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| 1 | Future Physics Programme of BESⅢ显示文摘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. | M.Ablikim M.N.Achasov P.Adlarson S.Ahmed M.Albrecht M.Alekseev A.Amoroso F.F.An Q.An Y.Bai O.Bakina R.Baldini Ferroli Y.Ban K.Begzsuren J.V.Bennett N.Berger M.Bertani D.Bettoni F.Bianchi J Biernat J.Bloms I.Boyko R.A.Briere L.Calibbi H.Cai X.Cai A.Calcaterra G.F.Cao N.Cao S.A.Cetin J.Chai J.F.Chang W.L.Chang J.Charles G.Chelkov Chen G.Chen H.S.Chen J.C.Chen M.L.Chen S.J.Chen Y.B.Chen H.Y.Cheng W.Cheng G.Cibinetto F.Cossio X.F.Cui H.L.Dai J.P.Dai X.C.Dai A.Dbeyssi D.Dedovich Z.Y.Deng A.Denig Denysenko M.Destefanis S.Descotes-Genon F.De Mori Y.Ding C.Dong J.Dong L.Y.Dong M.Y.Dong Z.L.Dou S.X.Du S.I.Eidelman J.Z.Fan J.Fang S.S.Fang Y.Fang R.Farinelli L.Fava F.Feldbauer G.Felici C.Q.Feng M.Fritsch C.D.Fu Y.Fu Q.Gao X.L.Gao Y.Gao Y.Gao Y.G.Gao Z.Gao B.Garillon I.Garzia E.M.Gersabeck A.Gilman K.Goetzen L.Gong W.X.Gong W.Gradl M.Greco L.M.Gu M.H.Gu Y.T.Gu A.Q.Guo F.K.Guo L.B.Guo R.P.Guo Y.P.Guo A.Guskov S.Han X.Q.Hao F.A.Harris K.L.He F.H.Heinsius T.Held Y.K.Heng Y.R.Hou Z.L.Hou H.M.Hu J.F.Hu T.Hu Y.Hu G.S.Huang J.S.Huang X.T.Huang X.Z.Huang Z.L.Huang N.Huesken T.Hussain W.Ikegami Andersson W.Imoehl M.Irshad Q.Ji Q.P.Ji X.B.Ji X.L.Ji H.L.Jiang X.S.Jiang X.Y.Jiang J.B.Jiao Z.Jiao D.P.Jin S.Jin Y.Jin T.Johansson N.Kalantar-Nayestanaki X.S.Kang R.Kappert M.Kavatsyuk B.C.Ke I.K.Keshk T.Khan A.Khoukaz P.Kiese R.Kiuchi R.Kliemt L.Koch O.B.Kolcu B.Kopf M.Kuemmel M.Kuessner A.Kupsc M.Kurth M.G.Kurth W.Kuhn J.S.Lange P.Larin L.Lavezzi H.Leithoff T.Lenz C.Li Cheng Li D.M.Li F.Li F.Y.Li G.Li H.B.Li H.J.Li J.C.Li J.W.Li Ke Li L.K.Li Lei Li P.L.Li P.R.Li Q.Y.Li W.D.Li W.G.Li X.H.Li X.L.Li X.N.Li X.Q.Li Z.B.Li H.Liang H.Liang Y.F.Liang Y.T.Liang G.R.Liao L.Z.Liao J.Libby C.X.Lin D.X.Lin Y.J.Lin B.Liu B.J.Liu C.X.Liu D.Liu D.Y.Liu F.H.Liu Fang Liu Feng Liu H.B.Liu H.M.Liu Huanhuan Liu Huihui Liu J.B.Liu J.Y.Liu K.Y.Liu Ke Liu Q.Liu S.B.Liu T.Liu X.Liu X.Y.Liu Y.B.Liu Z.A.Liu Zhiqing Liu Y.F.Long X.C.Lou H.J.Lu J.D.Lu J.G.Lu Y.Lu Y.P.Lu C.L.Luo M.X.Luo P.W.Luo T.Luo X.L.Luo S.Lusso X.R.Lyu F.C.Ma H.L.Ma L.L.Ma M.M.Ma Q.M.Ma X.N.Ma X.X.Ma X.Y.Ma Y.M.Ma F.E.Maas M.Maggiora S.Maldaner S.Malde Q.A.Malik A.Mangoni Y.J.Mao Z.P.Mao S.Marcello Z.X.Meng J.G.Messchendorp G.Mezzadri J.Min T.J.Min R.E.Mitchell X.H.Mo Y.J.Mo C.Morales Morales N.Yu.Muchnoi H.Muramatsu A.Mustafa S.Nakhoul Y.Nefedov F.Nerling I.B.Nikolaev Z.Ning S.Nisar S.L.Niu