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Spark plasma sintering of tungsten-based WTaVCr refractory high entropy alloys for nuclear fusion applications

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International Journal of Minerals,Metallurgy and Materials 2024年第1期31卷 146-154页

作者： Yongchul Yoo Xiang Zhang Fei Wang Xin Chen Xing-Zhong Li Michael nastasi Bai Cui Department of Mechanical&Materials Engineering University of Nebraska-LincolnLincolnNE 68588USA Nebraska Center for Materials and Nanoscience University of Nebraska-LincolnLincolnNE 68588USA Department of Nuclear Engineering Texas A&M UniversityCollege StationTX 77843USA

W-based WTaVCr refractory high entropy alloys (RHEA) may be novel and promising candidate materials for plasma facing components in the first wall and diverter in fusion reactors. This alloy has been developed by a powder metallurgy process combining mechanical alloying and spark plasma sintering (SPS). The SPSed samples contained two phases, in which the matrix is RHEA with a body-centered cubic structure, while the oxide phase was most likely Ta2VO6through a combined analysis of X-ray diffraction (XRD),energy-dispersive spectroscopy (EDS), and selected area electron diffraction (SAED). The higher oxygen affinity of Ta and V may explain the preferential formation of their oxide phases based on thermodynamic calculations. Electron backscatter diffraction (EBSD) revealed an average grain size of 6.2μm. WTaVCr RHEA showed a peak compressive strength of 2997 MPa at room temperature and much higher micro-and nano-hardness than W and other W-based RHEAs in the literature. Their high Rockwell hardness can be retained to at least 1000°C.

关键词： refractory high entropy alloy plasma-facing material fusion reactor spark plasma sintering

Simulation of Bipolar Charge Transport in Graphene by Using a Discontinuous Galerkin Method

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Communications in Computational Physics 2019年第6期26卷 114-134页

作者： Armando Majorana Giovanni nastasi Vittorio Romano Department of Mathematics and Computer Science Universita degli Studi di Cataniaviale Andrea Doria 695125 CataniaItaly

Charge transport in suspended monolayer graphene is simulated by a numerical deterministic approach,based on a discontinuous Galerkin(DG)method,for solving the semiclassical Boltzmann equation for *** the conduction and valence bands are included and the interband scatterings are taken into *** use of a Direct Simulation Monte Carlo(DSMC)approach,which properly describes the interband scatterings,is computationally very expensive because the va-lence band is very populated and a huge number of particles is *** the choice of simulating holes instead of electrons does not overcome the problem because there is a certain degree of ambiguity in the generation and recombination terms of electron-hole ***,direct solutions of the Boltzmann equations with a DSMC neglect the interband scatterings on the basis of physical *** DG approach does not suffer from the previous drawbacks and requires a reasonable computing *** the present paper the importance of the interband scatterings is accurately evaluated for several values of the Fermi energy,addressing the issue related to the validity of neglecting the generation-recombination *** is found out that the inclusion of the interband scatterings produces huge variations in the average values,as the current,with zero Fermi energy while,as expected,the effect of the interband scattering becomes negligible by increasing the absolute value of the Fermi energy.

关键词： Graphene bipolar charge transport discontinuous Galerkin method

Direct Simulation of Charge Transport in Graphene Nanoribbons

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Communications in Computational Physics 2022年第2期31卷 449-494页

作者： Giovanni nastasi V.Dario Camiola Vittorio Romano Universita degli Studi di Catania Dipartimento di Matematica e InformaticaViale Andrea Doria 695125 CataniaItaly

Graphene nanoribbons are considered as one of the most promising ways to design electron devices where the active area is made of *** fact,graphene nanoribbons present a gap between the valence and the conduction bands as in standard semiconductors such as Si or GaAs,at variancewith large area graphenewhich is gapless,a feature that hampers a good performance of graphene field effect *** use graphene nanoribbons as a semiconductor,an accurate analysis of their electron properties is ***,electron transport in graphene nanoribbons is investigated by solving the semiclassical Boltzmann equation with a discontinuous Galerkin *** the electron-phonon scattering mechanisms are *** adopted energy band structure is that devised in[1]while according to[2]the edge effects are described as an additional scattering stemming from the Berry-Mondragon model which is valid in presence of edge *** this approach a spacial 1D transport problem has been solved,even if it remains two dimensional in the wavevector space.A degradation of charge velocities,and consequently of the mobilities,is found by reducing the nanoribbon width due mainly to the edge scattering.

