, C., additional, Jones, P.G., additional, Kamdin, K., additional, Kaptanoglu, T., additional, Kaspar, J., additional, Keeter, K., additional, Kefelian, C., additional, Khaghani, P., additional, Kippenbrock, L., additional, Klein, J.R., additional, Knapik, R., additional, Kofron, J., additional, Kormos, L.L., additional, Korte, S., additional, Krar, B., additional, Kraus, C., additional, Krauss, C.B., additional, Kroupová, T., additional, Labe, K., additional, Lafleur, F., additional, Lam, I., additional, Lan, C., additional, Land, B.J., additional, Lane, R., additional, Langrock, S., additional, Larochelle, P., additional, Larose, S., additional, LaTorre, A., additional, Lawson, I., additional, Lebanowski, L., additional, Lefeuvre, G.M., additional, Leming, E.J., additional, Li, A., additional, Li, O., additional, Lidgard, J., additional, Liggins, B., additional, Liimatainen, P., additional, Lin, Y.H., additional, Liu, X., additional, Liu, Y., additional, Lozza, V., additional, Luo, M., additional, Maguire, S., additional, Maio, A., additional, Majumdar, K., additional, Manecki, S., additional, Maneira, J., additional, Martin, R.D., additional, Marzec, E., additional, Mastbaum, A., additional, Mathewson, A., additional, McCauley, N., additional, McDonald, A.B., additional, McFarlane, K., additional, Mekarski, P., additional, Meyer, M., additional, Miller, C., additional, Mills, C., additional, Mlejnek, M., additional, Mony, E., additional, Morissette, B., additional, Morton-Blake, I., additional, Mottram, M.J., additional, Nae, S., additional, Nirkko, M., additional, Nolan, L.J., additional, Novikov, V.M., additional, O'Keeffe, H.M., additional, O'Sullivan, E., additional, Orebi Gann, G.D., additional, Parnell, M.J., additional, Paton, J., additional, Peeters, S.J.M., additional, Pershing, T., additional, Petriw, Z., additional, Petzoldt, J., additional, Pickard, L., additional, Pracsovics, D., additional, Prior, G., additional, Prouty, J.C., additional, Quirk, S., additional, Read, S., additional, Reichold, A., additional, Riccetto, S., additional, Richardson, R., additional, Rigan, M., additional, Ritchie, I., additional, Robertson, A., additional, Robertson, B.C., additional, Rose, J., additional, Rosero, R., additional, Rost, P.M., additional, Rumleskie, J., additional, Schumaker, M.A., additional, Schwendener, M.H., additional, Scislowski, D., additional, Secrest, J., additional, Seddighin, M., additional, Segui, L., additional, Seibert, S., additional, Semenec, I., additional, Shaker, F., additional, Shantz, T., additional, Sharma, M.K., additional, Shokair, T.M., additional, Sibley, L., additional, Sinclair, J.R., additional, Singh, K., additional, Skensved, P., additional, Smiley, M., additional, Sonley, T., additional, Sörensen, A., additional, St-Amant, M., additional, Stainforth, R., additional, Stankiewicz, S., additional, Strait, M., additional, Stringer, M.I., additional, Stripay, A., additional, Svoboda, R., additional, Tacchino, S., additional, Tam, B., additional, Tanguay, C., additional, Tatar, J., additional, Tian, L., additional, Tolich, N., additional, Tseng, J., additional, Tseung, H.W.C., additional, Turner, E., additional, Van Berg, R., additional, Vázquez-Jáuregui, E., additional, Veinot, J.G.C., additional, Virtue, C.J., additional, von Krosigk, B., additional, Walker, J.M.G., additional, Walker, M., additional, Wallig, J., additional, Walton, S.C., additional, Wang, J., additional, Ward, M., additional, Wasalski, O., additional, Waterfield, J., additional, Weigand, J.J., additional, White, R.F., additional, Wilson, J.R., additional, Winchester, T.J., additional, Woosaree, P., additional, Wright, A., additional, Yanez, J.P., additional, Yeh, M., additional, Zhang, T., additional, Zhang, Y., additional, Zhao, T., additional, Zuber, K., additional, and Zummo, A., additional

Published
2021
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22. Development, characterisation, and deployment of the SNO+ liquid scintillator

