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Evidence for particle acceleration approaching PeV energies in the W51 complex

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Science Bulletin 2024年第18期69卷 2833-2841页

作者： LhAASO Collaboration Zhen Cao F.Aharonian Axikegu Y.X.Bai Y.W.Bao D.Bastieri X.J.Bi Y.J.Bi W.Bian A.V.Bukevich q.Cao W.Y.Cao Zhe Cao J.Chang J.F.Chang A.M.Chen E.S.Chen h.X.Chen Liang Chen Lin Chen Long Chen M.J.Chen M.L.Chen q.h.Chen S.Chen S.h.Chen S.Z.Chen T.L.Chen Y.Chen N.Cheng Y.D.Cheng M.Y.Cui S.W.Cui X.h.Cui Y.D.Cui B.Z.Dai h.L.Dai Z.G.Dai Danzengluobu X.q.Dong K.K.Duan J.h.Fan Y.Z.Fan J.Fang J.h.Fang K.Fang C.F.Feng h.Feng L.Feng S.h.Feng X.T.Feng Y.Feng Y.L.Feng S.Gabici B.Gao C.D.Gao q.Gao W.Gao W.K.Gao M.M.Ge L.S.Geng G.Giacinti G.h.Gong q.B.Gou M.h.Gu F.L.Guo X.L.Guo Y.q.Guo Y.Y.Guo Y.A.han M.hasan h.h.he h.N.he J.Y.he Y.he Y.K.hor B.W.hou C.hou X.hou h.B.hu q.h. S.C.hu D.h.huang T.q.h.ang W.J.huang X.T.huang X.Y.huang Y.huang X.L.Ji h.Y.Jia K.Jia K.Jiang X.W.Jiang Z.J.Jiang M.Jin M.M.Kang I.Karpikov D.Kuleshov K.Kurinov B.B.Li C.M.Li Cheng Li Cong Li D.Li F.Li h.B.Li h.C.Li Jian Li Jie Li K.Li S.D.Li W.L.Li W.L.Li X.R.Li Xin Li Y.Z.Li Zhe Li Zhuo Li E.W.Liang Y.F.Liang S.J.Lin B.Liu C.Liu D.Liu D.B.Liu h.Liu h.D.Liu J.Liu J.L.Liu M.Y.Liu R.Y.Liu S.M.Liu W.Liu Y.Liu Y.N.Liu q.Luo Y.Luo h.K.Lv B.q.Ma L.L.Ma X.h.Ma J.R.Mao Z.Min W.Mitthumsiri h.J.Mu Y.C.Nan A.Neronov L.J.Ou P.Pattarakijwanich Z.Y.Pei J.C.qi M.Y.qi B.q.qiao J.J.qin A.Raza D.Ruffolo A.Sáiz M.Saeed D.Semikoz L.Shao O.Shchegolev X.D.Sheng F.W.Shu h.C.Song Yu.V.Stenkin V.Stepanov Y.Su D.X.Sun q.N.Sun X.N.Sun Z.B.Sun J.Takata P.h.T.Tam q.W.Tang R.Tang Z.B.Tang W.W.Tian C.Wang C.B.Wang G.W.Wang h.G.Wang h.h.Wang J.C.Wang Kai Wang Kai Wang L.P.Wang L.Y.Wang P.h.Wang R.Wang W.Wang X.G.Wang X.Y.Wang Y.Wang Y.D.Wang Y.J.Wang Z.h.Wang Z.X.Wang Zhen Wang Zheng Wang D.M.Wei J.J.Wei Y.J.Wei T.Wen C.Y.Wu h.R.Wu q.W.Wu S.Wu X.F.Wu Y.S.Wu S.q.Xi J.Xia G.M.Xiang D.X.Xiao G.Xiao Y.L.Xin Y.Xing D.R.Xiong Z.Xiong D.L.Xu R.F.Xu R.X.Xu W.L.Xu L.Xue D.h.Yan J.Z.Yan T.Yan C.W.Yang C.Y.Yang F.Yang F.F.Yang L.L.Yang