关键词： Graphene nanoribbons bipolar charge transport discontinuous Galerkin method

采用发射光谱/脉冲分辨联用技术测定夹杂物粒度分布

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冶金分析 2013年第3期33卷 9-13页

作者： nastasi G WESTER R COLLA V NOLL R Scuola Superiore Sant'Anna-TeCIP Institute Pisa 56124Italy Fraunhofer-Institut für Lasertechnik Aachen 52074Germany

通过解析发射光谱和脉冲分辨分析联用技术(OES/PDA)数据确定钢铁中夹杂物的类型及计算其粒度分布需要借助于高等数学方法,以便在大量的数据中滤出那些与夹杂物相关的OES/PDA数据,从而找到可靠的该数据集的离群数据。强度及大多的质量分... 详细信息

通过解析发射光谱和脉冲分辨分析联用技术(OES/PDA)数据确定钢铁中夹杂物的类型及计算其粒度分布需要借助于高等数学方法,以便在大量的数据中滤出那些与夹杂物相关的OES/PDA数据,从而找到可靠的该数据集的离群数据。强度及大多的质量分布其分布函数都是非正态分布的,因此,通过对这些数据进行拟合即可得到非属于该正态分布的离群数据。离群数据确定后,通过这些信息可找到与一些特定夹杂物类型相关联的数据群。基于此目的,发现一种称为"自组织特征映射(SOM)"的数学方法非常适于进行此项研究。根据离群数据及夹杂物类型的相关信息,采用该方法可以计算出质量分布并能进一步进行不同夹杂物类型的粒度分布计算。

关键词：钢脉冲分辨技术夹杂数据处理

离子注入氧化锌纳米晶体光致发光特性(英文)

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纳米技术与精密工程 2012年第5期10卷 379-383页

作者： HARRIMAN T A HILDEBRAND D S LUCCA D A LEEJ-K WANG Y Q nastasi M 美国俄克拉荷马州立大学机械与航空航天工程学院 stillwaterok74078 美国匹兹堡大学机械工程与材料科学系 pittsburghpa15261 美国洛斯阿拉莫斯国家实验室材料科学与技术室 losalamosnm87545 美国内布拉斯加大学林肯分校内布拉斯加能源科学研究中心 lincolnne68583

为进一步了解离子注入过程对纳米晶体发光响应的损伤效果,研究了注入氢离子和氦离子对氧化锌纳米晶体光致发光(PL)特性的影响.首先在二氧化硅衬底上制备了直径为4 nm和9 nm的氧化锌纳米晶体薄膜,接着在室温下向生成的薄膜中注入氢离子... 详细信息

为进一步了解离子注入过程对纳米晶体发光响应的损伤效果,研究了注入氢离子和氦离子对氧化锌纳米晶体光致发光(PL)特性的影响.首先在二氧化硅衬底上制备了直径为4 nm和9 nm的氧化锌纳米晶体薄膜,接着在室温下向生成的薄膜中注入氢离子和氦离子,并研究其PL响应变化.结果表明,与未注入离子的纳米晶体相比,注入氦离子导致缺陷PL发光增加,而当注入氢离子之后,缺陷发光大幅降低,表明氢原子对注入损伤有钝化作用.比较近谱带边沿(NBE)与缺陷发光之比发现,较大颗粒的纳米晶体其近谱带边沿与缺陷发光比在注入氢离子后增大,而在注入氦离子后降低.该规律同样适用于较小颗粒的纳米晶体,但其近谱带边沿与缺陷发光比在注入氢离子之后的增幅比大颗粒晶体的小得多.

关键词：氧化锌离子注入缺陷光致发光

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写给喵星人的诗

英语学习 2015年第7期 51-53页

作者： Alison nastasi 柒月

美国诗人T．S．艾略特对猫咪有着深沉的爱，这种爱在他1939年的幽默诗集《老负鼠的猫经》中便有所体现。当然，爱猫的作家可不止他一个。法国诗人波德莱尔、美国诗人狄金森、爱尔兰诗人叶芝等等，对猫咪都有着各自的情怀。本文精心挑选... 详细信息

美国诗人T．S．艾略特对猫咪有着深沉的爱，这种爱在他1939年的幽默诗集《老负鼠的猫经》中便有所体现。当然，爱猫的作家可不止他一个。法国诗人波德莱尔、美国诗人狄金森、爱尔兰诗人叶芝等等，对猫咪都有着各自的情怀。本文精心挑选了八首小诗。

关键词：诗人 T.S.艾略特 1939年波德莱尔狄金森爱尔兰美国诗集

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别让我走

疯狂英语（初中天地） 2010年第10期 13-13页

作者： Alison nastasi 芥子

《别让我走）讲述了三个在寄宿学校一起长大的伙伴过着与世膈绝的生活。直到有一天，他们发现白己原来是克隆人，而存在的唯一目的就是为别人提供移植器官。听起来是否似曾相识？没错，这剧情跟2005年的《逃出克隆岛》（The Island）如... 详细信息

