Study of the decay D+ ? K*(892)+ KS0 in D+ ? K+KS0?0

Basit Öğe Kaydı
dc.authoridLavezzi, Lia/0000-0002-4928-8151|Messchendorp, Johan/0000-0001-6649-0549|Janchiv, Shinebayar/0000-0003-1207-3322|Chen, Qi/0000-0002-6568-7267|Yuncu, Alperen/0000-0001-9696-9331|wang, qi/0000-0002-2794-6897|Mangoni, Alessio/0000-0002-4786-6632|Pathak, Atanu/0000-0001-9861-2942|Zhemchugov, Alexey/0000-0002-3360-4965|Wu, Xin/0000-0001-7655-389X|Wang, Yue/0000-0001-8673-6358|Kolcu, Onur Bugra/0000-0002-9177-1286|Liu, Zhiyu/0000-0001-8351-1268|Gradl, Wolfgang/0000-0002-9974-8320|Li, Kun/0000-0002-3638-2974|Liu, Liang/0000-0002-6753-925X|Han, Jian/0000-0002-0647-4050|Farineli, Riccardo/0000-0002-7972-9093|Song, Weimin/0000-0003-1376-2293|Wang, Yunwen/0009-0008-3083-7799|Calligaris, Luigi/0000-0002-9951-9448|Fan, xiao/0000-0001-5147-6701|Zhang, Jiawei/0000-0001-9635-154X|Spataro, Stefano/0000-0001-9601-405X|Sheng, Jin-Huan/0000-0002-2655-6301|Muramatsu, Hajime/0000-0003-0305-4461|Xie, Xinhai/0000-0003-3530-6483|Lane, Jake/0000-0002-5816-9488|Aliberti, Riccardo/0000-0003-3500-4012
dc.authorwosidZhang, Li/GWM-7501-2022
dc.authorwosidZhu, Jie/JAC-4621-2023
dc.authorwosidyang, liu/JXX-5043-2024
dc.authorwosidMa, Mingyang/JXM-3330-2024
dc.authorwosidzhang, bx/HNR-3314-2023
dc.authorwosidLing, Li/JYO-7043-2024
dc.authorwosidWu, Lijuan/JJG-0701-2023
dc.contributor.authorAblikim, M.
dc.contributor.authorAchasov, M. N.
dc.contributor.authorAdlarson, P.
dc.contributor.authorAhmed, S.
dc.contributor.authorAlbrecht, M.
dc.contributor.authorAliberti, R.
dc.contributor.authorÇetin, Serkant Ali
dc.date.accessioned2024-07-18T20:47:07Z
dc.date.available2024-07-18T20:47:07Z
dc.date.issued2021
dc.departmentFakülteler, Mühendislik ve Doğa Bilimleri Fakültesi, Enerji Sistemleri Mühendisliği Bölümüen_US
dc.description.abstractBased on an e(+)e(-) collision data sample corresponding to an integrated luminosity of 2.93 fb(-1) collected with the BESIII detector at root s = 3.773 GeV, the first amplitude analysis of the singly Cabibbo-suppressed decay D+ -> (K+KS0)pi(0) is performed. From the amplitude analysis, the K* (892)(+) K-S(0) component is found to be dominant with a fraction of (57.1 +/- 2.6 +/- 4.2)%, where the first uncertainty is statistical and the second systematic. In combination with the absolute branching fraction B(D+ -> K+ K-S(0)pi(0)) measured by BESIII, we obtain B(D+ -> K* (892)+K-S(0)) = (8.69 +/- 0.40 +/- 0.64 +/- 0.51) x 10(-3), where the third uncertainty is due to the branching fraction B(D+ -> (K+KS0)pi(0)). The precision of this result is significantly improved compared to the previous measurement. This result also differs from most of theoretical predictions by about 4 sigma, which may help to improve the understanding of the dynamics behind.en_US
dc.description.sponsorshipNational Key Research and Development Program of China [2020YFA0406400, 2020YFA0406300]; National Natural Science Foundation of China (NSFC) [11605124, 11625523, 11635010, 11735014, 11822506, 11835012, 11935015, 11935016, 11935018, 11961141012, 12022510, 12035013, 12061131003, U1732263, U1832207, U1932101, U1932108]; Chinese Academy of Sciences (CAS) Large-Scale Scientific Facility Program; CAS [U1732263, U1832207, U1932101, U1932108]; CAS Key Research Program of Frontier Sciences [QYZDJ-SSW-SLH040]; 100 Talents Program of CAS; Fundamental