M.J.Yang R.Z.Yang W.X.Yang Y.h.Yao Z.G.Yao L.q.Yin N.Yin X.h.You Z.Y.You Y.h.Yu q.Yuan h.Yue h.D.Zeng T.X.Zeng W.Zeng M.Zha B.B.Zhang F.Zhang h.Zhang 不详 Key Laboratory of Particle Astrophysics&Experimental Physics Division&Computing Center Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China University of Chinese Academy of Sciences Beijing 100049China TIANFU Cosmic Ray Research Center ChengduChina Dublin Institute for Advanced Studies 31 Fitzwilliam Place2 DublinIreland Max-Planck-Institut for Nuclear Physics P.O.Box 103980Heidelberg 69029Germany School of Physical Science and Technology&School of Information Science and Technology Southwest Jiaotong UniversityChengdu 610031China School of Astronomy and Space Science Nanjing UniversityNanjing 210023China Center for Astrophysics Guangzhou UniversityGuangzhou 510006China Tsung-Dao Lee Institute&School of Physics and Astronomy Shanghai Jiao Tong UniversityShanghai 200240China Institute for Nuclear Research of Russian Academy of Sciences Moscow 117312Russia hebei Normal University Shijiazhuang 050024China University of Science and Technology of China Hefei 230026China State Key Laboratory of Particle Detection and Electronics China Key Laboratory of Dark Matter and Space Astronomy&Key Laboratory of Radio Astronomy Purple Mountain ObservatoryChinese Academy of SciencesNanjing 210023China Research Center for Astronomical Computing Zhejiang LaboratoryHangzhou 311121China Key Laboratory for Research in Galaxies and Cosmology Shanghai Astronomical ObservatoryChinese Academy of SciencesShanghai 200030China School of Physics and Astronomy Yunnan UniversityKunming 650091China Key Laboratory of Cosmic Rays(Tibet University) Ministry of EducationLhasa 850000China National Astronomical Observatories Chinese Academy of SciencesBeijing 100101China School of Physics and Astronomy(Zhuhai)&School of Physics(Guangzhou)&Sino-French Institute of Nuclear Engineering and Technology(Zhuhai) Sun Yat-sen UniversityZhuhai 519000&Guangzhou 510275GuangdongChina Institute of Frontier and Interdisciplinary Science Shandong UniversityQingdao 266237China APC UniversitéParis Cité

