Ahmed S N, Anthony A E, Beier E W, Bellerive A, Biller S D, Boger J, Boulay M G, Bowler M G, Bowles T J, Brice S J, Bullard T V, Chan Y D, Chen M, Chen X, Cleveland B T, Cox G A, Dai X, Dalnoki-Veress F, Doe P J, Dosanjh R S, Doucas G, Dragowsky M R, Duba C A, Duncan F A, Dunford M, Dunmore J A, Earle E D, Elliott S R, Evans H C, Ewan G T, Farine J, Fergani H, Fleurot F, Formaggio J A, Fowler M M, Frame K, Frati W, Fulsom B G, Gagnon N, Graham K, Grant D R, Hahn R L, Hall J C, Hallin A L, Hallman E D, Hamer A S, Handler W B, Hargrove C K, Harvey P J, Hazama R, Heeger K M, Heintzelman W J, Heise J, Helmer R L, Hemingway R J, Hime A, Howe M A, Jagam P, Jelley N A, Klein J R, Kos M S, Krumins A V, Kutter T, Kyba C C M, Labranche H, Lange R, Law J, Lawson I T, Lesko K T, Leslie J R, Levine I, Luoma S, MacLellan R, Majerus S, Mak H B, Maneira J, Marino A D, McCauley N, McDonald A B, McGee S, McGregor G, Mifflin C, Miknaitis K K S, Miller G G, Moffat B A, Nally C W, Neubauer M S, Nickel B G, Noble A J, Norman E B, Oblath N S, Okada C E, Ollerhead R W, Orrell J L, Oser S M, Ouellet C, Peeters S J M, Poon A W P, Robertson B C, Robertson R G H, Rollin E, Rosendahl S S E, Rusu V L, Schwendener M H, Simard O, Simpson J J, Sims C J, Sinclair D, Skensved P, Smith M W E, Starinsky N, Stokstad R G, Stonehill L C, Tafirout R, Takeuchi Y, Tesić G, Thomson M, Thorman M, Van Berg R, Van de Water R G, Virtue C J, Wall B L, Waller D, Waltham C E, Tseung H Wan Chan, Wark D L, West N, Wilhelmy J B, Wilkerson J F, Wilson J R, Wittich P, Wouters J M, Yeh M, Zuber K
Department of Physics, Queen's University, Kingston, Ontario, Canada K7L 3N6.
Phys Rev Lett. 2004 Mar 12;92(10):102004. doi: 10.1103/PhysRevLett.92.102004. Epub 2004 Mar 10.
Data from the Sudbury Neutrino Observatory have been used to constrain the lifetime for nucleon decay to "invisible" modes, such as n-->3nu. The analysis was based on a search for gamma rays from the deexcitation of the residual nucleus that would result from the disappearance of either a proton or neutron from 16O. A limit of tau(inv)>2 x 10(29) yr is obtained at 90% confidence for either neutron- or proton-decay modes. This is about an order of magnitude more stringent than previous constraints on invisible proton-decay modes and 400 times more stringent than similar neutron modes.
萨德伯里中微子观测站的数据已被用于限制核子衰变到“不可见”模式的寿命,例如n→3ν。该分析基于对16O中质子或中子消失后剩余核退激产生的伽马射线的搜索。在90%置信度下,对于中子或质子衰变模式,得到τ(inv)>2×10(29)年的限制。这比之前对不可见质子衰变模式的限制严格约一个数量级,比类似的中子模式严格400倍。