《别让我走）讲述了三个在寄宿学校一起长大的伙伴过着与世膈绝的生活。直到有一天，他们发现白己原来是克隆人，而存在的唯一目的就是为别人提供移植器官。听起来是否似曾相识？没错，这剧情跟2005年的《逃出克隆岛》（The Island）如出一辙，所以很多人把它称为后者的文艺版。从预告片可以看出，这部改编自石黑一雄同名小说的电影绝对不是卖弄特技的科幻片，而是一部刻画人性的细腻之作。本片清一色的英国演员阵容——凯瑞·穆里根、凯拉·奈特莉和安德鲁·加菲尔德（他可是新一任蜘蛛侠哦）也足够吸引眼球。

关键词：寄宿学校石黑一雄演员阵容加菲尔德克隆人科幻片安德鲁

Sub-percent precision measurement of neutrino oscillation parameters with JUNO

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Chinese Physics C 2022年第12期46卷 28-49页

作者： Angel Abusleme Thomas Adam Shakeel Ahmad Rizwan Ahmed Sebastiano Aiello Muhammad Akram Abid Aleem Fengpeng An Qi An Giuseppe Andronico Nikolay Anfimov Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde Marcondes de André Didier Auguste Weidong Bai Nikita Balashov Wander Baldini Andrea Barresi Davide Basilico Eric Baussan Marco Bellato Antonio Bergnoli Thilo Birkenfeld Sylvie Blin David Blum Simon Blyth Anastasia Bolshakova Mathieu Bongrand Clément Bordereau Dominique Breton Augusto Brigatti Riccardo Brugnera Riccardo Bruno Antonio Budano Jose Busto Ilya Butorov Anatael Cabrera Barbara Caccianiga Hao Cai Xiao Cai Yanke Cai Zhiyan Cai Riccardo Callegari Antonio Cammi Agustin Campeny Chuanya Cao Guofu Cao Jun Cao Rossella Caruso Cédric Cerna Chi Chan Jinfan Chang Yun Chang Guoming Chen Pingping Chen Po-An Chen Shaomin Chen Xurong Chen Yixue Chen Yu Chen Zhiyuan Chen Zikang Chen Jie Cheng Yaping Cheng Yu Chin Cheng Alexey Chetverikov Davide Chiesa Pietro Chimenti Artem Chukanov Gérard Claverie Catia Clementi Barbara Clerbaux Selma Conforti Di Lorenzo Daniele Corti Flavio Dal Corso Olivia Dalager Christophe De La Taille Zhi Deng Ziyan Deng Wilfried Depnering Marco Diaz Xuefeng Ding Yayun Ding Bayu Dirgantara Sergey Dmitrievsky Tadeas Dohnal Dmitry Dolzhikov Georgy Donchenko Jianmeng Dong Evgeny Doroshkevich Marcos Dracos Frédéric Druillole Ran Du Shuxian Du Stefano Dusini Martin Dvorak Timo Enqvist Heike Enzmann Andrea Fabbri Donghua Fan Lei Fan Jian Fang Wenxing Fang Marco Fargetta Dmitry Fedoseev Zhengyong Fei Li-Cheng Feng Qichun Feng Richard Ford Amélie Fournier Haonan Gan Feng Gao Alberto Garfagnini Arsenii Gavrikov Marco Giammarchi Nunzio Giudice Maxim Gonchar Guanghua Gong Hui Gong Yuri Gornushkin Alexandre Göttel Marco Grassi Vasily Gromov Minghao Gu Xiaofei Gu Yu Gu Mengyun Guan Yuduo Guan Nunzio Guardone Cong Guo Jingyuan Guo Wanlei Guo Xinheng Guo Yuhang Guo Paul Hackspacher Caren Hagner Ran Han Yang Han Miao He Wei He Tobias Heinz Patrick Hellmuth Yuekun Heng Rafael Herrera YuenKeung Ho Yerevan Physics Institute YerevanArmenia UniversiéLibre de Bruxelles BrusselsBelgium Universidade Estadual de Londrina LondrinaBrazil Pontificia Universidade Catolica do Rio de Janeiro Rio de JaneiroBrazil Pontificia Universidad Católica de Chile SantiagoChile Universidad Tecnica Federico Santa Maria ValparaisoChile Beijing Institute of Spacecraft Environment Engineering BeijingChina Beijing Normal University BeijingChina China Institute of Atomic Energy BeijingChina Institute of High Energy Physics BeijingChina North China Electric Power University BeijingChina School of Physics Peking UniversityBeijingChina Tsinghua University BeijingChina University of Chinese Academy of Sciences BeijingChina Jilin University ChangchunChina College of Electronic Science and Engineering National University of Defense TechnologyChangshaChina Chongqing University ChongqingChina Dongguan University of Technology DongguanChina Jinan University GuangzhouChina Sun Yat-Sen University GuangzhouChina Harbin Institute of Technology HarbinChina University of Science and Technology of China HefeiChina The Radiochemistry and Nuclear Chemistry Group in University of South China HengyangChina Wuyi University JiangmenChina Shandong University JinanChinaand Key Laboratory of Particle Physics and Particle Irradiation of Ministry of EducationShandong UniversityQingdaoChina Institute of Modern Physics Chinese Academy of SciencesLanzhouChina Nanjing University NanjingChina Guangxi University NanningChina East China University of Science and Technology ShanghaiChina School of Physics and Astronomy Shanghai Jiao Tong UniversityShanghaiChina Tsung-Dao Lee Institute Shanghai Jiao Tong UniversityShanghaiChina Institute of Hydrogeology and Environmental Geology Chinese Academy of Geological SciencesShijiazhuangChina Nankai University TianjinChina Wuhan University WuhanChina Xi'an Jiaotong University Xi'anChina Xiamen University XiamenChina School of Physics and Microelectronics Zhengzhou UniversityZhengzhou

