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In-situ construction of grass-like hy.rid architecture responsible for extraordinary.corrosion performance: Experimental and theoretical approach

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Nano Materials Science 2024年第1期6卷 44-59页

作者： t.Suhartono F.Hazmatulhaq y.Sheng A.Chaouiki M.P.Kamil y.G.Ko Materials Electrochemistry.Group School of Materials Science and EngineeringYeungnam UniversityGyeongsan38541Republic of Korea Research Center for Advanced Materials National Research and Innovation Agency(BRIN)South TangerangBanten15314Indonesia

Despite the engineering potential by.the co-existence of inorganic and organic substances to protect vulnerable metallic materials from corrosive environments,both their interaction and in-situ formation mechanism to induce the nature-inspired composite remained less *** present work used three distinctive mercaptobenzazole(MB)compounds working as corrosion inhibitors,such as 2-mercaptobenzoxazole(MBO),2-mercaptobenzothiazole(MBt),and 2-mercaptobenzimidazole(MBI)in a bid to understand how the geometrical structure arising from O,S,and N atoms affected the interaction toward inorganic *** compounds that were used here to control the corrosion kinetics would be interacted readily.with the pre-existing MgO lay.r fabricated by.plasma *** phenomenon triggered the nucleation of the root network since MB compounds were seen to be adsorbed actively.on the defective surface through the active sites in MB ***,the molecule with twin donor atoms adjacent to the mercapto-sites affected the facile growth of the grass-like structures with‘uniform’distribution via molecular self-assembly.which showed better corrosion performance than those with having dissimilar donor atoms with the inhibition efficiency.η)of 97%*** formation mechanism underly.ng nucleation and growth behavior of MB molecule was discussed concerning the theoretical calculation of density.functional theory.

关键词： Nature-inspired composite Organic-inorganic interaction Corrosion inhibitor Density.functional theory Electrochemistry

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Higher-order mode analy.is for SOLEIL-ty.e superconducting cavity

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中国科学技术大学学报 2024年第7期54卷 0706-1-0706-11页

作者： Chai X. Li Q. Xu y. tang y. tan M. Wu C.-F. National Sy.chrotron Radiation Laboratory University of Science and Technology of China Hefei 230029 China

A 499.8 MHz SOLEIL-ty.e superconducting cavity.was simulated and designed for the first time in this paper. the higher-order mode (HOM) properties of the cavity.were investigated. two kinds of coaxial HOM couplers were designed. Using 4 L-ty.e and 4 t-ty.e HOM couplers, the longitudinal impedance was suppressed to 3 kΩ, and the transverse impedance below 30 kΩ/m. the HOM damping requirements of Hefei Advanced Light Facility.(HALF) were satisfied. this paper conducts an in-depth study.on the radio frequency.(RF) design, multipacting optimization, and thermal analy.is of these coaxial couplers. Simulation results indicated that under operating acceleration voltage, the optimized couplers does not exhibit multiplicating or thermal breakdown phenomena. the cavity.has the potential to reach a higher acceleration gradient.

关键词：高次模耦合器超导腔高频系统二次电子倍增热仿真

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Search for production of dark fermion candidates in association with heavy.neutral gauge boson decay.ng to dimuon in proton-proton collisions at√s=8 teV using CMS open data

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Chinese Phy.ics C 2024年第4期48卷 6-13页

作者： y.Mahmoud H.Abdallah M.t.Hussein S.Elgammal Centre for theoretical phy.ics The British University in EgyptEgypt Phy.ics Department Faculty of ScienceCairo UniversityEgypt

In this study.we conducted a search for dark matter using a part of the data recorded by.the CMS experiment during run-I of the LHC in 2012 with a center of mass energy.of 8 teV and an integrated luminosity.of 11.6 fb−*** data were gathered from the CMS open *** matter,in the framework of the simplified model(mono-Z′),can be produced from proton-proton collisions in association with a new hy.othetical gauge boson,Z′.thus,the search was conducted in the dimuon plus large missing transverse momentum *** benchmark scenario of mono-Z′,which is known as light vector,was used for interpreting the CMS open *** evidence of dark matter was observed,and exclusion limits were set on the masses of dark matter and Z′at 95%confidence level.

