Observation of D+ → ρ(770)0μ+v

We report the first observation of the Cabibo disfavored semileptonic decay mode D+ → ρ(770)0μ+v and measure its decay rate relative to the Cabibbo favored mode D+ → K̄∗ (892)0 μ+v to be Λ(D+ → ρ(770)0 μ+vΛ(D+ → K̄∗ (892)0 μ+v) = 0.0440.031−0.025(stat.) ± 0.014 (syst.). The results are compared to t...

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Published inPhysics letters. B Vol. 316; no. 2-3; pp. 455 - 462
Main Authors Kodama, K., Ushida, N., Paolone, V.S., Volk, J.T., Wilcox, J.O., Yager, P.M., Edelstein, R.M., Freyberger, A.P., Gibaut, D.B., Lipton, R.J., Nichols, W.R., Potter, D.M., Russ, J.C., Zhang, C., Zhang, Y., Jang, H.I., Kim, J.Y., Kim, T.I., Lim, I.T., Pac, M.Y., Baller, B.R., Stefanski, R.J., Nakazawa, K., Chung, K.S., Chung, S.H., Kim, D.C., Park, I.G., Park, M.S., Song, J.S., Yoon, C.S., Chikawa, M., Abe, T., Aoki, S., Fujii, T., Fujioka, G., Fujiwara, K., Hara, T., Taruma, K., Yokoyama, C., Chang, S.D., Cheon, B.G., Cho, J.H., Kang, J.S., Kim, C.O., Kim, K.Y., Kim, T.Y., Lee, J.C., Lee, S.B., Nam, S.W., Shin, T.S., Sim, K.S., Woo, J.K., Isokane, Y., Tsuneoka, Y., Hoshino, K., Kitamura, H., Kobayashi, M., Miyanishi, M., Nakamura, K., Nakamura, M., Nakanishi, S., Niu, K., Niwa, K., Nomura, M., Okada, K., Tajima, H., Toshitou, T., Aryal, M., Dunlea, J.M., Frederiksen, S.G., Kuramata, S., Lundberg, B.G., Oleynik, G.A., Reay, N.W., Sidwell, R.A., Stanton, N.R., Moriyama, K., Shibata, H., Kalbfleisch, G.R., Skubic, P., Smow, J.M., Kusumoto, O., Ohashi, S., Teranaka, M., Tominaga, T., Yoshida, T., Okabe, H., Yokota, J., Ikegami, S., Kazuno, M., Koya, T., Ogawa, S., Shibuya, H., Watanabe, S., Sato, Y., Seshimo, M., Tezuka, I., Bahk, S.Y., Kim, S.K.
Format Journal Article
LanguageEnglish
Published Elsevier B.V 21.10.1993
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Summary:We report the first observation of the Cabibo disfavored semileptonic decay mode D+ → ρ(770)0μ+v and measure its decay rate relative to the Cabibbo favored mode D+ → K̄∗ (892)0 μ+v to be Λ(D+ → ρ(770)0 μ+vΛ(D+ → K̄∗ (892)0 μ+v) = 0.0440.031−0.025(stat.) ± 0.014 (syst.). The results are compared to theoretical predictions and to previous experimental upper limits.
ISSN:0370-2693
1873-2445
DOI:10.1016/0370-2693(93)90351-H