The Y(4260) as an omega chi_{c1} molecular state

dc.creatorYuan, C. Z.
dc.creatorWang, P.
dc.creatorMo, X. H.
dc.date2005-11-09
dc.date2006-02-22
dc.date.accessioned2026-07-07T10:29:47Z
dc.date.available2026-07-07T10:29:47Z
dc.descriptionIt is suggested that the newly observed Y(4260) by BARBAR collaboration is a molecular state composed of an omega and a chi_{c1}. Both the production and decay properties are discussed. A consequence for this molecular state, Y(4260), is that it decays into pi+pi-pi0 chi_{c1} with similar rate to pi+ pi- J/psi. It is also expected that Y(4260) -> pi0 pi0 J/psi is produced at half rate as Y(4260) ->pi+ pi- J/psi. These decay modes should be searched for in the B factories using initial state radiative return data and B decay data as well.
dc.description5 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0511107
dc.identifierhttp://arxiv.org/abs/hep-ph/0511107
dc.identifierPhys.Lett.B634:399-402,2006
dc.identifierdoi:10.1016/j.physletb.2006.01.031
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177929
dc.subjectHigh Energy Physics - Phenomenology
dc.titleThe Y(4260) as an omega chi_{c1} molecular state
dc.typetext

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