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dc.contributor.authorAmmar, Raymond G.
dc.contributor.authorBean, Alice
dc.contributor.authorBesson, David Zeke
dc.contributor.authorZhao, X.
dc.date.accessioned2007-04-09T23:45:50Z
dc.date.available2007-04-09T23:45:50Z
dc.date.issued2001-12
dc.identifier.citationChen, S, Hinson, JW, et al. Branching fraction and photon energy spectrum for b -> s gamma. PHYSICAL REVIEW LETTERS. December 2001. 87(25)
dc.identifier.otherhttp://publish.aps.org/
dc.identifier.urihttp://hdl.handle.net/1808/1321
dc.description.abstractWe have measured the branching fraction and photon energy spectrum for the radiative penguin process b --> s gamma. We find B(b --> s gamma) = (3.21 +/- 0.43 +/- 0.27(-0.10)(+0.18)) x 10(-4), where the errors are statistical, systematic, and from theory corrections. We obtain first and second moments of the photon energy spectrum above 2.0 GeV, (E gamma) = 2.346 +/- 0.032 +/- 0.011 GeV, and (E-gamma(2)) - (E-gamma)(2) = 0.0226 +/- 0.0066 +/- 0.0020 GeV2, where the errors are statistical and systematic. From the first moment, we obtain (in the modified minimal subtraction renormalization scheme, to order 1/M-B(3) and beta (o)alpha (2)(s)) the heavy quark effective theory parameter <(<Lambda>)over bar> = 0.35 +/- 0.08 +/- 0.10 GeV.
dc.language.isoen_US
dc.publisherAMERICAN PHYSICAL SOC
dc.titleBranching fraction and photon energy spectrum for b -> s gamma
dc.typeArticle
dc.rights.accessrightsopenAccess


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