Constraints on Nucleon Decay via “Invisible” Modes from the Sudbury Neutrino Observatory

dc.contributor.authorAhmed, S. N.
dc.contributor.authorAnthony, A. E.
dc.contributor.authorBeier, E. W.
dc.contributor.authorBellerive, A.
dc.contributor.authorBiller, S. D.
dc.contributor.authorBoger, J.
dc.contributor.authorBoulay, M. G.
dc.contributor.authorBowler, M. G.
dc.contributor.authorBowles, T. J.
dc.contributor.authorBrice, S. J.
dc.contributor.authorBullard, T. V.
dc.contributor.authorChan, Y. D.
dc.contributor.authorChen, M.
dc.contributor.authorChen, X.
dc.contributor.authorCleveland, B. T.
dc.contributor.authorCox, G. A.
dc.contributor.authorDai, X.
dc.contributor.authorDalnoki-Veress, F.
dc.contributor.authorDoe, P. J.
dc.contributor.authorDosanjh, R. S.
dc.contributor.authorDoucas, G.
dc.contributor.authorDragowsky, M. R.
dc.contributor.authorDuba, C. A.
dc.contributor.authorDuncan, F. A.
dc.contributor.authorDunford, M.
dc.contributor.authorDunmore, J. A.
dc.contributor.authorEarle, E. D.
dc.contributor.authorElliott, S. R.
dc.contributor.authorEvans, H. C.
dc.contributor.authorEwan, G. T.
dc.contributor.authorFarine, J.
dc.contributor.authorFergani, H.
dc.contributor.authorFleurot, F.
dc.contributor.authorFormaggio, J. A.
dc.contributor.authorFowler, M. M.
dc.contributor.authorFrame, K.
dc.contributor.authorFrati, W.
dc.contributor.authorFulsom, B. G.
dc.contributor.authorGagnon, N.
dc.contributor.authorGraham, K.
dc.contributor.authorGrant, D. R.
dc.contributor.authorHahn, R. L.
dc.contributor.authorHall, J. C.
dc.contributor.authorHallin, A. L.
dc.contributor.authorHallman, E. D.
dc.contributor.authorHamer, A. S.
dc.contributor.authorHandler, W. B.
dc.contributor.authorHargrove, C. K.
dc.contributor.authorHarvey, P. J.
dc.contributor.authorHazama, R.
dc.contributor.authorHeeger, K. M.
dc.contributor.authorHeintzelman, W. J.
dc.contributor.authorHeise, J.
dc.contributor.authorHelmer, R. L.
dc.contributor.authorHemingway, R. J.
dc.contributor.authorHime, A.
dc.contributor.authorHowe, M. A.
dc.contributor.authorJagam, P.
dc.contributor.authorJelley, N. A.
dc.contributor.authorKlein, J. R.
dc.contributor.authorKos, M. S.
dc.contributor.authorKrumins, A. V.
dc.contributor.authorKutter, T.
dc.contributor.authorKyba, C. C. M.
dc.contributor.authorLabranche, H.
dc.contributor.authorLange, R.
dc.contributor.authorLaw, J.
dc.contributor.authorLawson, I. T.
dc.contributor.authorLesko, K. T.
dc.contributor.authorLeslie, J. R.
dc.contributor.authorLevine, Ilan
dc.contributor.authorLuoma, S.
dc.contributor.authorMacLellan, R.
dc.contributor.authorMajerus, S.
dc.contributor.authorMak, H. B.
dc.contributor.authorManeira, J.
dc.contributor.authorMarino, A. D.
dc.contributor.authorMcCauley, N.
dc.contributor.authorMcDonald, A. B.
dc.contributor.authorMcGee, S.
dc.contributor.authorMcGregor, G.
dc.contributor.authorMifflin, C.
dc.contributor.authorMiknaitis, K. K. S.
dc.contributor.authorMiller, G. G.
dc.contributor.authorMoffat, B. A.
dc.contributor.authorNally, C. W.
dc.contributor.authorNeubauer, M. S.
dc.contributor.authorNickel, B. G.
dc.contributor.authorNoble, A. J.
dc.contributor.authorNorman, E. B.
dc.contributor.authorOblath, N. S.
dc.contributor.authorOkada, C. E.
dc.contributor.authorOllerhead, R. W.
dc.contributor.authorOrrell, J. L.
dc.contributor.authorOser, S. M.
dc.contributor.authorOuellet, C.
dc.contributor.authorPeeters, S. J. M.
dc.contributor.authorPoon, A. W. P.
dc.contributor.authorRobertson, B. C.
dc.contributor.authorRobertson, R. G. H.
dc.contributor.authorRollin, E.
dc.contributor.authorRosendahl, S. S. E.
dc.contributor.authorRusu, V. L.
dc.contributor.authorSchwendener, M. H.
dc.contributor.authorSimard, O.
dc.contributor.authorSimpson, J. J.
dc.contributor.authorSims, C. J.
dc.contributor.authorSinclair, D.
dc.contributor.authorSkensved, P.
dc.contributor.authorSmith, M. W. E.
dc.contributor.authorStarinsky, N.
dc.contributor.authorStokstad, R. G.
dc.contributor.authorStonehill, L. C.
dc.contributor.authorTafirout, R.
dc.contributor.authorTakeuchi, Y.
dc.contributor.authorTešić, G.
dc.contributor.authorThomson, M.
dc.contributor.authorThorman, M.
dc.contributor.authorVan Berg, R.
dc.contributor.authorVan de Water, R. G.
dc.contributor.authorVirtue, C. J.
dc.contributor.authorWall, B. L.
dc.contributor.authorWaller, D.
dc.contributor.authorWaltham, C. E.
dc.contributor.authorWan Chan Tseung, H.
dc.contributor.authorWark, D. L.
dc.contributor.authorWest, N.
dc.contributor.authorWilhelmy, J. B.
dc.contributor.authorWilkerson, J. F.
dc.contributor.authorWilson, J. R.
dc.contributor.authorWittich, P.
dc.contributor.authorWouters, J. M.
dc.contributor.authorYeh, M.
dc.contributor.authorZuber, K.
dc.date.accessioned2020-12-07T19:56:00Z
dc.date.available2020-12-07T19:56:00Z
dc.date.issued2004
dc.description.abstractData from the Sudbury Neutrino Observatory have been used to constrain the lifetime for nucleon decay to “invisible” modes, such as n -> 3v. The analysis was based on a search for y-rays from the de-excitation of the residual nucleus that would result from the disappearance of either a proton or neutron from ^16O. A limit of t inv > 2×1029 years 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.en
dc.identifier.urihttps://hdl.handle.net/2022/25983
dc.language.isoenen
dc.publisherPhysical Reviewen
dc.subject.lcshParticles (Nuclear physics)en
dc.titleConstraints on Nucleon Decay via “Invisible” Modes from the Sudbury Neutrino Observatoryen
dc.typeArticleen

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