학술논문

Dark photon search in the mass range between 1.5 and 3.4 GeV/c2
Document Type
article
Author
M. AblikimM.N. AchasovX.C. AiO. AlbayrakM. AlbrechtD.J. AmbroseA. AmorosoF.F. AnQ. AnJ.Z. BaiR. Baldini FerroliY. BanD.W. BennettJ.V. BennettM. BertaniD. BettoniJ.M. BianF. BianchiE. BogerI. BoykoR.A. BriereH. CaiX. CaiO. CakirA. CalcaterraG.F. CaoS.A. CetinJ.F. ChangG. ChelkovG. ChenH.S. ChenH.Y. ChenJ.C. ChenM.L. ChenS.J. ChenX. ChenX.R. ChenY.B. ChenH.P. ChengX.K. ChuG. CibinettoH.L. DaiJ.P. DaiA. DbeyssiD. DedovichZ.Y. DengA. DenigI. DenysenkoM. DestefanisF. De MoriY. DingC. DongJ. DongL.Y. DongM.Y. DongS.X. DuP.F. DuanE.E. ErenJ.Z. FanJ. FangS.S. FangX. FangY. FangL. FavaF. FeldbauerG. FeliciC.Q. FengE. FioravantiM. FritschC.D. FuQ. GaoX.Y. GaoY. GaoZ. GaoI. GarziaC. GengK. GoetzenW.X. GongW. GradlM. GrecoM.H. GuY.T. GuY.H. GuanA.Q. GuoL.B. GuoY. GuoY.P. GuoZ. HaddadiA. HafnerS. HanY.L. HanX.Q. HaoF.A. HarrisK.L. HeZ.Y. HeT. HeldY.K. HengZ.L. HouC. HuH.M. HuJ.F. HuT. HuY. HuG.M. HuangG.S. HuangH.P. HuangJ.S. HuangX.T. HuangY. HuangT. HussainQ. JiQ.P. JiX.B. JiX.L. JiL.L. JiangL.W. JiangX.S. JiangX.Y. JiangJ.B. JiaoZ. JiaoD.P. JinS. JinT. JohanssonA. JulinN. Kalantar-NayestanakiX.L. KangX.S. KangM. KavatsyukB.C. KeP. KieseR. KliemtB. KlossO.B. KolcuB. KopfM. KornicerW. KuehnA. KupscJ.S. LangeM. LaraP. LarinC. LengC. LiC.H. LiCheng LiD.M. LiF. LiG. LiH.B. LiJ.C. LiJin LiK. LiLei LiP.R. LiT. LiW.D. LiW.G. LiX.L. LiX.M. LiX.N. LiX.Q. LiZ.B. LiH. LiangY.F. LiangY.T. LiangG.R. LiaoD.X. LinB.J. LiuC.X. LiuF.H. LiuFang LiuFeng LiuH.B. LiuH.H. LiuH.M. LiuJ. LiuJ.B. LiuJ.P. LiuJ.Y. LiuK. LiuK.Y. LiuL.D. LiuP.L. LiuQ. LiuS.B. LiuX. LiuX.X. LiuY.B. LiuZ.A. LiuZhiqiang LiuZhiqing LiuH. LoehnerX.C. LouH.J. LuJ.G. LuR.Q. LuY. LuY.P. LuC.L. LuoM.X. LuoT. LuoX.L. LuoM. LvX.R. LyuF.C. MaH.L. MaL.L. MaQ.M. MaT. MaX.N. MaX.Y. MaF.E. MaasM. MaggioraY.J. MaoZ.P. MaoS. MarcelloJ.G. MesschendorpJ. MinT.J. MinR.E. MitchellX.H. MoY.J. MoC. Morales