Author

Anderson, Anderson, MR, Andringa, S, Anselmo, L, Arushanova, E, Asahi, S, Askins, M, Auty, DJ, Back, AR, Barnard, Z, Barros, N, Bartlett, D, Barao, F, Bayes, R, Beier, EW, Bialek, A, Biller, SD, Blucher, E, Bonventre, R, Boulay, M, Braid, D, Caden, E, Callaghan, EJ, Caravaca, J, Carvalho, J, Cavalli, L, Chauhan, D, Chen, M, Chkvorets, O, Clark, KJ, Cleveland, B, Cookman, D, Connors, C, Coulter, IT, Cox, MA, Cressy, D, Dai, X, Darrach, C, Davis-Purcell, B, Deluce, C, Depatie, MM, Descamps, F, Dittmer, J, Di Lodovico, F, Duhaime, N, Duncan, F, Dunger, J, Earle, AD, Fabris, D, Falk, E, Farrugia, A, Fatemighomi, N, Fischer, V, Fletcher, E, Ford, R, Frankiewicz, K, Gagnon, N, Gaur, A, Gilje, K, González-Reina, OI, Gooding, D, Gorel, P, Graham, K, Grant, C, Grove, J, Grullon, S, Guillian, E, Hall, S, Hallin, AL, Hallman, D, Hans, S, Hartnell, J, Harvey, P, Hedayatipour, M, Heintzelman, WJ, Heise, J, Helmer, RL, Horne, D, Hreljac, B, Hu, J, Hussain, SMA, Iida, T, Inácio, AS, Jackson, CM, Jelley, NA, Jillings, CJ, Jones, C, Jones, PG, Kamdin, K, Kaptanoglu, T, Kaspar, J, Keeter, K, Kefelian, C, Khaghani, P, Kippenbrock, L, Klein, JR, Knapik, R, Kofron, J, Kormos, LL, Korte, S, Krar, B, Anderson, Anderson, MR, Andringa, S, Anselmo, L, Arushanova, E, Asahi, S, Askins, M, Auty, DJ, Back, AR, Barnard, Z, Barros, N, Bartlett, D, Barao, F, Bayes, R, Beier, EW, Bialek, A, Biller, SD, Blucher, E, Bonventre, R, Boulay, M, Braid, D, Caden, E, Callaghan, EJ, Caravaca, J, Carvalho, J, Cavalli, L, Chauhan, D, Chen, M, Chkvorets, O, Clark, KJ, Cleveland, B, Cookman, D, Connors, C, Coulter, IT, Cox, MA, Cressy, D, Dai, X, Darrach, C, Davis-Purcell, B, Deluce, C, Depatie, MM, Descamps, F, Dittmer, J, Di Lodovico, F, Duhaime, N, Duncan, F, Dunger, J, Earle, AD, Fabris, D, Falk, E, Farrugia, A, Fatemighomi, N, Fischer, V, Fletcher, E, Ford, R, Frankiewicz, K, Gagnon, N, Gaur, A, Gilje, K, González-Reina, OI, Gooding, D, Gorel, P, Graham, K, Grant, C, Grove, J, Grullon, S, Guillian, E, Hall, S, Hallin, AL, Hallman, D, Hans, S, Hartnell, J, Harvey, P, Hedayatipour, M, Heintzelman, WJ, Heise, J, Helmer, RL, Horne, D, Hreljac, B, Hu, J, Hussain, SMA, Iida, T, Inácio, AS, Jackson, CM, Jelley, NA, Jillings, CJ, Jones, C, Jones, PG, Kamdin, K, Kaptanoglu, T, Kaspar, J, Keeter, K, Kefelian, C, Khaghani, P, Kippenbrock, L, Klein, JR, Knapik, R, Kofron, J, Kormos, LL, Korte, S, and Krar, B

Abstract

A liquid scintillator consisting of linear alkylbenzene as the solvent and 2,5-diphenyloxazole as the fluor was developed for the SNO+ experiment. This mixture was chosen as it is compatible with acrylic and has a competitive light yield to pre-existing liquid scintillators while conferring other advantages including longer attenuation lengths, superior safety characteristics, chemical simplicity, ease of handling, and logistical availability. Its properties have been extensively characterized and are presented here. This liquid scintillator is now used in several neutrino physics experiments in addition to SNO+.

