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Observation of the P-1(1) state of charmonium

Authors :
Rubin, P.
Cawlfield, C.
Eisenstein, B. I.
Gollin, G. D.
Karliner, I.
Kim, D.
Lowrey, N.
Naik, P.
Sedlack, C.
Selen, M.
White, E. J.
Williams, J.
Wiss, J.
Edwards, K. W.
Besson, D.
Pedlar, T. K.
Cronin-Hennessy, D.
Gao, K. Y.
Gong, D. T.
Hietala, J.
Kubota, Y.
Klein, T.
Lang, B. W.
Li, S. Z.
Poling, R.
Scott, A. W.
Smith, A.
Dobbs, S.
Metreveli, Z.
Seth, K. K.
Tomaradze, A.
Zweber, P.
Ernst, J.
Mahmood, A. H.
Severini, H.
Asner, D. M.
Dytman, S. A.
Love, W.
Mehrabyan, S.
Mueller, J. A.
Savinov, V.
Li, Z.
Lopez, A.
Mendez, H.
Ramirez, J.
Huang, G. S.
Miller, D. H.
Pavlunin, V.
Sanghi, B.
Shipsey, I. P. J.
Adams, G. S.
Cravey, M.
Cummings, J. P.
Danko, I.
Napolitano, J.
He, Q.
Muramatsu, H.
Park, C. S.
Park, W.
Thorndike, E. H.
Coan, T. E.
Gao, Y. S.
Liu, F.
Artuso, M.
Boulahouache, C.
Blusk, S.
Butt, J.
Dorjkhaidav, O.
Li, J.
Menaa, N.
Mountain, R.
Nandakumar, R.
Randrianarivony, K.
Redjimi, R.
Sia, R.
Skwarnicki, T.
Stone, S.
Wang, J. C.
Zhang, K.
Csorna, S. E.
Bonvicini, G.
Cinabro, D.
Dubrovin, M.
Briere, R. A.
Chen, G. P.
Chen, J.
Ferguson, T.
Tatishvili, G.
Vogel, H.
Watkins, M. E.
Rosner, J. L.
Adam, N. E.
Alexander, J. P.
Berkelman, K.
Cassel, D. G.
Crede, V.
Duboscq, J. E.
Ecklund, K. M.
Ehrlich, R.
Fields, L.
Galik, R. S.
Gibbons, L.
Gittelman, B.
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.
Meyer, T. O.
Onyisi, P. U. E.
Patterson, J. R.
Peterson, D.
Phillips, E. A.
Pivarski, J.
Riley, D.
Ryd, A.
Sadoff, A. J.
Schwarthoff, H.
Shi, X.
Shepherd, M. R.
Stroiney, S.
Sun, W. M.
Urner, D.
Wilksen, T.
Weaver, K. M.
Weinberger, M.
Athar, S. B.
Avery, P.
Breva-Newell, L.
Patel, R.
Potlia, V.
Stoeck, H.
Yelton, J.
Source :
Department of Physics and Astronomy Faculty Publications
Publication Year :
2005
Publisher :
Purdue University, 2005.

Abstract

The spin-singlet P-wave state of charmonium, h(c)(P-1(1)), has been observed in the decay psi(2S)->pi(0)h(c) followed by h(c)->gamma eta(c). Inclusive and exclusive analyses of the M(h(c)) spectrum have been performed. Two complementary inclusive analyses select either a range of energies for the photon emitted in h(c)->gamma eta(c) or a range of values of M(eta(c)). These analyses, consistent with one another within statistics, yield M(h(c))=[3524.9 +/- 0.7 (stat)+/- 0.4 (sys)] MeV/c(2) and a product of the branching ratios B-psi(psi(2S)->pi(0)h(c))xB(h)(h(c)->gamma eta(c))=[3.5 +/- 1.0 (stat)+/- 0.7 (sys)]x10(-4). When the eta(c) is reconstructed in seven exclusive decay modes, 17.5 +/- 4.5 h(c) events are seen with an average mass M(h(c))=[3523.6 +/- 0.9 (stat)+/- 0.5 (sys)] MeV/c(2), and BpsiBh=[5.3 +/- 1.5 (stat)+/- 1.0 (sys)]x10(-4). If combined, the inclusive and exclusive data samples yield an overall mass M(h(c))=[3524.4 +/- 0.6 (stat)+/- 0.4 (sys)] MeV/c(2) and product of branching ratios BpsiBh=[4.0 +/- 0.8 (stat)+/- 0.7 (sys)]x10(-4). The h(c) mass implies a P-wave hyperfine splitting Delta M-HF(1P)equivalent to < M(1(3)P)>-M(1(1)P(1))=[1.0 +/- 0.6 (stat)+/- 0.4 (sys)] MeV/c(2).

Details

Database :
OpenAIRE
Journal :
Department of Physics and Astronomy Faculty Publications
Accession number :
edsair.od.......540..e2506b51b65002d3481890e928629f20