Amplitude analysis and the nature of the $Z_c$(3900)
dc.contributor.author | Pilloni, A. | |
dc.contributor.author | Fernandez-Ramirez, C. | |
dc.contributor.author | Jackura, A. | |
dc.contributor.author | Mathieu, Vincent | |
dc.contributor.author | Mikhasenko, M. | |
dc.contributor.author | Nys, J. | |
dc.contributor.author | Szczepaniak, Adam P | |
dc.date.accessioned | 2025-02-20T16:42:27Z | |
dc.date.available | 2025-02-20T16:42:27Z | |
dc.date.issued | 2017-06-21 | |
dc.description.abstract | The 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.citation | Pilloni, 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.issn | 1873-2445 | |
dc.identifier.other | BRITE 1384 | |
dc.identifier.uri | https://hdl.handle.net/2022/31954 | |
dc.language.iso | en | |
dc.relation.isversionof | https://doi.org/10.1016/j.physletb.2017.06.030 | |
dc.relation.journal | Phys. Lett. | |
dc.title | Amplitude analysis and the nature of the $Z_c$(3900) |
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