JUNO is a multi-purpose neutrino observatory under construction in the south of *** publication presents new sensitivity estimates for the measurement of the △m_(31)^(2),△m_(21)^(2),sin^(2)θ_(12),and sin^(2)θ_(13) oscillation parameters using reactor antineutrinos,which is one of the primary physics goals of the *** sensitivities are obtained using the best knowledge available to date on the location and overburden of the experimental site,the nuclear reactors in the surrounding area and beyond,the detector response uncertainties,and the reactor antineutrino spectral shape constraints expected from the TAO satellite *** is found that the △m_(21)^(2) and sin^(2)θ_(12) oscillation parameters will be determined to 0.5%precision or better in six years of data *** the same period,the △m_(31)^(2) parameter will be determined to about 0.2%precision for each mass ordering *** new precision represents approximately an order of magnitude improvement over existing constraints for these three parameters.

关键词： neutrino oscillation reactor antineutrino precision measurement JUNO

Feasibility and physics potential of detecting ^(8)B solar neutrinos at JUNO

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Chinese Physics C 2021年第2期45卷 93-110页

作者： Angel Abusleme Thomas Adam Shakeel Ahmad Sebastiano Aiello Muhammad Akram Nawab Ali Fengpeng An Guangpeng An Qi An Giuseppe Andronico Nikolay Anfimov Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde Marcondes de André Didier Auguste Andrej Babic Wander Baldini Andrea Barresi Eric Baussan Marco Bellato Antonio Bergnoli Enrico Bernieri David Biare Thilo Birkenfeld Sylvie Blin David Blum Simon Blyth Anastasia Bolshakova Mathieu Bongrand Clément Bordereau Dominique Breton Augusto Brigatti Riccardo Brugnera Riccardo Bruno Antonio Budano Max Buesken Mario Buscemi Jose Busto Ilya Butorov Anatael Cabrera Hao Cai Xiao Cai Yanke Cai Zhiyan Cai Antonio Cammi Agustin Campeny Chuanya Cao Guofu Cao Jun Cao Rossella Caruso Cédric Cerna Jinfan Chang Yun Chang Pingping Chen Po-An Chen Shaomin Chen Shenjian Chen Xurong Chen Yi-Wen Chen Yixue Chen Yu Chen Zhang Chen Jie Cheng Yaping Cheng Alexander Chepurnov Davide Chiesa Pietro Chimenti Artem Chukanov Anna Chuvashova Gérard Claverie Catia Clementi Barbara Clerbaux Selma Conforti Di Lorenzo Daniele Corti Salvatore Costa Flavio Dal Corso Christophe De La Taille Jiawei Deng Zhi Deng Ziyan Deng Wilfried Depnering Marco Diaz Xuefeng Ding Yayun Ding Bayu Dirgantara Sergey Dmitrievsky Tadeas Dohnal Georgy Donchenko Jianmeng Dong Damien Dornic Evgeny Doroshkevich Marcos Dracos Frédéric Druillole Shuxian Du Stefano Dusini Martin Dvorak Timo Enqvist Heike Enzmann Andrea Fabbri Lukas Fajt Donghua Fan Lei Fan Can Fang Jian Fang Marco Fargetta Anna Fatkina Dmitry Fedoseev Vladko Fekete Li-Cheng Feng Qichun Feng Richard Ford Andrey Formozov Amélie Fournier Haonan Gan Feng Gao Alberto Garfagnini Alexandre Göttel Christoph Genster Marco Giammarchi Agnese Giaz Nunzio Giudice Franco Giuliani Maxim Gonchar Guanghua Gong Hui Gong Oleg Gorchakov Yuri Gornushkin Marco Grassi Christian Grewing Maxim Gromov Vasily Gromov Minghao Gu Xiaofei Gu Yu Gu Mengyun Guan Nunzio Guardone Maria Gul Cong Guo Jingyuan Guo Wanlei Guo Xinheng Guo Yuhang Guo Paul Hackspacher Caren Hagner Ran Han Yan Yerevan Physics Institute YerevanArmenia UniversitéLibre de Bruxelles BrusselsBelgium Universidade Estadual de Londrina LondrinaBrazil Pontificia Universidade Catolica do Rio de Janeiro RioBrazil Pontificia Universidad Católica de Chile SantiagoChile Universidad Tecnica Federico Santa Maria