Observation of the decay Ds+ ? ??+?

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dc.authoridLiu, Haibo/0000-0002-4213-2883
dc.authoridgarbolino, sara/0000-0001-5604-1395
dc.authoridZhang, Xiaofeng/0000-0003-2738-3286
dc.authoridZhang, Jiawei/0000-0001-9635-154X
dc.authoridLu, Xiankai/0000-0001-7720-6048
dc.authoridli, fangyu/0009-0009-8303-9157
dc.authoridLiu, Yilin/0000-0002-7581-3933
dc.authorwosidLiu, Yang/JVD-6777-2023
dc.authorwosidLiu, Haibo/JWP-8549-2024
dc.authorwosidSun, Peng/KDO-4243-2024
dc.authorwosidLin, Lin/JTU-1595-2023
dc.authorwosidWU, YANAN/JPK-7386-2023
dc.authorwosidMA, MANMAN/GZL-5038-2022
dc.authorwosidpeng, jin/JRW-4493-2023
dc.contributor.authorAblikim, M.
dc.contributor.authorAchasov, M. N.
dc.contributor.authorAdlarson, P.
dc.contributor.authorAlbrecht, M.
dc.contributor.authorAliberti, R.
dc.contributor.authorAmoroso, A.
dc.contributor.authorÇetin, Serkant Ali
dc.date.accessioned2024-05-19T14:50:46Z
dc.date.available2024-05-19T14:50:46Z
dc.date.issued2023
dc.departmentİstinye Üniversitesien_US
dc.description.abstractUsing 7.33 fb(-1) of e(+)e(-) collision data collected by the BESIII detector at c.m. energies between 4.128 GeV and 4.226 GeV, we observe for the first time the decay D-s(+/-) -> omega pi(+/-)eta with a statistical significance of 7.6 sigma. The measured branching fraction of this decay is (0.54 +/- 0.12 +/- 0.04)%, where the first uncertainty is statistical and the second is systematic.en_US
dc.description.sponsorshipNational Key R&D Program of China [2020YFA0406400, 2020YFA0406300]; National Natural Science Foundation of China (NSFC) [11635010, 11735014, 11835012, 11935015, 11935016, 11935018, 11961141012, 12022510, 12025502, 12035009, 12035013, 12192260, 12192261, 12192262, 12192263, 12192264, 12192265]; Chinese Academy of Sciences (CAS) Large-Scale Scientific Facility Program; NSFC; CAS [U1832207, U1932108]; CAS Center for Excellence in Particle Physics (CCEPP); 100 Talents Program of CAS; Institute of Nuclear and Particle Physics (INPAC); Shanghai Key Laboratory for Particle Physics and Cosmology; Suranaree University of Technology (SUT); ERC [758462]; STFC (United Kingdom); European Union [894790]; German Research Foundation DFG [443159800, 455635585]; Istituto Nazionale di Fisica Nucleare, Italy; Ministry of Development of Turkey [160355]; National Science and Technology fund; National Science Research and Innovation Fund (NSRF) via the Program Management Unit for Human Resources and Institutional Development, Research and Innovation [DH140054]; Olle Engkvist Foundation [DH160214]; Thailand Science Research and Innovation (TSRI); National Science Research and Innovation Fund (NSRF) [DE-FG02-05ER41374]; Royal Society, UK [DH140054, DH160214]; Swedish Research Council; U.S. Department of Energy [DEU1932108U1932108-FG02-05ER41374.]; [DPT2006K-120470]; [B16F640076]; [200-0605]en_US
dc.description.sponsorshipThe BESIII Collaboration thanks the staff of BEPCII and the IHEP computing center for their strong support. This work is supported in part by National Key R&D Program of China under Contracts No. 2020YFA0406400 and No. 2020YFA0406300; National Natural Science Foundation of China (NSFC) under Contracts No. 11635010, No. 11735014, No. 11835012, No. 11935015, No. 11935016, No. 11935018, No. 11961141012, No. 12022510, No. 12025502, No. 12035009, No. 12035013, No. 12192260, No. 12192261, No. 12192262, No. 12192263, No. 12192264, and No. 12192265; 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. U1832207 and No. U1932108; the CAS Center for Excellence in Particle Physics (CCEPP) ; 100 Talents Program of CAS; The Institute of Nuclear and Particle Physics (INPAC) and Shanghai Key Laboratory for Particle Physics and Cosmology; ERC under Contract No. 758462; European Union's Horizon 2020 research and innovation programme under Marie Sklodowska-Curie grant agreement under Contract No. 894790; German Research Foundation DFG under Contracts No. 443159800 and No. 455635585, Collaborative Research Center CRC 1044, FOR5327, GRK 2149; Istituto Nazionale di Fisica Nucleare, Italy; Ministry of Development of Turkey under Contract No. DPT2006K-120470; National Science and Technology fund; National Science Research and Innovation Fund (NSRF) via the Program Management Unit for Human Resources and Institutional Development, Research and Innovation under Contract No. B16F640076; Olle Engkvist Foundation under Contract No. 200-0605; STFC (United Kingdom) ; Suranaree University of Technology (SUT) , Thailand Science Research and Innovation (TSRI) , and National Science Research and Innovation Fund (NSRF) under Contract No. 160355; The Royal Society, UK under Contracts No. DH140054 and No. DH160214; The Swedish Research Council; U.S. Department of Energy under Contract No. DEU1932108U1932108-FG02-05ER41374.en_US
dc.identifier.doi10.1103/PhysRevD.107.052010
dc.identifier.issn2470-0010
dc.identifier.issn2470-0029
dc.identifier.issue5en_US
dc.identifier.scopus2-s2.0-85151320663en_US
dc.identifier.scopusqualityQ1en_US
dc.identifier.urihttps://doi.org10.1103/PhysRevD.107.052010
dc.identifier.urihttps://hdl.handle.net/20.500.12713/5803
dc.identifier.volume107en_US
dc.identifier.wosWOS:000989443400005en_US
dc.identifier.wosqualityN/Aen_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
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.snmz20240519_kaen_US
dc.subject[No Keywords]en_US
dc.titleObservation of the decay Ds+ ? ??+?en_US
dc.typeArticleen_US

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