Inclusive [Formula Presented] production from the [Formula Presented]

M. Artuso, C. Boulahouache, S. Blusk, K. Bukin, E. Dambasuren, R. Mountain, H. Muramatsu, R. Nandakumar, T. Skwarnicki, S. Stone, J. C. Wang, B. Gittelman, S. W. Gray, D. L. Hartill, B. K. Heltsley, L. Hsu, C. D. Jones, J. Kandaswamy, D. L. Kreinick, A. MagerkurthH. Mahlke-Krüger, T. O. Meyer, N. B. Mistry, J. R. Patterson, D. Peterson, J. Pivarski, S. J. Richichi, D. Riley, A. J. Sadoff, H. Schwarthoff, M. R. Shepherd, J. G. Thayer, D. Urner, T. Wilksen, A. Warburton, M. Weinberger

Research output: Contribution to journalArticlepeer-review


Using the CLEO II detector at CESR, we measure the (Formula presented) energy spectra in (Formula presented) decays that we compare with models of the (Formula presented) form factor. This form factor, especially at large (Formula presented) energies, may provide an explanation of the large rate for (Formula presented) Our data do not support a large anomalous coupling at higher (Formula presented) and thus the large (Formula presented) rate remains a mystery, possibly requiring a non-standard-model explanation.

Original languageEnglish (US)
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Issue number5
StatePublished - 2003

ASJC Scopus subject areas

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)


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