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Search for radiative decays of Υ(1S) into η and η

S. B. Athar1, R. Patel1, V. Potlia1, H. Stoeck1, J. Yelton1, P. Rubin2, C. Cawlfield3, B. I. Eisenstein3, I. Karliner3 et al. (CLEO Collaboration)

I. Karliner3, D. Kim3, N. Lowrey3, P. Naik3, C. Sedlack3, M. Selen3, E. J. White3, J. Wiss3, M. R. Shepherd4, D. Besson5, T. K. Pedlar6, D. Cronin-Hennessy7, K. Y. Gao7, D. T. Gong7, J. Hietala7, Y. Kubota7, T. Klein7, B. W. Lang7, R. Poling7, A. W. Scott7, A. Smith7, S. Dobbs8, Z. Metreveli8, K. K. Seth8, A. Tomaradze8, P. Zweber8, J. Ernst9, H. Severini10, S. A. Dytman11, W. Love11, V. Savinov11, O. Aquines12, Z. Li12, A. Lopez12, S. Mehrabyan12, H. Mendez12, J. Ramirez12, G. S. Huang13, D. H. Miller13, V. Pavlunin13, B. Sanghi13, I. P. J. Shipsey13, B. Xin13, G. S. Adams14, M. Anderson14, J. P. Cummings14, I. Danko14, J. Napolitano14, Q. He15, J. Insler15, H. Muramatsu15, C. S. Park15, E. H. Thorndike15, T. E. Coan16, Y. S. Gao16, F. Liu16, M. Artuso17, S. Blusk17, J. Butt17, J. Li17, N. Menaa17, R. Mountain17, S. Nisar17, K. Randrianarivony17, R. Redjimi17, R. Sia17, T. Skwarnicki17, S. Stone17, J. C. Wang17, K. Zhang17, S. E. Csorna18, G. Bonvicini19, D. Cinabro19, M. Dubrovin19, A. Lincoln19, D. M. Asner20, K. W. Edwards20, R. A. Briere21, I. Brock21, J. Chen21, T. Ferguson21, G. Tatishvili21, H. Vogel21, M. E. Watkins21, J. L. Rosner22, N. E. Adam23, J. P. Alexander23, K. Berkelman23, D. G. Cassel23, J. E. Duboscq23, K. M. Ecklund23, R. Ehrlich23, L. Fields23, R. S. Galik23, L. Gibbons23, R. Gray23, S. W. Gray23, D. L. Hartill23, B. K. Heltsley23, D. Hertz23, C. D. Jones23, J. Kandaswamy23, D. L. Kreinick23, V. E. Kuznetsov23, H. Mahlke-Krüger23, T. O. Meyer23, P. U. E. Onyisi23, J. R. Patterson23, D. Peterson23, J. Pivarski23, D. Riley23, A. Ryd23, A. J. Sadoff23, H. Schwarthoff23, X. Shi23, S. Stroiney23, W. M. Sun23, T. Wilksen23, and M. Weinberger23 (CLEO Collaboration)

  • 1University of Florida, Gainesville, Florida 32611, USA
  • 2George Mason University, Fairfax, Virginia 22030, USA
  • 3University of Illinois, Urbana-Champaign, Illinois 61801, USA
  • 4Indiana University, Bloomington, Indiana 47405, USA
  • 5University of Kansas, Lawrence, Kansas 66045, USA
  • 6Luther College, Decorah, Iowa 52101, USA
  • 7University of Minnesota, Minneapolis, Minnesota 55455, USA
  • 8Northwestern University, Evanston, Illinois 60208, USA
  • 9State University of New York at Albany, Albany, New York 12222, USA
  • 10University of Oklahoma, Norman, Oklahoma 73019, USA
  • 11University of Pittsburgh, Pittsburgh, Pennsylvania 15260, USA
  • 12University of Puerto Rico, Mayaguez, Puerto Rico 00681
  • 13Purdue University, West Lafayette, Indiana 47907, USA
  • 14Rensselaer Polytechnic Institute, Troy, New York 12180, USA
  • 15University of Rochester, Rochester, New York 14627, USA
  • 16Southern Methodist University, Dallas, Texas 75275, USA
  • 17Syracuse University, Syracuse, New York 13244, USA
  • 18Vanderbilt University, Nashville, Tennessee 37235, USA
  • 19Wayne State University, Detroit, Michigan 48202, USA
  • 20Carleton University, Ottawa, Ontario, Canada K1S 5B6
  • 21Carnegie Mellon University, Pittsburgh, Pennsylvania 15213, USA
  • 22Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA
  • 23Cornell University, Ithaca, New York 14853

Phys. Rev. D 76, 072003 – Published 11 October, 2007

DOI: https://doi.org/10.1103/PhysRevD.76.072003

Abstract

We report on a search for the radiative decay of Υ(1S) to the pseudoscalar mesons η and η in (21.2±0.2)×106 Υ(1S) decays collected with the CLEO III detector at the Cornell Electron Storage Ring. The η meson was reconstructed in the three modes ηγγ, ηπ+ππ0, or ηπ0π0π0. The η meson was reconstructed in the mode ηπ+πη with η decaying through any of the above three modes, and also ηγρ0, where ρ0π+π. Five out of the seven submodes are found to have very low backgrounds. In four of them we find no signal candidates and in one [Υ(1S)γη, ηπ+πη, ηπ+ππ0] there are two good signal candidates, which is insufficient evidence to claim a signal. The other two submodes (ηγγ and ηγρ) are background limited, and show no excess of events in their signal regions. We combine the results from different channels and obtain upper limits at the 90% C.L. which are B(Υ(1S)γη)<1.0×106 and B(Υ(1S)γη)<1.9×106. Our limits are an order of magnitude tighter than the previous ones and below the predictions made by some theoretical models.

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