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dc.contributor.authorGamermann, Daniel-
dc.contributor.authorOset, Eulogi-
dc.contributor.authorZou, B. S.-
dc.date.accessioned2009-08-10T09:53:26Z-
dc.date.available2009-08-10T09:53:26Z-
dc.date.issued2009-04-30-
dc.identifier.citationEur.Phys.J.A41:85-91,2009en_US
dc.identifier.issn1434-6001-
dc.identifier.urihttp://hdl.handle.net/10261/15864-
dc.description5 pages, 1 figure.-- ISI article identifier:000267299600009.-- ArXiv pre-print avaible at:http://arxiv.org/abs/0805.0499en_US
dc.description.abstractWe calculate the radiative decay width of the psi(3770) into the dynamically generated scalar resonance X(3700) which is predicted in a previous paper. The results show that it is possible that the upgraded BEPC-II facility will generate enough statistics in order to observe this decay and thus confirm the existence of the X(3700).en_US
dc.format.extent149401 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoengen_US
dc.publisherSpringeren_US
dc.rightsopenAccessen_US
dc.titleThe radiative decay of psi(3770) into the predicted scalar state X(3700)en_US
dc.typeartículoen_US
dc.identifier.doi10.1140/epja/i2009-10767-8-
dc.description.peerreviewedPeer revieweden_US
dc.relation.publisherversionhttp://dx.doi.org/10.1140/epja/i2009-10767-8en_US
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