ValparaisoChile Beijing Institute of Spacecraft Environment Engineering BeijingChina Beijing Normal University BeijingChina China Institute of Atomic Energy BeijingChina Institute of High Energy Physics BeijingChina North China Electric Power University BeijingChina School of Physics Peking UniversityBeijingChina Tsinghua University BeijingChina University of Chinese Academy of Sciences BeijingChina Jilin University ChangchunChina College of Electronic Science and Engineering National University of Defense TechnologyChangshaChina Chongqing University ChongqingChina Dongguan University of Technology DongguanChina Jinan University GuangzhouChina Sun Yat-Sen University GuangzhouChina Harbin Institute of Technology HarbinChina University of Science and Technology of China HefeiChina The Radiochemistry and Nuclear Chemistry Group in University of South China HengyangChina Wuyi University JiangmenChina Shandong University JinanChina Institute of Modern Physics Chinese Academy of SciencesLanzhouChina Nanjing University NanjingChina Guangxi University NanningChina East China University of Science and Technology ShanghaiChina School of Physics and Astronomy Shanghai Jiao Tong UniversityShanghaiChina Tsung-Dao Lee Institute Shanghai Jiao Tong UniversityShanghaiChina Institute of Hydrogeology and Environmental Geology Chinese Academy of Geological SciencesShijiazhuangChina Nankai University TianjinChina Wuhan University WuhanChina Xi’an Jiaotong University Xi’anChina Xiamen University XiamenChina School of Physics and Microelectronics Zhengzhou UniversityZhengzhouChina Institute of Physics National Chiao-Tung University Hsinchu National United University Miao-Li Department of Physics National T

The Jiangmen Underground Neutrino Observatory(JUNO)features a 20 kt multi-purpose underground liquid scintillator sphere as its main *** of JUNO's features make it an excellent location for^8B solar neutrino measurements,such as its low-energy threshold,high energy resolution compared with water Cherenkov detectors,and much larger target mass compared with previous liquid scintillator *** this paper,we present a comprehensive assessment of JUNO's potential for detecting^8B solar neutrinos via the neutrino-electron elastic scattering process.A reduced 2 MeV threshold for the recoil electron energy is found to be achievable,assuming that the intrinsic radioactive background^(238)U and^(232)Th in the liquid scintillator can be controlled to 10^(-17)g/*** ten years of data acquisition,approximately 60,000 signal and 30,000 background events are *** large sample will enable an examination of the distortion of the recoil electron spectrum that is dominated by the neutrino flavor transformation in the dense solar matter,which will shed new light on the inconsistency between the measured electron spectra and the predictions of the standard three-flavor neutrino oscillation *** m^(2)_(21)=4.8times10^(-5);(7.5times10^(-5))eV^(2),JUNO can provide evidence of neutrino oscillation in the Earth at approximately the 3sigma(2sigma)level by measuring the non-zero signal rate variation with respect to the solar zenith ***,JUNO can simultaneously measureDelta m^2_(21)using^8B solar neutrinos to a precision of 20% or better,depending on the central value,and to sub-percent precision using reactor antineutrinos.A comparison of these two measurements from the same detector will help understand the current mild inconsistency between the value of Delta m^2_(21)reported by solar neutrino experiments and the KamLAND experiment.

关键词： neutrino oscillation solar neutrino JUNO