S.L.Olsen Q.Ouyang S.Pacetti Y.Pan M.Papenbrock P.Patteri M.Pelizaeus H.P.Peng K.Peters A.A.Petrov J.Pettersson J.L.Ping R.G.Ping A.Pitka R.Poling V.Prasad M.Qi T.Y.Qi S.Qian C.F.Qiao N.Qin X.P.Qin X.S.Qin Z.H.Qin J.F.Qiu S.Q.Qu K.H.Rashid C.F.Redmer M.Richter M.Ripka A.Rivetti V.Rodin M.Rolo G.Rong J.L.Rosner Ch.Rosner M.Rump A.Sarantsev M.Savrie K.Schoenning W.Shan X.Y.Shan M.Shao C.P.Shen P.X.Shen X.Y.Shen H.Y.Sheng X.Shi X.D Shi J.J.Song Q.Q.Song X.Y.Song S.Sosio C.Sowa S.Spataro F.F.Sui G.X.Sun J.F.Sun L.Sun S.S.Sun X.H.Sun Y.J.Sun Y.K Sun Y.Z.Sun Z.J.Sun Z.T.Sun Y.T Tan C.J.Tang G.Y.Tang X.Tang V.Thoren B.Tsednee I.Uman B.Wang B.L.Wang C.W.Wang D.Y.Wang H.H.Wang K.Wang L.L.Wang L.S.Wang M.Wang M.Z.Wang Wang Meng P.L.Wang R.M.Wang W.P.Wang X.Wang X.F.Wang X.L.Wang Y.Wang Y.F.Wang Z.Wang Z.G.Wang Z.Y.Wang Zongyuan Wang T.Weber D.H.Wei P.Weidenkaff H.W.Wen S.P.Wen U.Wiedner G.Wilkinson M.Wolke L.H.Wu L.J.Wu Z.Wu L.Xia Y.Xia S.Y.Xiao Y.J.Xiao Z.J.Xiao Y.G.Xie Y.H.Xie T.Y.Xing X.A.Xiong Q.L.Xiu G.F.Xu L.Xu Q.J.Xu W.Xu X.P.Xu F.Yan L.Yan W.B.Yan W.C.Yan Y.H.Yan H.J.Yang H.X.Yang L.Yang R.X.Yang S.L.Yang Y.H.Yang Y.X.Yang Yifan Yang Z.Q.Yang M.Ye M.H.Ye J.H.Yin Z.Y.You B.X.Yu C.X.Yu J.S.Yu C.Z.Yuan X.Q.Yuan Y.Yuan A.Yuncu A.A.Zafar Y.Zeng B.X.Zhang B.Y.Zhang C.C.Zhang D.H.Zhang H.H.Zhang H.Y.Zhang J.Zhang J.L.Zhang J.Q.Zhang J.W.Zhang J.Y.Zhang J.Z.Zhang K.Zhang L.Zhang S.F.Zhang T.J.Zhang X.Y.Zhang Y.Zhang Y.H.Zhang Y.T.Zhang Yang Zhang Yao Zhang Yi Zhang Yu Zhang Z.H.Zhang Z.P.Zhang Z.Q.Zhang Z.Y.Zhang G.Zhao J.W.Zhao J.Y.Zhao J.Z.Zhao Lei Zhao Ling Zhao M.G.Zhao Q.Zhao S.J.Zhao T.C.Zhao Y.B.Zhao Z.G.Zhao A.Zhemchugov B.Zheng J.P.Zheng Y.Zheng Y.H.Zheng B.Zhong L.Zhou L.P.Zhou Q.Zhou X.Zhou X.K.Zhou Xingyu Zhou Xiaoyu Zhou Xu Zhou A.N.Zhu J.Zhu J.Zhu K.Zhu K.J.Zhu S.H.Zhu W.J.Zhu X.L.Zhu Y.C.Zhu Y.S.Zhu Z.A.Zhu J.Zhuang B.S.Zou J.H.Zou 无 | 2020 | Chinese Physics C2020，44，4： | 517 |
| 2 | Statistical moment-based structural damage detection method in time domain显示文摘A novel structural damage detection method with a new damage index,i.e.,the statistical moment-based damage detection(SMBDD) method in the frequency domain,has been recently proposed.The aim of this study is to extend the SMBDD method in the frequency domain to the time domain for building structures subjected to non-Gaussian and non-stationary excitations.The applicability and effectiveness of the SMBDD method in the time domainis verified both numerically and experimentally.Shear buildings with