Abstract
Using a data sample of 921.9 fb-1 collected with the Belle detector, we study the process of e+e-→Ds+Ds1(2536)-+c.c. via initial-state radiation. We report the first observation of a vector charmoniumlike state decaying to Ds+Ds1(2536)-+c.c. with a significance of 5.9σ, including systematic uncertainties. The measured mass and width are (4625.9-6.0+6.2(stat)±0.4(syst)) MeV/c2 and (49.8-11.5+13.9(stat)±4.0(syst)) MeV, respectively. The product of the e+e-→Ds+Ds1(2536)-+c.c. cross section and the branching fraction of Ds1(2536)-→D∗0K-is measured from the DsDs1(2536) threshold to 5.59 GeV.
Original language | English |
---|---|
Article number | 111103 |
Journal | Physical Review D |
Volume | 100 |
Issue number | 11 |
DOIs | |
Publication status | Published - 2019 Dec 31 |
ASJC Scopus subject areas
- Nuclear and High Energy Physics
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In: Physical Review D, Vol. 100, No. 11, 111103, 31.12.2019.
Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - Observation of a vector charmoniumlike state in e+e-→ Ds+ Ds1 (2536)-+ c. c.
AU - Jia, S.
AU - Shen, C. P.
AU - Yuan, C. Z.
AU - Wang, X. L.
AU - Adachi, I.
AU - Aihara, H.
AU - Asner, D. M.
AU - Atmacan, H.
AU - Aulchenko, V.
AU - Ayad, R.
AU - Babu, V.
AU - Badhrees, I.
AU - Bakich, A. M.
AU - Behera, P.
AU - Bhuyan, B.
AU - Bilka, T.
AU - Biswal, J.
AU - Bobrov, A.
AU - Bonvicini, G.
AU - Bozek, A.
AU - Bračko, M.
AU - Browder, T. E.
AU - Campajola, M.
AU - Cao, L.
AU - Červenkov, D.
AU - Chang, P.
AU - Chen, A.
AU - Cheon, B. G.
AU - Chilikin, K.
AU - Cho, H. E.
AU - Cho, K.
AU - Choi, S. K.
AU - Choi, Y.
AU - Cinabro, D.
AU - Cunliffe, S.
AU - De Nardo, G.
AU - Di Capua, F.
AU - Di Carlo, S.
AU - DoleŽal, Z.
AU - Dong, T. V.
AU - Eidelman, S.
AU - Epifanov, D.
AU - Fast, J. E.
AU - Ferber, T.
AU - Fulsom, B. G.
AU - Garg, R.
AU - Gaur, V.
AU - Gabyshev, N.
AU - Garmash, A.
AU - Giri, A.
AU - Goldenzweig, P.
AU - Golob, B.
AU - Hayasaka, K.
AU - Hayashii, H.
AU - Hou, W. S.
AU - Hsu, C. L.
AU - Iijima, T.
AU - Inami, K.
AU - Inguglia, G.
AU - Ishikawa, A.
AU - Itoh, R.
AU - Iwasaki, M.
AU - Iwasaki, Y.
AU - Jacobs, W. W.
AU - Jin, Y.
AU - Joo, K. K.
AU - Kang, K. H.
AU - Karyan, G.
AU - Kichimi, H.
AU - Kim, B. H.
AU - Kim, C. H.
AU - Kim, D. Y.
AU - Kim, S. H.
AU - Kinoshita, K.
AU - Kodyš, P.
AU - Korpar, S.
AU - Kroeger, R.
AU - Krokovny, P.
AU - Kulasiri, R.
AU - Kuzmin, A.
AU - Kwon, Y. J.
AU - Lalwani, K.
AU - Lange, J. S.
AU - Lee, I. S.
AU - Lee, S. C.
AU - Lewis, P.
AU - Li, C. H.
AU - Li, L. K.
AU - Li, Y. B.
AU - Li Gioi, L.
AU - Libby, J.
AU - Lieret, K.
AU - Liventsev, D.
AU - MacQueen, C.
AU - Masuda, M.
AU - Matsuda, T.
AU - Matvienko, D.
AU - Merola, M.
AU - Miyabayashi, K.
AU - Miyata, H.
AU - Mizuk, R.
AU - Mussa, R.
AU - Nath, K. J.
AU - Nayak, M.
AU - Niiyama, M.
AU - Nisar, N. K.
AU - Nishida, S.
AU - Nishimura, K.
AU - Ogawa, S.
AU - Ono, H.
AU - Onuki, Y.
AU - Oskin, P.
AU - Pakhlov, P.
AU - Pakhlova, G.
AU - Pang, T.
AU - Pardi, S.
AU - Park, H.
AU - Park, S. H.
AU - Patra, S.
AU - Paul, S.
AU - Pedlar, T. K.
AU - Pestotnik, R.
AU - Piilonen, L. E.
AU - Popov, V.
AU - Prencipe, E.
AU - Prim, M. T.
AU - Röhrken, M.
AU - Rostomyan, A.
AU - Rout, N.
AU - Russo, G.
AU - Sahoo, D.
AU - Sakai, Y.
AU - Sandilya, S.
AU - Santelj, L.
AU - Savinov, V.
AU - Schneider, O.
AU - Schnell, G.
AU - Schwanda, C.
AU - Seino, Y.
AU - Senyo, K.
AU - Sevior, M. E.