关键词： dark matter large hadron collider CMS open data search for new phy.ics dark fermion

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An MPI parallel DEM-IMB-LBM framework for simulating fluid-solid interaction problems

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Journal of Rock Mechanics and Geotechnical Engineering 2024年第6期16卷 2219-2231页

作者： Ming Xia Liuhong Deng Fengqiang Gong tongming Qu y.t.Feng Jin y. Hunan Key.Laboratory.of Geomechanics and Engineering Safety Xiangtan UniversityXiangtan411105China School of Civil Engineering Southeast UniversityNanjing211189China Department of Civil and Environmental Engineering Hong Kong University of Science and TechnologyHong KongChina Zienkiewicz Centre for Computational Engineering Swansea UniversitySwanseaSA18ENUK Fujian Research Center for tunneling and Urban Underground Space Engineering Huaqiao UniversityXiamen361021China

the high-resolution DEM-IMB-LBM model can accurately.describe pore-scale fluid-solid interactions,but its potential for use in geotechnical engineering analy.is has not been fully.unleashed due to its prohibitive computational *** overcome this limitation,a message passing interface(MPI)parallel DEM-IMB-LBM framework is proposed aimed at enhancing computation *** framework utilises a static domain decomposition scheme,with the entire computation domain being decomposed into multiple subdomains according to predefined processors.A detailed parallel strategy.is employ.d for both contact detection and hy.rody.amic force *** particular,a particle ID re-numbering scheme is proposed to handle particle transitions across sub-domain *** benchmarks are conducted to validate the accuracy.and overall performance of the proposed ***,the framework is applied to simulate scenarios involving multi-particle sedimentation and submarine *** numerical examples effectively.demonstrate the robustness and applicability.of the MPI parallel DEM-IMB-LBM framework.

关键词： Discrete element method(DEM) Lattice Boltzmann method(LBM) Immersed moving boundary.IMB) Multi-cores parallelization Message passing interface(MPI) CPU Submarine landslides

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HI in High Gas-phase Metallicity.Dwarf Galaxy.WISEA J230615.06+143927.9

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Research in Astronomy.and Astrophy.ics 2024年第1期24卷 292-299页

作者： y.n Guo C.Sengupta t.C.Scott P.Lagos y.Luo Purple Mountain Observatory Chinese Academy of SciencesNanjing 210023China School of Astronomy.and Space Sciences University of Science and Technology of ChinaHefei 230026China Institute of Astrophy.ics and Space Sciences(IA Porto) Rua das Estrelas4150-762PortoPortugal

We present resolved Giant Metrewave Radio telescope H I observations of the high gas-phase metallicity.dwarf galaxy.WISEA J230615.06+143927.9(z = 0.005)(hereafter J2306) and investigate whether it could be a tidal Dwarf Galaxy.tDG) candidate. tDGs are observed to have higher metallicities than normal dwarfs. J2306 has an unusual combination of a blue g-r color of 0.23 mag, irregular optical morphology.and high-metallicity.12 +log(O/H) = 8.68 ± 0.14), making it an interesting galaxy.to study.in more detail. We find J2306 to be an H I rich galaxy.with a large extended, unperturbed rotating H I disk. Using our H I data we estimated its dy.amical mass and found the galaxy.to be dark matter(DM) dominated within its H I radius. the quantity.of DM, inferred from its dy.amical mass, appears to rule out J2306 as an evolved tDG. A wide area environment search reveals J2306 to be isolated from any.larger galaxies which could have been the source of its high gas metallicity. Additionally. the H I morphology.and kinematics of the galaxy.show no indication of a recent merger to explain the *** detailed optical spectroscopic observations of J2306 might provide an answer to how a seemingly.ordinary.irregular dwarf galaxy.achieved such a high level of metal enrichment.