Theγ-ray emission from the W51 complex is widely acknowledged to be attributed to the interaction between the cosmic rays(CRs)accelerated by the shock of supernova remnant(SNR)W51C and the dense molecular clouds in the adjacent star-forming region,***,the maximum acceleration capability of W51C for CRs remains *** on observations conducted with the Large high Altitude Air Shower Observatory(LhAASO),we report a significant detection ofγrays emanating from the W51 complex,with energies from 2 to 200 *** LhAASO measurements,for the first time,extend theγ-ray emission from the W51 complex beyond 100 TeV and reveal a significant spectrum bending at tens of *** combining the"π^(0)-decay bump"featured data from Fermi-LAT,the broadbandγ-ray spectrum of the W51 region can be well-characterized by a simple pp-collision *** observed spectral bending feature suggests an exponential cutoff at~400 TeV or a power-law break at~200 TeV in the CR proton spectrum,most likely providing the first evidence of SNRs serving as CR accelerators approaching the PeV ***,two young star clusters within W51B could also be theoretically viable to produce the most energeticγrays observed by *** findings strongly support the presence of extreme CR accelerators within the W51 complex and provide new insights into the origin of Galactic CRs.

关键词： UhE c-ray Cosmic rays SNR W51C Star clusters

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故障解列与失步解列的协调优化

电力系统自动化 2009年第14期33卷 1-6,16页

作者：王达薛禹胜 q.h. WU 刘玉田张恒旭山东大学电气工程学院山东省济南市250061 国网电力科学研究院/南京南瑞集团公司江苏省南京市 210003 The University of Liverpool Liverpool L69 3GJ英国

解列控制既可由故障驱动(即第二道防线中的故障解列),也可由轨迹驱动(即第三道防线中的失步解列)。对完全确定性的理想情况,只需要考虑故障解列,以减少对系统的冲击;但客观存在的不确定因素模糊了连锁解列的充要条件,突出了失步解列及... 详细信息

解列控制既可由故障驱动(即第二道防线中的故障解列),也可由轨迹驱动(即第三道防线中的失步解列)。对完全确定性的理想情况,只需要考虑故障解列,以减少对系统的冲击;但客观存在的不确定因素模糊了连锁解列的充要条件,突出了失步解列及两者协调的重要性。将解列后使各孤立子系统稳定的最小控制代价与故障概率的乘积之和作为解列风险,并按该指标协调2种解列方案。采用"在线预算、实时匹配"的方法提高故障解列的自适应性;由控制中心站、就地主站和解列装置组成自适应失步解列系统。其中,控制中心站负责应对振荡中心的转移;就地主站按断面功率或风险代价在线判断最优的解列割集。通过仿真验证了其有效性。

关键词：故障解列失步解列风险自适应协调优化

基于MRI的自动化多任务深度学习系统评估冈上肌腱损伤

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国际医学放射学杂志 2024年第4期 499-500页

作者： M.Ni Y.q.Zhao L.h.Zhang W.Chen q.Z.Wang C.Y.Tian 常雪

摘要目的建立一个自动化、多任务、基于MRI的深度学习系统，用于精细评估冈上肌腱（SST）损伤。方法根据关节镜检查结果，将3 087例病人分为SST正常组、退变组和

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Reducing carbon emissions with Geoscience solutions:A look at the contributions of nuclear energy,technology,and green finance

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Geoscience Frontiers 2024年第4期15卷 411-426页

作者： Aifeng Liu Muhammad Imran Abdelmohsen A.Nassani Rima h.Binsaeed Khalid Zaman International Business School Shaanxi Normal UniversityXi’anChina Department of Economics The University of HaripurHaripur Khyber Pakhtunkhwa 22620Pakistan Department of Management College of Business AdministrationKing Saud UniversityP.O.Box 71115Riyadh 11587Saudi Arabia

Standards for Low-Carbon Energy Portfolios(LC-EPS)mandate that a certain percentage of a region's electricity generation originate from zero-or low-emissions *** 1995q1 through 2020q4,the study used the ARDL-Bounds testing technique to estimate coefficient parameters,Granger causality to draw causal inferences,and variance decomposition analysis to anticipate the factors that will have the greatest impact on carbon emissions in the US *** power significantly impacts carbon emissions,as seen by an inverted U-shaped environmental Kuznets curve,whereas long-term impact of innovation leads to lower *** the other hand,exports of sophisticated technology reduce carbon *** growth has a discernible effect on carbon emissions,nuclear power,innovation,and environmentally friendly ***-tech exports will likely impact carbon emissions most,followed by a demand for nuclear power,innovation,economic expansion,and sustainable finance for the next ten *** results give policymakers helpful insight into how the US economy may reduce carbon emissions and fight climate change via renewable energy and green finance.

关键词： Nuclear energy demand high technology exports Innovation Economic growth Green finance USA

ChANGES OF MEAN VELOCITY PROFILES IN ThE WAVE-CURRENT COMBINED FLOW

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Journal of hydrodynamics 2001年第1期13卷 47-53页

作者： Wu, Y.S. Lian, J.J. Zhang, q.h. qin, C.R. Dep. of hydraulic Eng. Tsinghua Univ. Beijing 100084 China

A mathematical model is developed to simulate the change in mean velocity for the coexistent case of waves and current. The experimental results of mean velocity profile in a wave-current flume show the following features: Eulerian mean current profile for following current is more uniformly distributed than the corresponding pure current case, whereas , the case of an opposing current leads to the more straight profile. This model is based on Eulerian mean framework, and motions of wave and current are solved simultaneously. The comparisons of numerical results and experimental data show that the mathematical model presented in this paper is reasonable and feasible.