Published
2021

23. Optical calibration of the SNO+ detector in the water phase with deployed sources

Author

Collaboration, SNO+, Anderson, M. R., Andringa, S., Askins, M., Auty, D. J., Barão, F., Barros, N., Bayes, R., Beier, E. W., Bialek, A., Biller, S. D., Blucher, E., Boulay, M., Caden, E., Callaghan, E. J., Caravaca, J., Chen, M., Chkvorets, O., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Deluce, C., Depatie, M. M., Di Lodovico, F., Dittmer, J., Falk, E., Fatemighomi, N., Fischer, V., Ford, R., Frankiewicz, K., Gaur, A., Gilje, K., González-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hallin, A. L., Hallman, D., Hartnell, J., Heintzelman, W. J., Helmer, R. L., Hu, J., Hunt-Stokes, R., Hussain, S. M. A., Inácio, A. S., Jillings, C. J., Kaptanoglu, T., Khaghani, P., Khan, H., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupová, T., Lam, I., Land, B. J., LaTorre, A., Lawson, I., Lebanowski, L., Lefebvre, C., Li, A., Lidgard, J., Lin, Y. H., Liu, Y., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Meyer, M., Mills, C., Morton-Blake, I., Nae, S., Nirkko, M., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Parker, W., Paton, J., Peeters, S. J. M., Pershing, T., Pickard, L., Prior, G., Ravi, P., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Rose, J., Rumleskie, J., Semenec, I., Shaker, F., Sharma, M. K., Skensved, P., Smiley, M., Stainforth, R., Svoboda, R., Tam, B., Tseng, J., Turner, E., Valder, S., Vázquez-Jáuregui, E., Veinot, J. G. C., Virtue, C. J., Wang, J., Ward, M., Weigand, J. J., Wilson, J. R., Wright, A., Yanez, J. P., Yeh, M., Yu, S., Zhang, T., Zhang, Y., Zuber, K., Zummo, A., Collaboration, SNO+, Anderson, M. R., Andringa, S., Askins, M., Auty, D. J., Barão, F., Barros, N., Bayes, R., Beier, E. W., Bialek, A., Biller, S. D., Blucher, E., Boulay, M., Caden, E., Callaghan, E. J., Caravaca, J., Chen, M., Chkvorets, O., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Deluce, C., Depatie, M. M., Di Lodovico, F., Dittmer, J., Falk, E., Fatemighomi, N., Fischer, V., Ford, R., Frankiewicz, K., Gaur, A., Gilje, K., González-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hallin, A. L., Hallman, D., Hartnell, J., Heintzelman, W. J., Helmer, R. L., Hu, J., Hunt-Stokes, R., Hussain, S. M. A., Inácio, A. S., Jillings, C. J., Kaptanoglu, T., Khaghani, P., Khan, H., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupová, T., Lam, I., Land, B. J., LaTorre, A., Lawson, I., Lebanowski, L., Lefebvre, C., Li, A., Lidgard, J., Lin, Y. H., Liu, Y., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Meyer, M., Mills, C., Morton-Blake, I., Nae, S., Nirkko, M., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Parker, W., Paton, J., Peeters, S. J. M., Pershing, T., Pickard, L., Prior, G., Ravi, P., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Rose, J., Rumleskie, J., Semenec, I., Shaker, F., Sharma, M. K., Skensved, P., Smiley, M., Stainforth, R., Svoboda, R., Tam, B., Tseng, J., Turner, E., Valder, S., Vázquez-Jáuregui, E., Veinot, J. G. C., Virtue, C. J., Wang, J., Ward, M., Weigand, J. J., Wilson, J. R., Wright, A., Yanez, J. P., Yeh, M., Yu, S., Zhang, T., Zhang, Y., Zuber, K., and Zummo, A.

Abstract

SNO+ is a large-scale liquid scintillator experiment with the primary goal of searching for neutrinoless double beta decay, and is located approximately 2 km underground in SNOLAB, Sudbury, Canada. The detector acquired data for two years as a pure water Cherenkov detector, starting in May 2017. During this period, the optical properties of the detector were measured in situ using a deployed light diffusing sphere, with the goal of improving the detector model and the energy response systematic uncertainties. The measured parameters included the water attenuation coefficients, effective attenuation coefficients for the acrylic vessel, and the angular response of the photomultiplier tubes and their surrounding light concentrators, all across different wavelengths. The calibrated detector model was validated using a deployed tagged gamma source, which showed a 0.6% variation in energy scale across the primary target volume., Comment: Accepted by JINST (30 pages, 19 figures)

Published
2021
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24. Development, characterisation, and deployment of the SNO+ liquid scintillator

