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Observation of D(0) → K+pi-

dc.contributor.authorAmmar, Raymond G.
dc.contributor.authorBall, S.
dc.contributor.authorBaringer, Philip S.
dc.contributor.authorBean, Alice
dc.contributor.authorBesson, David Zeke
dc.contributor.authorCoppage, Don
dc.contributor.authorCopty, N.
dc.contributor.authorDavis, Robin E. P.
dc.contributor.authorHancock, N.
dc.contributor.authorKelly, M.
dc.contributor.authorKwak, Nowhan
dc.contributor.authorLam, H.
dc.date.accessioned2007-04-13T21:12:44Z
dc.date.available2007-04-13T21:12:44Z
dc.date.issued1994-03
dc.identifier.citationCINABRO, D, HENDERSON, S, et al. Observation of D(0) → K+pi-. PHYSICAL REVIEW LETTERS. March 1994. 72(10) : 1406-1410
dc.identifier.urihttp://hdl.handle.net/1808/1438
dc.description.abstractUsing the CLEO II data sample, with an integrated luminosity of 1.8 fb-1 at and near the UPSILON(4S) resonance, we have observed a signal for D0 --> K+pi-, which could be due to either D0D0BAR mixing or doubly Cabibbo suppressed decay, or a combination of the two. We find B(D0 --> K+pi-)/B(D0 --> K- pi+)= 0.0077 +/- 0.0025 (stat) +/- 0.0025 (syst).
dc.language.isoen_US
dc.publisherAMERICAN PHYSICAL SOC
dc.relation.isversionofhttp://publish.aps.org/
dc.titleObservation of D(0) → K+pi-
dc.typeArticle
dc.rights.accessrightsopenAccess


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