Observation of a charged charmoniumlike structure in e+e−→(D∗Dˉ∗)±π∓e^+e^- \to (D^{*} \bar{D}^{*})^{\pm} π^\mp at s=4.26\sqrt{s}=4.26GeV

preprint2014arXivOpen access
BESIII CollaborationM. AblikimM. N. AchasovO. AlbayrakD. J. AmbroseF. F. AnQ. AnJ. Z. BaiR. Baldini FerroliY. BanJ. BeckerJ. V. BennettM. BertaniJ. M. BianE. BogerO. BondarenkoI. BoykoS. BraunR. A. BriereV. BytevH. CaiX. CaiO. CakirA. CalcaterraG. F. CaoS. A. CetinJ. F. ChangG. ChelkovG. ChenH. S. ChenJ. C. ChenM. L. ChenS. J. ChenX. R. ChenY. B. ChenH. P. ChengY. P. ChuD. Cronin-HennessyH. L. DaiJ. P. DaiD. DedovichZ. Y. DengA. DenigI. DenysenkoM. DestefanisW. M. DingY. DingL. Y. DongM. Y. DongS. X. DuJ. FangS. S. FangL. FavaC. Q. FengP. FriedelC. D. FuJ. L. FuO. FuksY. GaoC. GengK. GoetzenW. X. GongW. GradlM. GrecoM. H. GuY. T. GuY. H. GuanA. Q. GuoL. B. GuoT. GuoY. P. GuoY. L. HanF. A. HarrisK. L. HeM. HeZ. Y. HeT. HeldY. K. HengZ. L. HouC. HuH. M. HuJ. F. HuT. HuG. M. HuangG. S. HuangJ. S. HuangL. HuangX. T. HuangY. HuangT. HussainC. S. JiQ. JiQ. P. JiX. B. JiX. L. JiL. L. JiangX. S. JiangJ. B. JiaoZ. JiaoD. P. JinS. JinF. F. JingN. Kalantar-NayestanakiM. KavatsyukB. KlossB. KopfM. KornicerW. KuehnW. LaiJ. S. LangeM. LaraP. LarinM. LeyheC. H. LiCheng LiCui LiD. M. LiF. LiG. LiH. B. LiJ. C. LiK. LiLei LiP. R. LiQ. J. LiW. D. LiW. G. LiX. L. LiX. N. LiX. Q. LiX. R. LiZ. B. LiH. LiangY. F. LiangY. T. LiangG. R. LiaoX. T. LiaoD. X. LinB. J. LiuC. L. LiuC. X. LiuF. H. LiuFang LiuFeng LiuH. LiuH. B. LiuH. H. LiuH. M. LiuH. W. LiuJ. P. LiuK. LiuK. Y. LiuL. D. LiuP. L. LiuQ. LiuS. B. LiuX. LiuY. B. LiuZ. A. LiuZhiqiang LiuZhiqing LiuH. LoehnerX. C. LouG. R. LuH. J. LuJ. G. LuX. R. LuY. P. LuC. L. LuoM. X. LuoT. LuoX. L. LuoM. LvF. C. MaH. L. MaQ. M. MaS. MaT. MaX. Y. MaF. E. MaasM. MaggioraQ. A. MalikY. J. MaoZ. P. MaoJ. G. MesschendorpJ. MinT. J. MinR. E. MitchellX. H. MoH. MoeiniC. Morales MoralesK. MoriyaN. Yu. MuchnoiH. MuramatsuY. NefedovI. B. NikolaevZ. NingS. L. OlsenQ. OuyangS. PacettiJ. W. ParkM. PelizaeusH. P. PengK. PetersJ. L. PingR. G. PingR. PolingE. PrencipeM. QiS. QianC. F. QiaoL. Q. QinX. S. QinY. QinZ. H. QinJ. F. QiuK. H. RashidC. F. RedmerG. RongX. D. RuanA. SarantsevM. ShaoC. P. ShenX. Y. ShenH. Y. ShengM. R. ShepherdW. M. SongX. Y. SongS. SpataroB. SpruckD. H. SunG. X. SunJ. F. SunS. S. SunY. J. SunY. Z. SunZ. J. SunZ. T. SunC. J. TangX. TangI. TapanE. H. ThorndikeD. TothM. UllrichI. UmanG. S. VarnerB. WangD. WangD. Y. WangK. WangL. L. WangL. S. WangM. WangP. WangP. L. WangQ. J. WangS. G. WangX. F. WangX. L. WangY. D. WangY. F. WangY. Q. WangZ. WangZ. G. WangZ. Y. WangD. H. WeiJ. B. WeiP. WeidenkaffQ. G. WenS. P. WenM. WernerU. WiednerL. H. WuN. WuS. X. WuW. WuZ. WuL. G. XiaY. X XiaZ. J. XiaoY. G. XieQ. L. XiuG. F. XuQ. J. XuQ. N. XuX. P. XuZ. R. XuZ. XueL. YanW. B. YanY. H. YanH. X. YangY. YangY. X. YangH. YeM. YeM. H. YeB. X. YuC. X. YuH. W. YuJ. S. YuS. P. YuC. Z. YuanY. YuanA. A. ZafarA. ZalloS. L. ZangY. ZengB. X. ZhangB. Y. ZhangC. ZhangC. C. ZhangD. H. ZhangH. H. ZhangH. Y. ZhangL. ZhangJ. Q. ZhangJ. W. ZhangJ. Y. ZhangJ. Z. ZhangR. ZhangS. H. ZhangX. J. ZhangX. Y. ZhangY. ZhangY. H. ZhangZ. P. ZhangZ. Y. ZhangZhenghao ZhangG. ZhaoH. S. ZhaoJ. W. ZhaoLei ZhaoLing ZhaoM. G. ZhaoQ. ZhaoS. J. ZhaoT. C. ZhaoX. H. ZhaoY. B. ZhaoZ. G. ZhaoA. ZhemchugovB. ZhengJ. P. ZhengY. H. ZhengB. ZhongL. ZhouX. ZhouX. K. ZhouX. R. ZhouC. ZhuK. ZhuK. J. ZhuS. H. ZhuX. L. ZhuY. C. ZhuY. S. ZhuZ. A. ZhuJ. ZhuangB. S. ZouJ. H. Zou