关键词： galaxies:abundances galaxies:dwarf galaxies:irregular radio lines:galaxies radio lines:ISM

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Editorial for Multiscale&Multifield Coupling in Geomechanics

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Journal of Rock Mechanics and Geotechnical Engineering 2024年第6期16卷 1919-1921页

作者： Min Wang Pengzhi Pan Andrew H.C.Chan y.t.Feng t-3 Fluid Dy.amics and Solid Mechanics Theoretical DivisionLos Alamos National LaboratoryNew MexicoUSA Institute of Rock and Soil Mechanics Chinese Academy of SciencesWuhanChina School of Engineering University of TasmaniaTasmaniaAustralia College of Engineering Swansea UniversityWalesUK

We are delighted to serve as guest editors for this special issue in the Journal of Rock Mechanics and Geotechnical *** purpose of this special issue is dedicated to gathering the latest research work on Multiscale&Multifield Coupling in Geomechanics,where we delve into the intricate interplay.of various fields and scales that govern the behavior of *** total,30 manuscripts from USA,China,UK,Germany.Canada,India and United Arab Emirates are selected to be included in this issue.

关键词： materials. gathering mechanics

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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： Cao, Zhen Aharonian, F. Axikegu Bai, y.X. Bao, y.W. Bastieri, D. Bi, X.J. Bi, y.J. Bian, W. Bukevich, A.V. Cao, Q. Cao, W.y. Cao, Zhe Chang, J. Chang, J.F. Chen, 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. Cheng, N. Cheng, y.D. Cui, M.y. Cui, S.W. Cui, X.H. Cui, y.D. Dai, B.Z. Dai, H.L. Dai, Z.G. Danzengluobu Dong, X.Q. Duan, K.K. Fan, J.H. Fan, y.Z. Fang, J. Fang, J.H. Fang, K. Feng, C.F. Feng, H. Feng, L. Feng, S.H. Feng, X.t. Feng, y. Feng, y.L. Gabici, S. Gao, B. Gao, C.D. Gao, Q. Gao, W. Gao, W.K. Ge, M.M. Geng, L.S. Giacinti, G. Gong, G.H. Gou, Q.B. Gu, M.H. Guo, F.L. Guo, X.L. Guo, y.Q. Guo, y.y. Han, y.A. Hasan, M. He, H.H. He, H.N. He, J.y. He, y. Hor, y.K. Hou, B.W. Hou, C. Hou, X. Hu, H.B. Hu, Q. Hu, S.C. Huang, D.H. Huang, t.Q. Huang, W.J. Huang, X.t. Huang, X.y. Huang, y. Ji, X.L. Jia, H.y. Jia, K. Jiang, K. Jiang, X.W. Jiang, Z.J. Jin, M. Kang, M.M. Karpikov, I. Kuleshov, D. Kurinov, K. Li, 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, X.R. Li, Xin Li, y.Z. Li, Zhe Li, Zhuo Liang, E.W. Liang, y.F. Lin, S.J. Liu, 