Amplitude analysis and the nature of the $Z_c$(3900)

dc.contributor.authorPilloni, A.
dc.contributor.authorFernandez-Ramirez, C.
dc.contributor.authorJackura, A.
dc.contributor.authorMathieu, Vincent
dc.contributor.authorMikhasenko, M.
dc.contributor.authorNys, J.
dc.contributor.authorSzczepaniak, Adam P
dc.date.accessioned2025-02-20T16:42:27Z
dc.date.available2025-02-20T16:42:27Z
dc.date.issued2017-06-21
dc.description.abstractThe microscopic nature of the XYZ states remains an unsettled topic. We show how a thorough amplitude analysis of the data can help constraining models of these states. Specifically, we consider the case of the $Z_c$(3900) peak and discuss possible scenarios of a QCD state, virtual state, or a kinematical enhancement. We conclude that current data are not precise enough to distinguish between these hypotheses, however, the method we propose, when applied to the forthcoming high-statistics measurements should shed light on the nature of these exotic enhancements.
dc.identifier.citationPilloni, A., et al. "Amplitude analysis and the nature of the $Z_c$(3900)." Phys. Lett., vol. B772, pp. 200-209, 2017-6-21, https://doi.org/10.1016/j.physletb.2017.06.030.
dc.identifier.issn1873-2445
dc.identifier.otherBRITE 1384
dc.identifier.urihttps://hdl.handle.net/2022/31954
dc.language.isoen
dc.relation.isversionofhttps://doi.org/10.1016/j.physletb.2017.06.030
dc.relation.journalPhys. Lett.
dc.titleAmplitude analysis and the nature of the $Z_c$(3900)

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