关键词： Computer simulation hydrodynamics Mathematical models Sediment transport

Large Amplitude Low Frequency Waves in a Magnetized Nonuniform Electron-Positron-Ion Plasma

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Chinese Physics Letters 2004年第5期21卷 884-887页

作者： q.h.que h.Saleem Abdus-SalamInternationalCentreforTheoreticalPhysicsTrieste Italy Permanentaddresses:DepartmentofPhysics COMSATSInstituteofInformationTechnologyH-8IslamabadPakistan.

It is shown that the large amplitude low-frequency electromagnetic drift waves in electron–positron–ion plasmas might give rise to dipolar vortices. A linear dispersion relation of several coupled electrostatic and electromagnetic low-frequency modes is obtained. The relevance of this work to both laboratory and astrophysical situations is pointed out.

关键词： Positrons

STRUCTURAL DETERMINATION OF TITANIUM-OXIDE NANOPARTICLES BY X-RAY ABSORPTION SPECTROSCOPY

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Acta Metallurgica Sinica(English Letters) 2002年第1期15卷 53-57页

作者： Z.Y. Wu J. Zhang K. Ibrahim M.I. Abbas G. Li Y. Tao T.D. hu F.q. Liu h.J. qian Y.N. Xie q.h. Zhang L. Gao Z.Z. Chen Beijing Synchrotron Radiat. Facility Inst. of High Energy Phys. Chinese Acad. of Sci. Beijing 100039 China

As a potential application of titanium-oxide nanoparticles, it is extremely important to investigate a detailed picture of the surface and interior structural properties of nanocrystalline materials, such as rutile and anatase with diameters 7.0 and 4.5nm, respectively. X-ray absorption spectroscopy has been used to identify the local Ti environment and related electronic structure. We combine the experimental results at the Ti edge in both bulk and nano-crystals to determine the lattice distortion in terms of differently characteristic preedge features and the variation in the multiple-scattering region of X-ray absorption near-edge structure (XANES) spectra. The relationship between the transition peaks and the surface-to volume ratio is also discussed.

关键词： X-ray absorption near edge structure nano particle transition metal oxide

Acasta片麻杂岩多期次热事件:来自锆石、榍石和磷灰石的原位微区年代学证据

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中国科学：地球科学 2024年第3期54卷 693-707页

作者：梅清风杨进辉孙金凤李秋立吴石头凌潇潇彭澎王浩中国科学院地质与地球物理研究所岩石圈演化国家重点实验室北京100029 中国科学院大学地球与行星科学学院北京100049 中国科学院大学计算地球动力学重点实验室北京100049

本文使用激光剥蚀电感耦合等离子体质谱(LA-ICPMS)和二次离子质谱(SIMS)对Acasta片麻杂岩样品碎片(大小约1cm2)中的锆石、磷灰石和榍石进行了原位微区定年,以制约Acasta片麻杂岩的热演化历史.这些样品碎片中的锆石显示多期年龄,反映了... 详细信息

