SNO+ CollaborationA. AllegaM. R. AndersonS. AndringaM. AskinsD. J. AutyA. BaconN. BarrosF. BarãoR. BayesE. W. BeierT. S. BezerraA. BialekS. D. BillerE. BlucherE. CadenE. J. CallaghanS. ChengM. ChenO. ChkvoretsB. ClevelandD. CookmanJ. CorningM. A. CoxR. DehghaniC. DeluceM. M. DepatieJ. DittmerK. H. DixonF. Di LodovicoE. FalkN. FatemighomiR. FordK. FrankiewiczA. GaurO. I. González-ReinaD. GoodingC. GrantJ. GroveA. L. HallinD. HallmanJ. HartnellW. J. HeintzelmanR. L. HelmerJ. HuR. Hunt-StokesS. M. A. HussainA. S. InácioC. J. JillingsT. KaptanogluP. KhaghaniH. KhanJ. R. KleinL. L. KormosB. KrarC. KrausC. B. KraussT. KroupováI. LamB. J. LandI. LawsonL. LebanowskiJ. LeeC. LefebvreJ. LidgardY. H. LinV. LozzaM. LuoA. MaioS. ManeckiJ. ManeiraR. D. MartinN. McCauleyA. B. McDonaldM. MeyerC. MillsI. Morton-BlakeS. NaugleL. J. NolanH. M. O'KeeffeG. D. Orebi GannJ. PageW. ParkerJ. PatonS. J. M. PeetersL. PickardP. RaviA. ReicholdS. RiccettoR. RichardsonM. RiganJ. RoseJ. RumleskieI. SemenecP. SkensvedM. SmileyR. SvobodaB. TamJ. TsengE. TurnerS. ValderJ. G. C. VeinotC. J. VirtueE. Vázquez-JáureguiJ. WangM. WardJ. J. WeigandJ. D. WilsonJ. R. WilsonA. WrightJ. P. YanezS. YangM. YehS. YuT. ZhangY. ZhangK. ZuberA. Zummo2023-07-142023-07-142022-06-27http://hdl.handle.net/10400.26/45468This 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.engjournal article10.1103/PhysRevD.105.112012