期刊
CHINESE PHYSICS C
卷 44, 期 4, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/1674-1137/44/4/040001
关键词
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资金
- National Key Basic Research Program of China [2015CB856700]
- National Natural Science Foundation of China (NSFC) [11335008, 11425524, 11625523, 11635010, 11735014, 11822506, 11935018]
- Chinese Academy of Sciences (CAS) Large-Scale Scientific Facility Program
- CAS Center for Excellence in Particle Physics (CCEPP)
- NSFC [U1532257, U1532258, U1732263]
- CAS [U1532257, U1532258, U1732263]
- CAS Key Research Program of Frontier Science [QYZDJ-SSW-SLH003, QYZDJ-SSW-SLH040]
- 100 Talents Program of CAS
- CAS PIFI
- Thousand Talents Program of China
- Shanghai Key Laboratory for Particle Physics and Cosmology
- German Research Foundation DFG [Collaborative Research Center CRC 104, FOR 2359]
- Istituto Nazionale di Fisica Nucleare, Italy
- Koninklijke Nederlandse Akademie van Wetenschappen (KNAW) [530-4CDP03]
- Ministry of Development of Turkey [DPT2006K-120470]
- National Science and Technology fund
- Knut and Alice Wallenberg Foundation (Sweden) [2016.0157]
- Swedish Research Council
- U.S. Department of Energy [DE-FG02-05ER41374, DESC-0010118, DE-SC-0012069]
- University of Groningen (RuG), Darmstadt
- Helmholtzzentrum fuer Schwerionenforschung GmbH (GSI), Darmstadt
- Russian Ministry of Science and Higher Education [14.W03.31.0026]
- INPAC
There has recently been a dramatic renewal of interest in hadron spectroscopy and charm physics. This renaissance has been driven in part by the discovery of a plethora of charmonium-like XYZ states at BESIII and B factories, and the observation of an intriguing proton-antiproton threshold enhancement and the possibly related X(1835) meson state at BESIII, as well as the threshold measurements of charm mesons and charm baryons. We present a detailed survey of the important topics in tau-charm physics and hadron physics that can be further explored at BESIII during the remaining operation period of BEPCII. This survey will help in the optimization of the data-taking plan over the coming years, and provides physics motivation for the possible upgrade of BEPCII to higher luminosity.
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