Decay D0K»0

C. Bebek, K. Berkelman, E. Blucher, D. G. Cassel, T. Copie, R. Desalvo, J. W. Dewire, R. Ehrlich, R. S. Galik, M. G.D. Gilchriese, B. Gittelman, S. W. Gray, A. M. Halling, D. L. Hartill, B. K. Heltsley, S. Holzner, M. Ito, J. Kandaswamy, R. Kowalewski, D. L. KreinickY. Kubota, N. B. Mistry, J. Mueller, E. Nordberg, M. Ogg, D. Peterson, D. Perticone, M. Pisharody, K. Read, D. Riley, A. Silverman, P. C. Stein, S. Stone, A. J. Sadoff, P. Avery, D. Besson, T. Bowcock, R. T. Giles, J. Hassard, K. Kinoshita, F. M. Pipkin, Richard Wilson, P. Haas, M. Hempstead, T. Jensen, H. Kagan, R. Kass, S. Behrends, T. Gentile, Jan M. Guida, Joan A. Guida, F. Morrow, R. Poling, C. Rosenfeld, E. H. Thorndike, P. Tipton, J. Green, R. Namjoshi, F. Sannes, R. Stone, M. S. Alam, N. Katayama, I. J. Kim, C. R. Sun, V. Tanikella, D. Bortoletto, A. Chen, L. Garren, M. Goldberg, N. Horwitz, A. Jawahery, P. Lubrano, G. C. Moneti, S. E. Csorna, M. D. Mestayer, R. S. Panvini, G. B. Word, Xia Yi, A. Bean, G. J. Bobbink, I. Brock, A. Engler, T. Ferguson, R. Kraemer, C. Rippich, R. Sutton, H. Vogel

Research output: Contribution to journalArticle

31 Scopus citations

Abstract

We have observed a signal for the decay D0'K»0. We find that a broad threshold enhancement in the K+K- mass spectrum in the decay D0'K+K-K»0 is the main source of background to the D0'K»0 signal. Accounting for this background, we obtain the branching fraction B(D0'K»0)=(1.18±0. 40±0.17)%.

Original languageEnglish (US)
Pages (from-to)1893-1896
Number of pages4
JournalPhysical Review Letters
Volume56
Issue number18
DOIs
StatePublished - Jan 1 1986
Externally publishedYes

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ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Bebek, C., Berkelman, K., Blucher, E., Cassel, D. G., Copie, T., Desalvo, R., Dewire, J. W., Ehrlich, R., Galik, R. S., Gilchriese, M. G. D., Gittelman, B., Gray, S. W., Halling, A. M., Hartill, D. L., Heltsley, B. K., Holzner, S., Ito, M., Kandaswamy, J., Kowalewski, R., ... Vogel, H. (1986). Decay D0K»0. Physical Review Letters, 56(18), 1893-1896. https://doi.org/10.1103/PhysRevLett.56.1893