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chi(cJ) decays to h(+)h(-)h(0)

Authors :
Athar, S. B.
Patel, R.
Potlia, V.
Yelton, J.
Rubin, P.
Cawlfield, C.
Eisenstein, B. I.
Karliner, I.
Kim, D.
Lowrey, N.
Naik, P.
Selen, M.
White, E. J.
Wiss, J.
Mitchell, R. E.
Shepherd, M. R.
Besson, D.
Pedlar, T. K.
Cronin-Hennessy, D.
Gao, K. Y.
Hietala, J.
Kubota, Y.
Klein, T.
Lang, B. W.
Poling, R.
Scott, A. W.
Smith, A.
Zweber, P.
Dobbs, S.
Metreveli, Z.
Seth, K. K.
Tomaradze, A.
Ernst, J.
Ecklund, K. M.
Severini, H.
Love, W.
Savinov, V.
Aquines, O.
Li, Z.
Lopez, A.
Mehrabyan, S.
Mendez, H.
Ramirez, J.
Huang, G. S.
Miller, D. H.
Pavlunin, V.
Sanghi, B.
Shipsey, I. P. J.
Xin, B.
Adams, G. S.
Anderson, M.
Cummings, J. P.
Danko, I.
Hu, D.
Moziak, B.
Napolitano, J.
He, Q.
Insler, J.
Muramatsu, H.
Park, C. S.
Thorndike, E. H.
Yang, F.
Coan, T. E.
Gao, Y. S.
Artuso, M.
Blusk, S.
Butt, J.
Li, J.
Menaa, N.
Mountain, R.
Nisar, S.
Randrianarivony, K.
Sia, R.
Skwarnicki, T.
Stone, S.
Wang, J. C.
Zhang, K.
Bonvicini, G.
Cinabro, D.
Dubrovin, M.
Lincoln, A.
Asner, D. M.
Edwards, K. W.
Briere, R. A.
Ferguson, T.
Tatishvili, G.
Vogel, H.
Watkins, M. E.
Rosner, J. L.
Adam, N. E.
Alexander, J. P.
Cassel, D. G.
Duboscq, J. E.
Ehrlich, R.
Fields, L.
Gibbons, L.
Gray, R.
Gray, S. W.
Hartill, D. L.
Heltsley, B. K.
Hertz, D.
Jones, C. D.
Kandaswamy, J.
Kreinick, D. L.
Kuznetsov, V. E.
Mahlke-Kruger, H.
Onyisi, P. U. E.
Patterson, J. R.
Peterson, D.
Pivarski, J.
Riley, D.
Ryd, A.
Sadoff, A. J.
Schwarthoff, H.
Shi, X.
Stroiney, S.
Sun, W. M.
Wilksen, T.
Weinberger, M.
Source :
Department of Physics and Astronomy Faculty Publications
Publication Year :
2007
Publisher :
Purdue University, 2007.

Abstract

Using a sample of 3 X 10(6) psi(2S) decays recorded by the CLEO detector, we study three-body decays of the X(c)0, X-c1, and X-c2 produced in radiative decays of the psi(2S). We consider the final states pi(+) pi(-) eta, K+ K- eta pp eta, pi(+) pi(-) eta', K+ K- pi(0), pp pi(0), pi(+) K- K-S(0) and K+ p Lambda , measuring branching fractions or placing upper limits. For X-c1 -> pi(+) pi(-) eta, K+ K- pi(0), and pi(+) K- K-S(0) our observed samples are large enough to indicate the largest contributions to the substructure.

Details

Database :
OpenAIRE
Journal :
Department of Physics and Astronomy Faculty Publications
Accession number :
edsair.od.......540..21e1499927c3ef1ef88febcd15864be5