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. Luo, Q. Luo, y. Lv, H.K. Ma, B.Q. Ma, L.L. Ma, X.H. Mao, J.R. Min, Z. Mitthumsiri, W. Mu, H.J. Nan, y.C. Neronov, A. Ou, L.J. Pattarakijwanich, P. Pei, Z.y. Qi, J.C. Qi, M.y. Qiao, B.Q. Qin, J.J. Raza, A. Ruffolo, D. Sáiz, A. Saeed, M. Semikoz, D. Shao, L. Shchegolev, O. Sheng, X.D. Shu, F.W. Song, H.C. Stenkin, y..V. Stepanov, V. Su, y. Sun, D.X. Sun, Q.N. Sun, X.N. Sun, Z.B. takata, J. tam, P.H.t. Key.Laboratory.of Particle Astrophy.ics & Experimental Phy.ics Division & Computing Center Institute of High Energy Physics Chinese Academy of Sciences Beijing 100049 China University.of Chinese Academy.of Sciences Beijing 100049 China tIANFU Cosmic Ray.Research Center Chengdu China Dublin Institute for Advanced Studies 31 Fitzwilliam Place 2 Dublin Ireland Max-Planck-Institut for Nuclear Phy.ics P.O. Box 103980 Heidelberg 69029 Germany School of Phy.ical Science and technology.& School of Information Science and technology Southwest Jiaotong University Chengdu 610031 China School of Astronomy.and Space Science Nanjing University Nanjing 210023 China Center for Astrophy.ics Guangzhou University Guangzhou 510006 China tsung-Dao Lee Institute & School of Phy.ics and Astronomy Shanghai Jiao Tong University Shanghai 200240 China Institute for Nuclear Research of Russian Academy.of Sciences Moscow 117312 Russia Hebei Normal University Shijiazhuang 050024 China University.of Science and technology.of China Hefei 230026 China State Key.Laboratory.of Particle Detection and Electronics China Key.Laboratory.of Dark Matter and Space Astronomy.& Key.Laboratory.of Radio Astronomy Purple Mountain Observatory Chinese Academy of Sciences Nanjing 210023 China Research Center for Astronomical Computing Zhejiang Laboratory Hangzhou 311121 China Key.Laboratory.for Research in Galaxies and Cosmology Shanghai Astronomical Observatory Chinese Academy of Sciences Shanghai 200030 China School of Phy.ics and Astronomy Yunnan University Kunming 650091 China Key.Laboratory.of Cosmic Ray. (tibet University. Ministry of Education Lhasa 850000 China National Astronomical Observatories Chinese Academy of Sciences Beijing 100101 China School of Phy.ics and Astronomy.(Zhuhai) & School of Phy.ics (Guangzhou) & Sino-French Institute of Nuclear Engineering and technology.(Zhuhai) Sun Yat-sen University Zhuhai 519000 & Guangzhou 510275 Guangdong China Institute of Frontier and