various damage scenarios are first numerically investigated in the time domain taking into account the effect of measurement noise.The applicability of the proposed method in the time domain to building structures subjected to non-Gaussian and non-stationary excitations is then experimentally investigated through a series of shaking table tests,in which two three-story shear building models with four damage scenarios aretested.The identified damage locations and severities are then compared with the preset values.The comparative results are found to be satisfactory,and the SMBDD method is shown to be feasible and effective for building structures subjected to non-Gaussian and non-stationary excitations. | J.Zhang Y.L.Xu J.Li Y.Xia J.C.Li | 2013 | Earthquake Engineering and Engineering Vibration2013，12，1： | 6 |
| 3 | 查看详情显示文摘 | Y.Xia D.Qian D.Hsieh L.Wray A.Pal H.Lin A.Bansil D.Grauer Y.S.Hor R.J.Cava and M.Z.Hasan | | 0，，： | 1 |
| 4 | Predictive control of Networked systems with random network delays and data dropout显示文摘 | Y.Xia G.-P.Liu M.Fu | | 0，，03： | 1 |
| 5 | 查看详情显示文摘 | D.Hsieh Y.Xia D.Qian L.Wray F.Meier J.H.Dil J.Osterwalder L.Patthey A.V.Fedorov H.Lin A.Bansil D.Grauer Y.S.Hor R.J.Cara and M.Z.Hasan | | 0，，14： | 1 |
| 6 | 查看详情显示文摘 | L.A.Wray S.Y.Xu Y.Xia Y.S.Hor D.Qian A.V.Fedorov H.Lin A.Bansil R.J.Cara and M.Z.Hasan | | 0，，： | 1 |
| 7 | Photonic Papers and Inks: Color Writing with Colorless Materials显示文摘 | N.Fudouzi Y.Xia | | 0，，11： | 1 |
| 8 | 查看详情显示文摘 | D.Hsieh Y.Xia D.Qian L.Wray J.H.Dil F.Meier J.Osterwalder L.Patthey J.G.Checkelsky N.P.Ong A.V.Fedorov H.Lin A.Bansil D.Grauer Y.S.Hor R.J.Cavs and M.Z.Hasan | | 0，，： | 1 |
| 9 | Application Prospect of Fission-Powered Spacecraft in Solar System Exploration Missions显示文摘Fission power is a promising technology,and it has been proposed for several future space uses.It is being considered for highpower missions whose goal is to explore the solar system and even beyond.Space fission power has made great progress when NASA’s 1 kWe Kilowatt Reactor Using Stirling TechnologY(KRUSTY)prototype completed a full power scale nuclear test in 2018.Its success stimulated a new round of research competition among the major space countries.This article reviews the development of the Kilopower reactor and the KRUSTY system design.It summarizes the current missions that fission reactors are being considered as a power and/or propulsion source.These projects include visiting Jupiter and Saturn systems,Chiron,and Kuiper