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arxiv: 1410.6538 · v2 · submitted 2014-10-24 · ✦ hep-ex

Recognition: unknown

Study of e^+e^-toωchi_{cJ} at center-of-mass energies from 4.21 to 4.42 GeV

BESIII collaboration: M.Ablikim , M.N.Achasov , X.C.Ai , O.Albayrak , M.Albrecht , D.J.Ambrose , A.Amoroso , F.F.An
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Q.An J.Z.Bai R.Baldini Ferroli Y.Ban D.W.Bennett J.V.Bennett M.Bertani D.Bettoni J.M.Bian F.Bianchi E.Boger O.Bondarenko I.Boyko R.A.Briere H.Cai X.Cai O.Cakir A.Calcaterra G.F.Cao S.A.Cetin J.F.Chang G.Chelkov G.Chen H.S.Chen H.Y.Chen J.C.Chen M.L.Chen S.J.Chen X.Chen X.R.Chen Y.B.Chen H.P.Cheng X.K.Chu Y.P.Chu G.Cibinetto D.Cronin-Hennessy H.L.Dai J.P.Dai D.Dedovich Z.Y.Deng A.Denig I.Denysenko M.Destefanis F.De Mori Y.Ding C.Dong J.Dong L.Y.Dong M.Y.Dong S.X.Du P.F.Duan J.Z.Fan J.Fang S.S.Fang X.Fang Y.Fang L.Fava F.Feldbauer G.Felici C.Q.Feng E.Fioravanti C.D.Fu Q.Gao Y.Gao I.Garzia K.Goetzen W.X.Gong W.Gradl M.Greco M.H.Gu Y.T.Gu Y.H.Guan A.Q.Guo L.B.Guo T.Guo Y.Guo Y.P.Guo Z.Haddadi A.Hafner S.Han Y.L.Han F.A.Harris K.L.He Z.Y.He T.Held Y.K.Heng Z.L.Hou C.Hu H.M.Hu J.F.Hu T.Hu Y.Hu G.M.Huang G.S.Huang H.P.Huang J.S.Huang X.T.Huang Y.Huang T.Hussain Q.Ji Q.P.Ji X.B.Ji X.L.Ji L.L.Jiang L.W.Jiang X.S.Jiang J.B.Jiao Z.Jiao D.P.Jin S.Jin T.Johansson A.Julin N.Kalantar-Nayestanaki X.L.Kang X.S.Kang M.Kavatsyuk B.C.Ke R.Kliemt B.Kloss O.B.Kolcu B.Kopf M.Kornicer W.Kuehn A.Kupsc W.Lai J.S.Lange M.Lara P.Larin Cheng Li C.H.Li D.M.Li F.Li G.Li H.B.Li J.C.LI Jin Li K.Li P.R.Li T.Li W.D.Li W.G.Li X.L.Li X.M.Li X.N.Li X.Q.Li Z.B.Li H.Liang Y.F.Liang Y.T.Liang G.R.Liao D.X.Lin B.J.Liu C.L.Liu C.X.Liu F.H.Liu Fang Liu Feng Liu H.B.Liu H.H.Liu H.M.Liu J.Liu J.P.Liu J.Y.Liu K.Liu K.Y.Liu L.D.Liu Q.Liu S.B.Liu X.Liu X.X.Liu Y.B.Liu Z.A.Liu Zhiqiang Liu Zhiqing Liu H.Loehner X.C.Lou H.J.Lu J.G.Lu R.Q.Lu Y.LU Y.P.Lu C.L.Luo M.X.Luo T.Luo X.L.Luo M.Lv X.R.Lyu F.C.Ma H.L.Ma L.L.Ma Q.M.Ma S.Ma T.Ma X.N.Ma X.Y.Ma F.E.Maas M.Maggiora Q.A.Malik Y.J.Mao Z.P.Mao S.Marcello J.G.Messchendorp J.Min T.J.Min R.E.Mitchell X.H.Mo Y.J.Mo H.Moeini C.Morales Morales K.Moriya N.Yu.Muchnoi H.Muramatsu Y.Nefedov F.Nerling I.B.Nikolaev Z.Ning S.Nisar S.L.Niu X.Y.Niu S.L.Olsen Q.Ouyang S.Pacetti P.Patteri M.Pelizaeus H.P.Peng K.Peters J.L.Ping R.G.Ping R.Poling Y.N.Pu M.Qi S.Qian C.F.Qiao L.Q.Qin N.Qin X.S.Qin Y.Qin Z.H.Qin J.F.Qiu K.H.Rashid C.F.Redmer H.L.Ren M.Ripka G.Rong X.D.Ruan V.Santoro A.Sarantsev M.Savri\'e K.Schoenning S.Schumann W.Shan M.Shao C.P.Shen P.X.Shen X.Y.Shen H.Y.Sheng M.R.Shepherd W.M.Song