Abstract

We study the process e+e−→(D∗Dˉ∗)±π∓e^+e^- \to (D^{*} \bar{D}^{*})^{\pm} π^\mp at a center-of-mass energy of 4.26GeV using a 827pb−1^{-1} data sample obtained with the BESIII detector at the Beijing Electron Positron Collider. Based on a partial reconstruction technique, the Born cross section is measured to be (137±9±15)(137\pm9\pm15)pb. We observe a structure near the (D∗Dˉ∗)±(D^{*} \bar{D}^{*})^{\pm} threshold in the π∓π^\mp recoil mass spectrum, which we denote as the Zc±(4025)Z^{\pm}_c(4025). The measured mass and width of the structure are (4026.3±2.6±3.7)(4026.3\pm2.6\pm3.7)MeV/c2^2 and (24.8±5.6±7.7)(24.8\pm5.6\pm7.7)MeV, respectively. Its production ratio σ(e+e−→Zc±(4025)π∓→(D∗Dˉ∗)±π∓)σ(e+e−→(D∗Dˉ∗)±π∓)\frac{σ(e^+e^-\to Z^{\pm}_c(4025)π^\mp \to (D^{*} \bar{D}^{*})^{\pm} π^\mp)}{σ(e^+e^-\to (D^{*} \bar{D}^{*})^{\pm} π^\mp)} is determined to be 0.65±0.09±0.060.65\pm0.09\pm0.06. The first uncertainties are statistical and the second are systematic.

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