belt object;Neptune exploration missions;and lunar and Mars surface base missions.These studies suggest that the Fission Electric Propulsion(FEP)/Fission Power System(FPS)is better than the Radioisotope Electric Propulsion(REP)/Radioisotope Power System(RPS)in the aspect of cost for missions with a power level that reaches~1 kWe,and when the power levels reaches~8 kWe,it has the advantage of lower mass.For a mission that travels further than~Saturn,REP with plutonium may not be cost acceptable,leaving FEP the only choice.Surface missions prefer the use of FPS because it satisfies the power level of 10’s kWe,and FPS vastly widens the choice of possible landing location.According to the current situation,we are expecting a flagship-level fission-powered space exploration mission in the next 1-2 decades. | Y.Xia J.Li R.Zhai J.Wang B.Lin Q.Zhou | 2021 | Space(Science & Technology)2021，，1： | 1 |
| 10 | 查看详情显示文摘 | Y.Xia D.Qian D.Hsieh L.Wray A.Pal H.Lin A.Bansil D.Grauer Y.S.Hor R.J.Cava and M.Z.Hasan | | 0，，06： | 1 |
| 11 | Monodispersed Colloidal Spheres: Old Materials with New Applications显示文摘 | Y.Xia B.Gates Y.Yin Y.Lu | 2000 | Adv Mater2000，，10： | 1 |
| 12 | Methylenetetrahydrofolate reductase C677T polymorphism and the risk of male infertility: a meta‐analysis显示文摘 | W.Wu O.Shen Y.Qin J.Lu X.Niu Z.Zhou C.Lu Y.Xia S.Wang X.Wang | 2012 | International Journal of Andrology2012，，1： | 1 |
| 13 | 查看详情显示文摘 | Y.Xia D.Qian D.Hsieh L.Wray A.Pal H.Lin A.Bansil D.Grauer Y.Hor R.Cava and M.Z.Hasan | | 0，，： | 1 |
| 14 | 查看详情显示文摘 | D.Hsieh Y.Xia D.Qian L.Wray J.H.Dil F.Meier J.Osterwalder L.Patthey J.G.Checkelsky N.P.Ong A.V.Fedorov H.Lin A.Bansil D.Grauer Y.S.Hor R.J.Cava and M.Z.Hasan | | 0，，： | 1 |
| 15 | 查看详情显示文摘 | Y.Xia D.Qian D.Hsieh L.Wray A.Pal H.Lin A.Bansil D.Grauer Y.S.Hor R.J.Cava and M.Z.Hasan | | 0，，： | 1 |
| 16 | 查看详情显示文摘 | D.Hsieh Y.Xia D.Qian L.Wray F.Meier J.H.Dil J.Osterwalder L.Patthey A.V.Fedorov H.Lin A.Bansil D.Grauer Y.S.Hor R.J.Cava and M.Z.Hasan | | 0，，： | 1 |
| 17 | 查看详情显示文摘 | Z. Wang J. Xia X. Qiang Y.Xia G.Shi F.Zhang G.Han L.Xia J.Tang | | 0，，： | 1 |
| 18 | 查看详情显示文摘 | H.Lin L.Wray Y.Xia S.Xu S.Jia R.Cava A.Bansil and M.Hasan | | 0，，： | 1 |
| 19 | 查看详情显示文摘 | Y.Xia D.Qian D.Hsieh L.Wray A.Pal H.Lin A.Bansil D.Grauer Y.S.Hor R.J.Cava and M.Z.Hasan | | 0，，06： | 1 |
| 20 | 查看详情显示文摘 | Y.S.Hot A.Richardella P.Roushan Y.Xia J.G.Checkelsky A.Yazdani M.Z.Hasan N.P.Ong and R.J.Cava | | 0，，19： | 1 |
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