AU - Shiu, J. G.
AU - Shwartz, B.
AU - Sokolov, A.
AU - Solovieva, E.
AU - Stanič, S.
AU - Starič, M.
AU - Stottler, Z. S.
AU - Sumiyoshi, T.
AU - Sutcliffe, W.
AU - Takizawa, M.
AU - Tanida, K.
AU - Tenchini, F.
AU - Trabelsi, K.
AU - Uchida, M.
AU - Uglov, T.
AU - Unno, Y.
AU - Uno, S.
AU - Usov, Y.
AU - Van Tonder, R.
AU - Varner, G.
AU - Vinokurova, A.
AU - Vorobyev, V.
AU - Wang, C. H.
AU - Wang, M. Z.
AU - Watanabe, M.
AU - Won, E.
AU - Yang, S. B.
AU - Ye, H.
AU - Yin, J. H.
AU - Zhang, Z. P.
AU - Zhilich, V.
AU - Zhukova, V.
AU - Zhulanov, V.
N1 - Funding Information: We thank the KEKB group for the excellent operation of the accelerator; the KEK cryogenics group for the efficient operation of the solenoid; and the KEK computer group, and the Pacific Northwest National Laboratory (PNNL) Environmental Molecular Sciences Laboratory (EMSL) computing group for strong computing support; and the National Institute of Informatics, and Science Information NETwork 5 (SINET5) for valuable network support. We acknowledge support from the Ministry of Education, Culture, Sports, Science, and Technology (MEXT) of Japan, the Japan Society for the Promotion of Science (JSPS), and the Tau-Lepton Physics Research Center of Nagoya University; the Australian Research Council including Grants No. DP180102629, No. DP170102389, No. DP170102204, No. DP150103061, and No. FT130100303; Austrian Science Fund (FWF); the National Natural Science Foundation of China under Contracts No. 11435013, No. 11475187, No. 11521505, No. 11575017, No. 11675166, No. 11705209, No. 11761141009, No. 11975076; Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS), Grant No. QYZDJ-SSW-SLH011; the CAS Center for Excellence in Particle Physics (CCEPP); the Shanghai Pujiang Program under Grant No. 18PJ1401000; the Ministry of Education, Youth and Sports of the Czech Republic under Contract No. LTT17020; the Carl Zeiss Foundation, the Deutsche Forschungsgemeinschaft, the Excellence Cluster Universe, and the VolkswagenStiftung; the Department of Science and Technology of India; the Istituto Nazionale di Fisica Nucleare of Italy; National Research Foundation (NRF) of Korea Grants No. 2016R1-D1A1B-01010135, No. 2016R1-D1A1B-02012900, No. 2018R1-A2B-3003643, No. 2018R1-A6A1A-06024970, No. 2018R1-D1A1B-07047294, No. 2019K1-A3A7A-09033840, and No. 2019R1-I1A3A-01058933; Radiation Science Research Institute, Foreign Large-size Research Facility Application Supporting project, the Global Science Experimental Data Hub Center of the Korea Institute of Science and Technology Information and KREONET/GLORIAD; the Polish Ministry of Science and Higher Education and the National Science Center; the Ministry of Science and Higher Education of the Russian Federation, Agreement 14.W03.31.0026; from 15.02.2018; the Slovenian Research Agency; Ikerbasque, Basque Foundation for Science, Spain; the Swiss National Science Foundation; the Ministry of Education and the Ministry of Science and Technology of Taiwan; and the United States Department of Energy and the National Science Foundation. Publisher Copyright: © 2019 authors. Published by the American Physical Society.
PY - 2019/12/31
Y1 - 2019/12/31
N2 - Using a data sample of 921.9 fb-1 collected with the Belle detector, we study the process of e+e-→Ds+Ds1(2536)-+c.c. via initial-state radiation. We report the first observation of a vector charmoniumlike state decaying to Ds+Ds1(2536)-+c.c. with a significance of 5.9σ, including systematic uncertainties. The measured mass and width are (4625.9-6.0+6.2(stat)±0.4(syst)) MeV/c2 and (49.8-11.5+13.9(stat)±4.0(syst)) MeV, respectively. The product of the e+e-→Ds+Ds1(2536)-+c.c. cross section and the branching fraction of Ds1(2536)-→D∗0K-is measured from the DsDs1(2536) threshold to 5.59 GeV.
AB - Using a data sample of 921.9 fb-1 collected with the Belle detector, we study the process of e+e-→Ds+Ds1(2536)-+c.c. via initial-state radiation. We report the first observation of a vector charmoniumlike state decaying to Ds+Ds1(2536)-+c.c. with a significance of 5.9σ, including systematic uncertainties. The measured mass and width are (4625.9-6.0+6.2(stat)±0.4(syst)) MeV/c2 and (49.8-11.5+13.9(stat)±4.0(syst)) MeV, respectively. The product of the e+e-→Ds+Ds1(2536)-+c.c. cross section and the branching fraction of Ds1(2536)-→D∗0K-is measured from the DsDs1(2536) threshold to 5.59 GeV.
UR - http://www.scopus.com/inward/record.url?scp=85077912813&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.100.111103
DO - 10.1103/PhysRevD.100.111103
M3 - Article
AN - SCOPUS:85077912813
SN - 2470-0010
VL - 100
JO - Physical Review D
JF - Physical Review D
IS - 11
M1 - 111103
ER -