MoralesK. MoriyaN.Yu. MuchnoiH. MuramatsuY. NefedovF. NerlingI.B. NikolaevZ. NingS. NisarS.L. NiuX.Y. NiuS.L. OlsenQ. OuyangS. PacettiP. PatteriM. PelizaeusH.P. PengK. PetersJ. PetterssonJ.L. PingR.G. PingR. PolingV. PrasadY.N. PuM. QiS. QianC.F. QiaoL.Q. QinN. QinX.S. QinY. QinZ.H. QinJ.F. QiuK.H. RashidC.F. RedmerH.L. RenM. RipkaG. RongCh. RosnerX.D. RuanV. SantoroA. SarantsevM. SavriéK. SchoenningS. SchumannW. ShanM. ShaoC.P. ShenP.X. ShenX.Y. ShenH.Y. ShengW.M. SongX.Y. SongS. SosioS. SpataroG.X. SunJ.F. SunS.S. SunY.J. SunY.Z. SunZ.J. SunZ.T. SunC.J. TangX. TangI. TapanE.H. ThorndikeM. TiemensM. UllrichI. UmanG.S. VarnerB. WangB.L. WangD. WangD.Y. WangK. WangL.L. WangL.S. WangM. WangP. WangP.L. WangS.G. WangW. WangX.F. WangY.D. WangY.F. WangY.Q. WangZ. WangZ.G. WangZ.H. WangZ.Y. WangT. WeberD.H. WeiJ.B. WeiP. WeidenkaffS.P. WenU. WiednerM. WolkeL.H. WuZ. WuL.G. XiaY. XiaD. XiaoH. XiaoZ.J. XiaoY.G. XieQ.L. XiuG.F. XuL. XuQ.J. XuQ.N. XuX.P. XuL. YanW.B. YanW.C. YanY.H. YanH.J. YangH.X. YangL. YangY. YangY.X. YangH. YeM. YeM.H. YeJ.H. YinB.X. YuC.X. YuH.W. YuJ.S. YuC.Z. YuanW.L. YuanY. YuanA. YuncuA.A. ZafarA. ZalloY. ZengB.X. ZhangB.Y. ZhangC. ZhangC.C. ZhangD.H. ZhangH.H. ZhangH.Y. ZhangJ.J. ZhangJ.L. ZhangJ.Q. ZhangJ.W. ZhangJ.Y. ZhangJ.Z. ZhangK. ZhangL. ZhangS.H. ZhangX.Y. ZhangY. ZhangY.N. ZhangY.H. ZhangY.T. ZhangYu ZhangZ.H. ZhangZ.P. ZhangZ.Y. ZhangG. ZhaoJ.W. ZhaoJ.Y. ZhaoJ.Z. ZhaoLei ZhaoLing ZhaoM.G. ZhaoQ. ZhaoQ.W. ZhaoS.J. ZhaoT.C. ZhaoY.B. ZhaoZ.G. ZhaoA. ZhemchugovB. ZhengJ.P. ZhengW.J. ZhengY.H. ZhengB. ZhongL. ZhouLi ZhouX. ZhouX.K. ZhouX.R. ZhouX.Y. ZhouK. ZhuK.J. ZhuS. ZhuX.L. ZhuY.C. ZhuY.S. ZhuZ.A. ZhuJ. ZhuangL. ZottiB.S. ZouJ.H. Zou
Source
Physics Letters B, Vol 774, Iss C, Pp 252-257 (2017)
Subject
Dark photon search
Initial state radiation
BESIII
Physics
QC1-999
Language
English
ISSN
0370-2693
1873-2445
Abstract
Using a data set of 2.93 fb−1 taken at a center-of-mass energy s=3.773 GeV with the BESIII detector at the BEPCII collider, we perform a search for an extra U(1) gauge boson, also denoted as a dark photon. We examine the initial state radiation reactions e+e−→e+e−γISR and e+e−→μ+μ−γISR for this search, where the dark photon would appear as an enhancement in the invariant mass distribution of the leptonic pairs. We observe no obvious enhancement in the mass range between 1.5 and 3.4 GeV/c2 and set a 90% confidence level upper limit on the mixing strength of the dark photon and the Standard Model photon. We obtain a competitive limit in the tested mass range.