Decay of the ψ ( 3770 ) to light hadrons
2006; American Physical Society; Volume: 73; Issue: 1 Linguagem: Inglês
10.1103/physrevd.73.012002
ISSN1550-7998
AutoresG. S. Adams, Mark Anderson, J. P. Cummings, I. Dankó, J. Napolitano, Q. He, H. Muramatsu, C. S. Park, E. H. Thorndike, T. E. Coan, Yang Gao, F. Liu, M. Artuso, C. Boulahouache, S. Blusk, J. Butt, O. Dorjkhaidav, J. Li, N. Menaa, R. Mountain, R. Nandakumar, K. Randrianarivony, R. Redjimi, R. Sia, T. Skwarnicki, S. Stone, J. C. Wang, K. Zhang, S. E. Csorna, G. Bonvicini, D. Cinabro, M. Dubrovin, A. Lincoln, R. A. Briere, G. P. Chen, J. Chen, T. Ferguson, G. Tatishvili, H. Vogel, M. E. Watkins, J. L. Rosner, N. E. Adam, J. P. Alexander, K. Berkelman, D. G. Cassel, V. Credé, J. E. Duboscq, K. M. Ecklund, R. Ehrlich, L. Fields, R. S. Galik, L. Gibbons, B. Gittelman, R. Gray, S. W. Gray, D. L. Hartill, B. K. Heltsley, D. Hertz, C. D. Jones, J. Kandaswamy, D. L. Kreinick, В. Е. Кузнецов, H. Mahlke-Krüger, T. O. Meyer, P. U. E. Onyisi, J. R. Patterson, D. Peterson, E. A. Phillips, J. Pivarski, D. Riley, A. Rýd, A. J. Sadoff, H. Schwarthoff, X. Shi, M. R. Shepherd, S. Stroiney, W. Sun, D. Urner, T. Wilksen, K. M. Weaver, M. Weinberger, S. B. Athar, P. Avery, L. Breva-Newell, R. Patel, V. Potlia, H. Stoeck, J. Yelton, P. Rubin, C. Cawlfield, B. I. Eisenstein, G. D. Gollin, I. Karliner, D. Kim, N. Lowrey, P. Naik, C. Sedlack, M. Selen, E. J. White, J. S. Williams, J. Wiss, D. M. Asner, K. W. Edwards, D. Besson, T. K. Pedlar, D. Cronin-Hennessy, K. Y. Gao, D. T. Gong, J. Hietala, Y. Kubota, T. Klein, B. W. Lang, S. Z. Li, R. Poling, A. W. Scott, A. Smith, S. Dobbs, Z. Metreveli, K. K. Seth, A. Tomaradze, P. Zweber, J. Ernst, H. Severini, S. Dytman, W. A. Love, S. Mehrabyan, J. Mueller, V. Savinov, Z. Li, A. Lopez, H. Méndez, J. E. Ramirez Vargas, G. S. Huang, D. H. Miller, V. Pavlunin, B. Sanghi, I. P. J. Shipsey,
Tópico(s)Dark Matter and Cosmic Phenomena
ResumoWe describe a search for ψ(3770) decay to two-body non-D¯¯¯D final states in e+e− data produced by the CESR collider and analyzed with the CLEO-c detector. Vector-pseudoscalar production ρ0π0, ρ+π−, ωπ0, ϕπ0, ρη, ωη, ϕη, ρη′, ωη′, ϕη′, K*0¯¯¯¯¯K0, and K*+K− is studied along with that of b1π (b01π0 and b+1π−) and π+π−π0. The largest amount of disagreement between the expected rate for e+e−→γ∗→X and that for e+e−→X at √s=3.773 GeV is found for X=ϕη, at an excess cross section of (2.4±0.6) pb [Γψ(3770)ϕη=(7.4±1.6) keV], and a suggestive suppression is seen for π+π−π0 and ρπ. We conclude with form factor determinations for ωπ0, ρη, and ρη′.Received 9 September 2005DOI:https://doi.org/10.1103/PhysRevD.73.012002©2006 American Physical Society
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