Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/57806
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dc.contributor.authorGuo, X.H.-
dc.contributor.authorLeitner, O.-
dc.contributor.authorThomas, A.-
dc.contributor.editorNieves, J.F.-
dc.contributor.editorVolkas, R.R.-
dc.date.issued2003-
dc.identifier.citationAIP Conference Proceedings, 2003 / Nieves, J.F., Volkas, R.R. (ed./s), vol.689, pp.126-136-
dc.identifier.isbn0-7354-0160-8-
dc.identifier.issn1931-3063-
dc.identifier.urihttp://hdl.handle.net/2440/57806-
dc.descriptionNeutrinos, Flavor Physics, and Precision Cosmology: Fourth Tropical Workshop on Particle Physics and Cosmology, 9-13 June 2003, Cairns, Queensland (AUSTRALIA) / José F. Nieves and Raymond R. Volkas (eds.) isbn: 0735401608-
dc.description.abstractBased on the QCD factorization approach we analyse the branching ratios for the channel $B \to \rho \pi$. From the comparisons with experimental data provided by CLEO, BELLE and BABAR we constrain the form factor $F^{B \to \pi}(m_{\rho}^{2})$ and propose boundaries for this form factor depending on the CKM matrix element parameters $\rho$ and $\eta$.-
dc.description.statementofresponsibilityX.-H. Guo, O.M.A. Leitner and A.W. Thomas-
dc.language.isoen-
dc.publisherAmerican Institute of Physics-
dc.relation.ispartofseriesAIP Conference Proceedings-
dc.rights© 2003 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics.-
dc.source.urihttp://link.aip.org/link/?APCPCS/689/126/1-
dc.titleQCD factorization in B decays into ρπ-
dc.title.alternativeQCD factorization in B decays into rhoPi-
dc.typeConference paper-
dc.contributor.conference4th Tropical Workshop on Particle Physics and Cosmology (9 Jun 2003 - 13 Jun 2003 : CAIRNS, AUSTRALIA)-
dc.identifier.doi10.1063/1.1627732-
pubs.publication-statusPublished-
dc.identifier.orcidThomas, A. [0000-0003-0026-499X]-
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Chemistry and Physics publications

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