X.Y.Song S.Sosio S.Spataro B.Spruck G.X.Sun J.F.Sun S.S.Sun Y.J.Sun Y.Z.Sun Z.J.Sun Z.T.Sun C.J.Tang X.Tang I.Tapan E.H.Thorndike M.Tiemens D.Toth M.Ullrich I.Uman G.S.Varner B.Wang B.L.Wang D.Wang D.Y.Wang K.Wang L.L.Wang L.S.Wang M.Wang P.Wang P.L.Wang Q.J.Wang S.G.Wang W.Wang X.F.Wang Y.D.Wang Y.F.Wang Y.Q.Wang Z.Wang Z.G.Wang Z.H.Wang Z.Y.Wang D.H.Wei J.B.Wei P.Weidenkaff S.P.Wen U.Wiedner M.Wolke L.H.Wu Z.Wu L.G.Xia Y.Xia D.Xiao Z.J.Xiao Y.G.Xie Q.L.Xiu G.F.Xu L.Xu Q.J.Xu Q.N.Xu X.P.Xu L.Yan W.B.Yan W.C.Yan Y.H.Yan H.X.Yang L.Yang Y.Yang Y.X.Yang H.Ye M.Ye M.H.Ye J.H.Yin B.X.Yu C.X.Yu H.W.Yu J.S.Yu C.Z.Yuan W.L.Yuan Y.Yuan A.Yuncu A.A.Zafar A.Zallo Y.Zeng B.X.Zhang B.Y.Zhang C.Zhang C.C.Zhang D.H.Zhang H.H.Zhang H.Y.Zhang J.J.Zhang J.L.Zhang J.Q.Zhang J.W.Zhang J.Y.Zhang J.Z.Zhang K.Zhang L.Zhang S.H.Zhang X.J.Zhang X.Y.Zhang Y.Zhang Y.H.Zhang Z.H.Zhang Z.P.Zhang Z.Y.Zhang G.Zhao J.W.Zhao J.Y.Zhao J.Z.Zhao Lei Zhao Ling Zhao M.G.Zhao Q.Zhao Q.W.Zhao S.J.Zhao T.C.Zhao Y.B.Zhao Z.G.Zhao A.Zhemchugov B.Zheng J.P.Zheng W.J.Zheng Y.H.Zheng B.Zhong L.Zhou Li Zhou X.Zhou X.K.Zhou X.R.Zhou X.Y.Zhou K.Zhu K.J.Zhu S.Zhu X.L.Zhu Y.C.Zhu Y.S.Zhu Z.A.Zhu J.Zhuang B.S.Zou J.H.Zou
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classification ✦ hep-ex
keywords omegacenter-of-masscrossenergiessignalsfirstobservedresonance
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Based on data samples collected with the BESIII detector at the BEPCII collider at 9 center-of-mass energies from 4.21 to 4.42 GeV, we search for the production of $e^+e^-\to \omega\chi_{cJ}$ ($J$=0, 1, 2). The process $e^+e^-\to \omega\chi_{c0}$ is observed for the first time, and the Born cross sections at $\sqrt{s}$=4.23 and 4.26 GeV are measured to be $(55.4\pm 6.0\pm 5.9)$ and $(23.7\pm 5.3\pm 3.5)$ pb, respectively, where the first uncertainties are statistical and the second are systematic. The $\omega\chi_{c0}$ signals at the other 7 energies and $e^+e^-\to \omega\chi_{c1}$ and $\omega\chi_{c2}$ signals are not significant, and the upper limits on the cross sections are determined. By examining the $\omega\chi_{c0}$ cross section as a function of center-of-mass energy, we find that it is inconsistent with the line shape of the $Y(4260)$ observed in $e^+ e^-\to\pi^+\pi^-J/\psi$. Assuming the $\omega\chi_{c0}$ signals come from a single resonance, we extract mass and width of the resonance to be $(4230\pm8\pm6)$ MeV/$c^2$ and $(38\pm12\pm2)$ MeV, respectively, and the statistical significance is more than $9\sigma$.

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