# Search for invisible modes of nucleon decay in water with the SNO+   detector

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

arXiv: 1812.05552 · 2019-08-12

## TL;DR

This study searches for invisible nucleon decay modes in water using the SNO+ detector, setting new limits on the partial lifetimes of protons, neutrons, and dinucleon modes, significantly improving previous constraints.

## Contribution

It provides the first limits on invisible nucleon decay modes using the SNO+ detector and enhances existing bounds by up to three orders of magnitude.

## Key findings

- Limits of $2.5 	imes 10^{29}$ y for neutron decay
- Limits of $3.6 	imes 10^{29}$ y for proton decay
- Order-of-magnitude improvements for dinucleon modes

## Abstract

This paper reports results from a search for nucleon decay through 'invisible' modes, where no visible energy is directly deposited during the decay itself, during the initial water phase of SNO+. However, such decays within the oxygen nucleus would produce an excited daughter that would subsequently de-excite, often emitting detectable gamma rays. A search for such gamma rays yields limits of $2.5 \times 10^{29}$ y at 90% Bayesian credibility level (with a prior uniform in rate) for the partial lifetime of the neutron, and $3.6 \times 10^{29}$ y for the partial lifetime of the proton, the latter a 70% improvement on the previous limit from SNO. We also present partial lifetime limits for invisible dinucleon modes of $1.3\times 10^{28}$ y for $nn$, $2.6\times 10^{28}$ y for $pn$ and $4.7\times 10^{28}$ y for $pp$, an improvement over existing limits by close to three orders of magnitude for the latter two.

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1812.05552/full.md

## References

36 references — full list in the complete paper: https://tomesphere.com/paper/1812.05552/full.md

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Source: https://tomesphere.com/paper/1812.05552