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

Autor: Anderson, M, Andringa, S, 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, Connors, C, Coulter, IT, Cressy, D, Dai, X, Darrach, C, Davis-Purcell, B, Depatie, MM, Descamps, F, Di Lodovico, F, Duhaime, N, Duncan, F, Dunger, J, Falk, E, Fatemighomi, N, Fischer, V, Fletcher, E, Ford, R, Gagnon, N, Gilje, K, Gorel, P, Graham, K, Grant, C, Grove, J, Grullon, S, Guillian, E, Hallin, AL, Hallman, D, Hans, S, Hartnell, J, Harvey, P, Hedayatipour, M, Heintzelman, WJ, Heise, J, Helmer, RL, Hernández-Hernández, JL, Hreljac, B, Hu, J, 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, Krar, B, Kraus, C, Krauss, CB, Kroupova, T, Labe, K, Lam, I, Lan, C, Land, BJ, Lane, R, Langrock, S, Latorre, A, Lawson, I, Lebanowski, L, Lefeuvre, GM, Leming, EJ, Li, A
Rok vydání: 2019
Předmět:
Zdroj: Physical Review D, vol 99, iss 3
Popis: 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 deexcite, often emitting detectable gamma rays. A search for such gamma rays yields limits of 2.5×1029 y at 90% Bayesian credibility level (with a prior uniform in rate) for the partial lifetime of the neutron, and 3.6×1029 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 1.3×1028 y for nn, 2.6×1028 y for pn and 4.7×1028 y for pp, an improvement over existing limits by close to 3 orders of magnitude for the latter two.
Databáze: OpenAIRE