Author

Collaboration, SNO+, Anderson, M. R., Andringa, S., Anselmo, L., Arushanova, E., Asahi, S., Askins, M., Auty, D. J., Back, A. R., Barnard, Z., Barros, N., Bartlett, D., Barão, F., Bayes, R., Beier, E. W., Bialek, A., Biller, S. D., Blucher, E., Bonventre, R., Boulay, M., Braid, D., Caden, E., Callaghan, E. J., Caravaca, J., Carvalho, J., Cavalli, L., Chauhan, D., Chen, M., Chkvorets, O., Clark, K. J., Cleveland, B., Cookman, D., Connors, C., Coulter, I. T., Cox, M. A., Cressy, D., Dai, X., Darrach, C., Davis-Purcell, B., Deluce, C., Depatie, M. M., Descamps, F., Dittmer, J., Di Lodovico, F., Duhaime, N., Duncan, F., Dunger, J., Earle, A. D., Fabris, D., Falk, E., Farrugia, A., Fatemighomi, N., Fischer, V., Fletcher, E., Ford, R., Frankiewicz, K., Gagnon, N., Gaur, A., Gilje, K., González-Reina, O. I., Gooding, D., Gorel, P., Graham, K., Grant, C., Grove, J., Grullon, S., Guillian, E., Hall, S., Hallin, A. L., Hallman, D., Hans, S., Hartnell, J., Harvey, P., Hedayatipour, M., Heintzelman, W. J., Heise, J., Helmer, R. L., Horne, D., Hreljac, B., Hu, J., Hussain, A. S. M., Iida, T., Inácio, A. S., Jackson, M., Jelley, N. A., Jillings, C. J., Jones, C., Jones, P. G., Kamdin, K., Kaptanoglu, T., Kaspar, J., Keeter, K., Kefelian, C., Khaghani, P., Kippenbrock, L., Klein, J. R., Knapik, R., Kofron, J., Kormos, L. L., Korte, S., Krar, B., Kraus, C., Krauss, C. B., Kroupova, T., Labe, K., Lafleur, F., Lam, I., Lan, C., Land, B. J., Lane, R., Langrock, S., LaTorre, A., Lawson, I., Lebanowski, L., Lefeuvre, G. M., Leming, E. J., Li, A., Lidgard, J., Liggins, B., Lin, Y. H., Liu, X., Liu, Y., Lozza, V., Luo, M., Maguire, S., Maio, A., Majumdar, K., Manecki, S., Maneira, J., Martin, R. D., Marzec, E., Mastbaum, A., Mauel, J., McCauley, N., McDonald, A. B., Mekarski, P., Meyer, M., Miller, C., Mills, C., Mlejnek, M., Mony, E., Morton-Blake, I., Mottram, M. J., Nae, S., Nirkko, M., Nolan, L. J., Novikov, V. M., O'Keeffe, H. M., O'Sullivan, E., Gann, G. D. Orebi, Parnell, M. J., Paton, J., Peeters, S. J. M., Pershing, T., Petriw, Z., Petzoldt, J., Pickard, L., Pracsovics, D., Prior, G., Prouty, J. C., Quirk, S., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Robertson, A., Rose, J., Rosero, R., Rost, P. M., Rumleskie, J., Schumaker, M. A., Schwendener, M. H., Scislowski, D., Secrest, J., Seddighin, M., Segui, L., Seibert, S., Semenec, I., Shaker, F., Shantz, T., Sharma, M. K., Shokair, T. M., Sibley, L., Sinclair, J. R., Singh, K., Skensved, P., Smiley, M., Sonley, T., Stainforth, R., Strait, M., Stringer, M. I., Svoboda, R., Sörensen, A., Tam, B., Tatar, J., Tian, L., Tolich, N., Tseng, J., Tseung, H. W. C., Turner, E., Van Berg, R., Veinot, J. G. C., Virtue, C. J., von Krosigk, B., Vázquez-Jáuregui, E., Walker, J. M. G., Walker, M., Walton, S. C., Wang, J., Ward, M., Wasalski, O., Waterfield, J., Weigand, J. J., White, R. F., Wilson, J. R., Winchester, T. J., Woosaree, P., Wright, A., Yanez, J. P., Yeh, M., Zhang, T., Zhang, Y., Zhao, T., Zuber, K., Zummo, A., Collaboration, SNO+, Anderson, M. R., Andringa, S., Anselmo, L., Arushanova, E., Asahi, S., Askins, M., Auty, D. J., Back, A. R., Barnard, Z., Barros, N., Bartlett, D., Barão, F., Bayes, R., Beier, E. W., Bialek, A., Biller, S. D., Blucher, E., Bonventre, R., Boulay, M., Braid, D., Caden, E., Callaghan, E. J., Caravaca, J., Carvalho, J., Cavalli, L., Chauhan, D., Chen, M., Chkvorets, O., Clark, K. J., Cleveland, B., Cookman, D., Connors, C., Coulter, I. T., Cox, M. A., Cressy, D., Dai, X., Darrach, C., Davis-Purcell, B., Deluce, C., Depatie, M. M., Descamps, F., Dittmer, J., Di