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dc.contributor.authorFerretti, J.
dc.contributor.authorSantopinto, E.
dc.contributor.authorAnwar, M. Naeem
dc.contributor.authorLu, Yu
dc.date.accessioned2020-05-27T11:40:01Z
dc.date.available2020-05-27T11:40:01Z
dc.date.issued2020
dc.identifier.citationFerretti, J., Santopinto, E., Anwar, M. N., & Lu, Y. (2020). Quark structure of the χc(3P) and X(4274) resonances and their strong and radiative decays. <i>European Physical Journal C</i>, <i>80</i>(5), Article 464. <a href="https://doi.org/10.1140/epjc/s10052-020-8032-5" target="_blank">https://doi.org/10.1140/epjc/s10052-020-8032-5</a>
dc.identifier.otherCONVID_35732647
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/69267
dc.description.abstractWe calculate the masses of χc(3P) states with threshold corrections in a coupled-channel model. The model was recently applied to the description of the properties of χc(2P) and χb(3P) multiplets (Ferretti and Santopinto in Phys Lett B 789:550, 2019]. We also compute the open-charm strong decay widths of the χc(3P) states and their radiative transitions. According to our predictions, the χc(3P) states should be dominated by the charmonium core, but they may also show small meson-meson components. The X(4274) is interpreted as a cc¯ χc1(3P) state. More information on the other members of the χc(3P) multiplet, as well as a more rigorous analysis of the X(4274)’s decay modes, are needed to provide further indications on the quark structure of the previous resonance.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherSpringer
dc.relation.ispartofseriesEuropean Physical Journal C
dc.rightsCC BY 4.0
dc.subject.othertheoretical physics
dc.titleQuark structure of the χc(3P) and X(4274) resonances and their strong and radiative decays
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202005273520
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn1434-6044
dc.relation.numberinseries5
dc.relation.volume80
dc.type.versionpublishedVersion
dc.rights.copyright© 2020 the Authors
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber320062
dc.subject.ysohiukkasfysiikka
dc.subject.ysoydinfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1140/epjc/s10052-020-8032-5
dc.relation.funderResearch Council of Finlanden
dc.relation.funderSuomen Akatemiafi
jyx.fundingprogramResearch costs of Academy Research Fellow, AoFen
jyx.fundingprogramAkatemiatutkijan tutkimuskulut, SAfi
jyx.fundinginformationJ. Ferretti acknowledges financial support from the US Department of Energy, Grant No. DE-FG-02-91ER-40608, and the Academy of Finland, Project no. 320062. Y. Lu and M. Naeem Anwar are supported by the DFG (Grant no. TRR110) and the NSFC (Grant no. 11621131001) through the funds provided to the Sino-German CRC 110 “Symmetries and the Emergence of Structure in QCD”. M. N. Anwar acknowledges partial support from the Munich Institute for Astro- and Particle Physics (MIAPP) which is funded by the DFG under Germany’s Excellence Strategy−EXC-2094−390783311.
dc.type.okmA1


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