Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/5397
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dc.contributorDepartment of Applied Physics-
dc.creatorO'Donnell, PJ-
dc.creatorXu, QP-
dc.creatorTung, HKK-
dc.date.accessioned2014-12-11T08:25:42Z-
dc.date.available2014-12-11T08:25:42Z-
dc.identifier.issn1550-7998-
dc.identifier.urihttp://hdl.handle.net/10397/5397-
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.rightsPhysical Review D © 1995 The American Physical Society. The Journal's web site is located at http://prd.aps.org/en_US
dc.subjectB mesonsen_US
dc.subjectForm factors (elementary particles)en_US
dc.subjectMeson decayen_US
dc.subjectQuark massen_US
dc.subjectQuark modelsen_US
dc.subjectScaling phenomenaen_US
dc.subjectSemileptonic decaysen_US
dc.subjectWeak particle decayen_US
dc.titleWeak decays in the light-front quark modelen_US
dc.typeJournal/Magazine Articleen_US
dc.identifier.spage3966-
dc.identifier.epage3977-
dc.identifier.volume52-
dc.identifier.issue7-
dc.identifier.doi10.1103/PhysRevD.52.3966-
dcterms.abstractWe study the form factors of heavy-to-heavy and heavy-to-light weak decays using the light-front relativistic quark model. For the heavy-to-heavy B→D(*) semileptonic decays we calculate the corresponding Isgur-Wise function for the while kinematic region. For the heavy-to-light B→P and B→V semileptonic decays we calculate the form factors at q²=0; in particular, we have derived the dependence of the form factors on the b-quark mass in the mb→∞ limit. This dependence cannot be produced by extrapolating the scaling behavior of the form factors at q[sub max]² using the single-pole assumption. This shows that the q² dependence of the form factors in regions far away from the zero recoil could be much more complicated than that predicted by the single-pole assumption.-
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitationPhysical review. D, Particles, fields, gravitation, and cosmology, Oct. 1995, v. 52, no. 7, p. 3966-3977-
dcterms.isPartOfPhysical review. D, Particles, fields, gravitation, and cosmology-
dcterms.issued1995-10-01-
dc.identifier.isiWOS:A1995TL18200025-
dc.identifier.scopus2-s2.0-33751084401-
dc.identifier.eissn1550-2368-
dc.description.oaVersion of Recorden_US
dc.identifier.FolderNumberOA_IR/PIRAen_US
dc.description.pubStatusPublisheden_US
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