Lodovico, F., Duhaime, N., Duncan, F., Dunger, J., Earle, A. D., Fabris, D., Falk, E., Farrugia, A., Fatemighomi, N., Fischer, V., Fletcher, E., Ford, R., Frankiewicz, K., Gagnon, N., Gaur, A., Gilje, K., González-Reina, O. I., Gooding, D., Gorel, P., Graham, K., Grant, C., Grove, J., Grullon, S., Guillian, E., Hall, S., Hallin, A. L., Hallman, D., Hans, S., Hartnell, J., Harvey, P., Hedayatipour, M., Heintzelman, W. J., Heise, J., Helmer, R. L., Horne, D., Hreljac, B., Hu, J., Hussain, A. S. M., Iida, T., Inácio, A. S., Jackson, M., Jelley, N. A., Jillings, C. J., Jones, C., Jones, P. G., Kamdin, K., Kaptanoglu, T., Kaspar, J., Keeter, K., Kefelian, C., Khaghani, P., Kippenbrock, L., Klein, J. R., Knapik, R., Kofron, J., Kormos, L. L., Korte, S., Krar, B., Kraus, C., Krauss, C. B., Kroupova, T., Labe, K., Lafleur, F., Lam, I., Lan, C., Land, B. J., Lane, R., Langrock, S., LaTorre, A., Lawson, I., Lebanowski, L., Lefeuvre, G. M., Leming, E. J., Li, A., Lidgard, J., Liggins, B., Lin, Y. H., Liu, X., Liu, Y., Lozza, V., Luo, M., Maguire, S., Maio, A., Majumdar, K., Manecki, S., Maneira, J., Martin, R. D., Marzec, E., Mastbaum, A., Mauel, J., McCauley, N., McDonald, A. B., Mekarski, P., Meyer, M., Miller, C., Mills, C., Mlejnek, M., Mony, E., Morton-Blake, I., Mottram, M. J., Nae, S., Nirkko, M., Nolan, L. J., Novikov, V. M., O'Keeffe, H. M., O'Sullivan, E., Gann, G. D. Orebi, Parnell, M. J., Paton, J., Peeters, S. J. M., Pershing, T., Petriw, Z., Petzoldt, J., Pickard, L., Pracsovics, D., Prior, G., Prouty, J. C., Quirk, S., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Robertson, A., Rose, J., Rosero, R., Rost, P. M., Rumleskie, J., Schumaker, M. A., Schwendener, M. H., Scislowski, D., Secrest, J., Seddighin, M., Segui, L., Seibert, S., Semenec, I., Shaker, F., Shantz, T., Sharma, M. K., Shokair, T. M., Sibley, L., Sinclair, J. R., Singh, K., Skensved, P., Smiley, M., Sonley, T., Stainforth, R., Strait, M., Stringer, M. I., Svoboda, R., Sörensen, A., Tam, B., Tatar, J., Tian, L., Tolich, N., Tseng, J., Tseung, H. W. C., Turner, E., Van Berg, R., Veinot, J. G. C., Virtue, C. J., von Krosigk, B., Vázquez-Jáuregui, E., Walker, J. M. G., Walker, M., Walton, S. C., Wang, J., Ward, M., Wasalski, O., Waterfield, J., Weigand, J. J., White, R. F., Wilson, J. R., Winchester, T. J., Woosaree, P., Wright, A., Yanez, J. P., Yeh, M., Zhang, T., Zhang, Y., Zhao, T., Zuber, K., and Zummo, A.

Abstract

A liquid scintillator consisting of linear alkylbenzene as the solvent and 2,5-diphenyloxazole as the fluor was developed for the SNO+ experiment. This mixture was chosen as it is compatible with acrylic and has a competitive light yield to pre-existing liquid scintillators while conferring other advantages including longer attenuation lengths, superior safety characteristics, chemical simplicity, ease of handling, and logistical availability. Its properties have been extensively characterized and are presented here. This liquid scintillator is now used in several neutrino physics experiments in addition to SNO+., Comment: 21 pages, 10 figures

Published
2020
Full Text
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