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Observation of the decay D-s(+)->omega pi(+)

dc.contributor.authorAmmar, Raymond G.
dc.contributor.authorBaringer, Philip S.
dc.contributor.authorBean, Alice
dc.contributor.authorBesson, David Zeke
dc.contributor.authorCoppage, Don
dc.contributor.authorDarling, C.
dc.contributor.authorDavis, Robin E. P.
dc.contributor.authorHancock, N.
dc.contributor.authorKotov, S.
dc.contributor.authorKravchenko, I.
dc.contributor.authorKwak, Nowhan
dc.date.accessioned2007-04-13
dc.date.available2007-04-13
dc.date.issued1997-08
dc.identifier.citationBalest, R, Behrens, BH, et al. Observation of the decay D-s(+)->omega pi(+). PHYSICAL REVIEW LETTERS. August 1997. 79(8) : 1436-1440
dc.identifier.otherhttp://publish.aps.org/
dc.identifier.urihttp://hdl.handle.net/1808/1391
dc.description.abstractUsing e(+)e(-) annihilation data collected by the CLEO II detector at CESR, we have observed the decay D-s(+)-->omega pi(+). This final state may be produced through the annihilation decay df the D-s(+), or through final state interactions. We find a branching ratio of Gamma(D-s(+)-->omega pi(+))/Gamma(D-s(+)-->eta pi(+)) = 0.16+/-0.04+/-0.03, where the first error is statistical and the second is systematic.
dc.language.isoen_US
dc.publisherAMERICAN PHYSICAL SOC
dc.titleObservation of the decay D-s(+)->omega pi(+)
dc.typeArticle
dc.rights.accessrightsopenAccess


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