Research Funds for the Central Universities; INPAC; Shanghai Key Laboratory for Particle Physics and Cosmology; ERC [758462]; European Union Horizon 2020 research and innovation programme under Marie Sklodowska-Curie Grant [894790]; German Research Foundation DFG [443159800, CRC 1044, FOR 2359, GRK 214]; Istituto Nazionale di Fisica Nucleare, Italy; Ministry of Development of Turkey [DPT2006K-120470]; National Science and Technology fund; Olle Engkvist Foundation [200-0605]; STFC (United Kingdom); Knut and Alice Wallenberg Foundation (Sweden) [2016.0157]; Royal Society, United Kingdom [DH140054, DH160214]; Swedish Research Council; U.S. Department of Energy [DE-FG0205ER41374, DE-SC-0012069]en_US
dc.description.sponsorshipThe BESIII Collaboration thanks the staff of BEPCII and the IHEP computing center for their strong support. This work was supported in part by National Key Research and Development Program of China under Contracts No. 2020YFA0406400 and No. 2020YFA0406300; National Natural Science Foundation of China (NSFC) under Contracts No. 11605124, No. 11625523, No. 11635010, No. 11735014, No. 11822506, No. 11835012, No. 11935015, No. 11935016, No. 11935018, No. 11961141012, No. 12022510, No. 12035013, and No. 12061131003; the Chinese Academy of Sciences (CAS) Large-Scale Scientific Facility Program; Joint Large-Scale Scientific Facility Funds of the NSFC and CAS under Contracts No. U1732263, No. U1832207, No. U1932101, and No. U1932108; CAS Key Research Program of Frontier Sciences under Contract No. QYZDJ-SSW-SLH040; 100 Talents Program of CAS; Fundamental Research Funds for the Central Universities; INPAC and Shanghai Key Laboratory for Particle Physics andCosmology; ERCunder Contract No. 758462; European Union Horizon 2020 research and innovation programme under Marie Sklodowska-Curie Grant No. 894790; German Research Foundation DFG under Contract No. 443159800, Collaborative Research Center CRC 1044, FOR 2359, GRK 214; Istituto Nazionale di Fisica Nucleare, Italy; Ministry of Development of Turkey under Contract No. DPT2006K-120470; National Science and Technology fund; Olle Engkvist Foundation under Contract No. 200-0605; STFC (United Kingdom); The Knut and Alice Wallenberg Foundation (Sweden) under Contract No. 2016.0157; The Royal Society, United Kingdom under Contracts No. DH140054 and No. DH160214; The Swedish Research Council; U.S. Department of Energy under Contracts No. DE-FG0205ER41374 and No. DE-SC-0012069.en_US
dc.identifier.doi10.1103/PhysRevD.104.012006
dc.identifier.issn2470-0010
dc.identifier.issn2470-0029
dc.identifier.issue1en_US
dc.identifier.scopus2-s2.0-85110297164en_US
dc.identifier.scopusqualityQ1en_US
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.104.012006
dc.identifier.urihttps://hdl.handle.net/11411/7675
dc.identifier.volume104en_US
dc.identifier.wosWOS:000674571000001en_US
dc.identifier.wosqualityQ1en_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
dc.institutionauthorÇetin, Serkant Ali
dc.language.isoenen_US
dc.publisherAmer Physical Socen_US
dc.relation.ispartofPhysical Review Den_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.titleStudy of the decay D+ ? K*(892)+ KS0 in D+ ? K+KS0?0
dc.typeArticle

Dosyalar

Koleksiyon

Web of Science Indexed Publications
Faculty of Engineering and Natural Sciences
Scopus Indexed Publications