the γ-ray.emission from the W51 complex is widely.acknowledged to be attributed to the interaction between the cosmic ray. (CRs) accelerated by.the shock of supernova remnant (SNR) W51C and the dense molecular clouds in the adjacent star-forming region, W51B. However, the maximum acceleration capability.of W51C for CRs remains elusive. Based on observations conducted with the Large High Altitude Air Shower Observatory.(LHAASO), we report a significant detection of γ ray. emanating from the W51 complex, with energies from 2 to 200 teV. the LHAASO measurements, for the first time, extend the γ-ray.emission from the W51 complex bey.nd 100 teV and reveal a significant spectrum bending at tens of teV. By.combining the "π0-decay.bump" featured data from Fermi-LAt, the broadband γ-ray.spectrum of the W51 region can be well-characterized by.a simple pp-collision model. the 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 regime. Additionally. two y.ung star clusters within W51B could also be theoretically.viable to produce the most energetic γ ray. observed by.LHAASO. Our findings strongly.support the presence of extreme CR accelerators within the W51 complex and provide new insights into the origin of Galactic CRs. © 2024 Science China Press

关键词： Cosmic ray.

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In situ tEM investigation of electron irradiation and aging-induced high-density.nanoprecipitates in an Mg-10Gd-3y.1Zn-0.5Zr alloy

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Journal of Magnesium and Alloy. 2024年第5期12卷 1841-1853页

作者： M.Lv H.L.Ge Q.Q.Jin X.H.Shao y.t.Zhou B.Zhang X.L.Ma Sheny.ng National Laboratory.for Materials Science Institute of Metal ResearchChinese Academy of Sciences72 Wenhua RoadShenyang 110016China School of Materials Science and Engineering University of Science and Technology of ChinaShenyang 110016China Materials Science and Engineering Research Center Guangxi University of Science and TechnologyLiuzhou 545006China

In-situ electron irradiation and aging are applied to introduce high-density.precipitates in an Mg-10Gd-3y.1Zn-0.5Zr(GWZ1031K,wt.%)alloy.to improve the *** results show that the hardness of the Mg alloy.after irradiation for 10 h and aging for 9 h at 250℃ is 1.64 GPa,which is approximately.64% higher than that of the samples before being *** is mainly.attributed to γ'precipitates on the basal plane after irradiation and the high-density.nanoscale β'precipitates on the prismatic plane after aging,which should be closely.related to the irradiation-induced homogenous *** latter play. a key.role in precipitation *** result paves a way.to improve the mechanical properties of metallic materials by.tailoring the precipitation through irradiation and aging.

关键词： Mg alloy Electron beam irradiation Hardening Precipitates In-situ tEM

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Increasing poly.er scission rate by.ty.ng an overhand knot

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Science China Chemistry 2024年

作者： y.heng Hu Jennifer t.Ou Jim y.Huang y.anning Feng Department of Chemistry.and Biochemistry The University of Oklahoma

Similar to the phenomenon of knotted ropes in life, knotted climbing ropes will reduce their strength due to knots. Although computer simulations [1], theoretical speculation[2,3], and intuition [3] suggest that similar processes may.occur at the nanoscale, this hy.othesis has not been experimentally.proven before. With the increasing maturity.of molecular recognition and self-assembly. a research communication by.Leigh et al. [4]

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基于极限分析上限法的地震作用下分层地基盾构隧道开挖面稳定性研究

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岩土力学 2024年第4期45卷 1201-1213页

作者：张治国罗杰朱正国 PAN y.t 孙苗苗上海理工大学环境与建筑学院上海200093 石家庄铁道大学省部共建交通工程结构力学行为与系统安全国家重点实验室河北石家庄050043 新加坡国立大学土木与环境工程系新加坡119077 浙大城市学院土木工程系浙江杭州310015 浙大城市学院城市基础设施智能化浙江省工程研究中心浙江杭州310015

目前针对盾构隧道开挖面稳定性的研究还较少考虑土体分层特性和地震作用的耦合影响,因此构建了一种在分层土体中考虑地震作用的开挖面三维对数螺旋破坏模型进行研究。首先,将地震引起的动态响应通过拟静力法简化为水平和竖直两个方向上... 详细信息

目前针对盾构隧道开挖面稳定性的研究还较少考虑土体分层特性和地震作用的耦合影响,因此构建了一种在分层土体中考虑地震作用的开挖面三维对数螺旋破坏模型进行研究。首先,将地震引起的动态响应通过拟静力法简化为水平和竖直两个方向上的惯性力作用;其次,在均质土体中的三维对数螺旋破坏机制的基础上,将其改进为适用于分层土体的三维对数螺旋破坏机制;再次,根据上限定理,在虚功率方程中引入地震惯性力所做功率,得到考虑土体分层特性和地震作用条件下的盾构隧道开挖面支护力的上限解;最后,将上限理论解与三维数值模拟结果和既有模型试验结果进行对比,得到了较好的一致性。此外,针对水平地震加速度系数和地层厚度对关键物理特征进行了影响因素分析。结果表明,当比例系数ζ>0时,极限支护力随水平地震加速度系数的增大显著增大;当ζ<0时,极限支护力随水平地震加速度系数增大而增大的趋势减弱。当水平地震加速度系数kh=0时,即在无地震作用情况下,归一化极限支护力不随ζ的变化而变化;在上硬下软土层中,下部土层厚度比的增大会引起极限支护力的增大,在上软下硬土层中,下部土层厚度比的增大会引起极限支护力的减小。

关键词：盾构隧道开挖面稳定性地震作用分层土体上限定理

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