本文使用激光剥蚀电感耦合等离子体质谱(LA-ICPMS)和二次离子质谱(SIMS)对Acasta片麻杂岩样品碎片(大小约1cm2)中的锆石、磷灰石和榍石进行了原位微区定年,以制约Acasta片麻杂岩的热演化历史.这些样品碎片中的锆石显示多期年龄,反映了继承锆石的存在或者锆石结晶后的再生长过程.结合前人研究,本文锆石数据揭示, Acasta片麻杂岩经历的多期岩浆事件发生时间分别为:>3.96、约3.72和约3.57Ga.样品AY199中榍石的PbPb等时线年龄为(2911±22)Ma(95%置信水平, MSWD=1.5),与Acasta片麻杂岩记录的太古宙最后一次岩浆事件年龄一致.样品AC478和AY066中榍石U-Pb年龄分别为(1932±270)Ma(95%置信水平, MSWD=2.3)和(1813±45)Ma(95%置信水平, MSWD=2.3).样品P090803-C中磷灰石的Pb-Pb等时线年龄为(1833±26)Ma(95%置信水平,MSWD=1.4).样品AC478、AY199和AY066中磷灰石U-Pb年龄分别为(1850±20)Ma(95%置信水平, MSWD=1.3)、(1827±100)Ma(95%置信水平, MSWD=6.3)和(1807±58)Ma(95%置信水平, MSWD=3.9).样品AC478和AY066中的榍石U-Pb年龄以及本文所有样品中的磷灰石Pb-Pb或U-Pb年龄相同,均为约1.9~1.8Ga,指示Wopmay造山作用导致的矿物U-Pb体系重置,证明了Wopmay造山作用的峰期温度超过了磷灰石的U-Pb体系封闭温度,并接近或者超过榍石的U-Pb体系封闭温度.

关键词：锆石榍石磷灰石 Acasta片麻杂岩 Wopmay造山带

Improving the operational stability of perovskite solar cells with cesium-doped graphene oxide interlayer

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Journal of Energy Chemistry 2024年第9期96卷 483-490页

作者： Masaud Almalki Katerina Anagnostou Konstantinos Rogdakis Felix T.Eickemeyer Mostafa Othman Minas M.Stylianakis Dimitris Tsikritzis Anwar q.Alanazi Nikolaos Tzoganakis Lukas Pfeifer Rita Therisod Xiaoliang Mo Christian M.Wolff Aïcha hessler-Wyser Shaik M.Zakeeruddin hong Zhang Emmanuel Kymakis Michael Grätzel Laboratory of Photonics and Interfaces École Polytechnique Fédérale de Lausanne(EPFL)Lausanne 1015Switzerland Department of Electrical and Computer Engineering Hellenic Mediterranean UniversityHeraklionCrete 71410Greece Institute of Electrical and Microengineering(IEM)Photovoltaics and Thin-Film Electronics Laboratory(PV-Lab) École Polytechnique Fédérale de Lausanne(EPFL)Neuchâtel 2000Switzerland Department of Nursing Faculty of Health SciencesHellenic Mediterranean UniversityCrete 71410Greece Centre Interdisciplinaire de Microscopie Electronique École Polytechnique Fédérale de Lausanne(EPFL)Lausanne 1015Switzerland Future Energy Technology Institute King Abdulaziz City for Science and Technology(KACST)P.O.Box 6086Riyadh 11442Saudi Arabia State Key Laboratory of Photovoltaic Science and Technology Shanghai Frontiers Science Research Base of Intelligent Optoelectronics and PerceptionInstitute of OptoelectronicsDepartment of Materials ScienceFudan UniversityShanghai 200433China

Perovskite solar cells(PSCs)have made great advances in terms of power conversion efficiency(PCE),yet their subpar stability continues to hinder their *** interface between the perovskite layer and the charge-carrier transporting layers plays a crucial role in undermining the stability of *** this work,we propose a strategy to stabilize high-performance PSCs with PCE over 23%by introducing a cesium-doped graphene oxide(GO-Cs)as an interlayer between the perovskite and hole-transporting *** GO-Cs treated PSCs exhibit excellent operational stability with a projected T80(the time where the device PCE reduces to 80%of its initial value)of 2143 h of operation at the maximum powering point under one sun illumination.

关键词： Perovskite solar cells Doped graphene oxide Graphene related material Long-term operational stability