检索结果-南通市图书馆

在线全文

同方期刊数据库

学校读者我要写书评

暂无评论

19世纪4部《大清律例》法文译本译者序言

南大法学 2021年第5期 155-166页

作者： [法]菲利克斯·勒努阿尔 [法]加布里埃尔·奥巴雷 [法]保罗-路易-菲利克斯·菲拉斯特 [法]鲍来思王春荣(译) 孙雅文(校) 不详上海政法学院华东政法大学华东政法大学外语学院

《大清律例》自1810年被英国汉学家及时任英属东印度公司广州特选委员会成员的小斯当东爵士(Sir George thomas Staunton)译成英文在欧洲出版后,四部法文译本也相继于19世纪问世。1812年,勒努阿尔侯爵率先把小斯当东的英译本转译成法文;... 详细信息

《大清律例》自1810年被英国汉学家及时任英属东印度公司广州特选委员会成员的小斯当东爵士(Sir George thomas Staunton)译成英文在欧洲出版后,四部法文译本也相继于19世纪问世。1812年,勒努阿尔侯爵率先把小斯当东的英译本转译成法文;1865年,加布里埃尔·奥巴雷中校把当时越南阮朝效仿《大清律例》所撰的《皇越律例》(欧洲人称之为《安南法典》)首次从中文原著译成法文,它是法国在殖民安南初期对安南乃至中国法律的首次窥探;1876年,霍道生上尉重译《安南法典》,该法译本以其译文和内容的完整性而闻名;1891年,来华耶稣会士鲍来思神父基于《大清律例》《大清会典》等书籍编译了一本给传教士用的手册,取名为《大清律例便览》。现把这4部译著的译者序言译成中文,以此展示19世纪法国人眼中的中国传统法律观。为便于读者理解,对文中相关术语、词条及文本考证以脚注形式作补充说明,脚注皆为译者注。

关键词：《大清律例》法文译本译者序言《安南法典》、中国法

f.asibility and physics potential of.detecting ^(8)B solar neutrinos at JUNO

在线全文

学校读者我要写书评

暂无评论

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 f.ngpeng An Guangpeng An Qi An Giuseppe Andronico Nikolay Anf.mov 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 Birkenf.ld 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 Guof. Cao Jun Cao Rossella Caruso Cédric Cerna Jinf.n 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 Conf.rti Di Lorenzo Daniele Corti Salvatore Costa f.avio Dal Corso Christophe De La Taille Jiawei Deng Zhi Deng Ziyan Deng Wilf.ied Depnering Marco Diaz Xuef.ng Ding Yayun Ding Bayu Dirgantara Sergey Dmitrievsky Tadeas Dohnal Georgy Donchenko Jianmeng Dong Damien Dornic Evgeny Doroshkevich Marcos Dracos f.édéric Druillole Shuxian Du Stef.no Dusini Martin Dvorak Timo Enqvist Heike Enzmann Andrea f.bbri Lukas f.jt Donghua f.n Lei f.n Can f.ng Jian f.ng Marco f.rgetta Anna f.tkina Dmitry f.doseev Vladko f.kete Li-Cheng f.ng Qichun f.ng Richard f.rd Andrey f.rmozov Amélie f.urnier Haonan Gan f.ng Gao Alberto Garf.gnini Alexandre Göttel Christoph Genster Marco Giammarchi Agnese Giaz Nunzio Giudice f.anco Giuliani Maxim Gonchar Guanghua Gong Hui Gong Oleg Gorchakov Yuri Gornushkin Marco Grassi Christian Grewing Maxim Gromov Vasily Gromov Minghao Gu Xiaof.i 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 Pontif.cia Universidade Catolica do Rio de Janeiro RioBrazil Pontif.cia Universidad Católica de Chile SantiagoChile Universidad Tecnica f.derico Santa Maria ValparaisoChile Beijing Institute of.Spacecraf. 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)f.atures a 20 kt multi-purpose underground liquid scintillator sphere as its main *** of.JUNO's f.atures make it an excellent location f.r^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 f.r detecting^8B solar neutrinos via the neutrino-electron elastic scattering process.A reduced 2 MeV threshold f.r the recoil electron energy is f.und 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 f.avor transf.rmation 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-f.avor 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 f.om 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

Sub-percent precision measurement of.neutrino oscillation parameters with JUNO

在线全文

学校读者我要写书评

暂无评论

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 f.ngpeng An Qi An Giuseppe Andronico Nikolay Anf.mov 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 Birkenf.ld 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 Guof. Cao Jun Cao Rossella Caruso Cédric Cerna Chi Chan Jinf.n 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 Conf.rti Di Lorenzo Daniele Corti f.avio Dal Corso Olivia Dalager Christophe De La Taille Zhi Deng Ziyan Deng Wilf.ied Depnering Marco Diaz Xuef.ng Ding Yayun Ding Bayu Dirgantara Sergey Dmitrievsky Tadeas Dohnal Dmitry Dolzhikov Georgy Donchenko Jianmeng Dong Evgeny Doroshkevich Marcos Dracos f.édéric Druillole Ran Du Shuxian Du Stef.no Dusini Martin Dvorak Timo Enqvist Heike Enzmann Andrea f.bbri Donghua f.n Lei f.n Jian f.ng Wenxing f.ng Marco f.rgetta Dmitry f.doseev Zhengyong f.i Li-Cheng f.ng Qichun f.ng Richard f.rd Amélie f.urnier Haonan Gan f.ng Gao Alberto Garf.gnini Arsenii Gavrikov Marco Giammarchi Nunzio Giudice Maxim Gonchar Guanghua Gong Hui Gong Yuri Gornushkin Alexandre Göttel Marco Grassi Vasily Gromov Minghao Gu Xiaof.i 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 Raf.el Herrera YuenKeung Ho Yerevan Physics Institute YerevanArmenia UniversiéLibre de Bruxelles BrusselsBelgium Universidade Estadual de Londrina LondrinaBrazil Pontif.cia Universidade Catolica do Rio de Janeiro Rio de JaneiroBrazil Pontif.cia Universidad Católica de Chile SantiagoChile Universidad Tecnica f.derico Santa Maria ValparaisoChile Beijing Institute of.Spacecraf. 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 f.r 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 f.om the TAO satellite *** is f.und 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 f.r each mass ordering *** new precision represents approximately an order of.magnitude improvement over existing constraints f.r these three parameters.

关键词： neutrino oscillation reactor antineutrino precision measurement JUNO

JUNO sensitivity on proton decay p→νK^(+)searches

在线全文

学校读者我要写书评

暂无评论

Chinese Physics C 2023年第11期47卷 7-22页

作者： Angel Abusleme thomas Adam Shakeel Ahmad Rizwan Ahmed Sebastiano Aiello Muhammad Akram 安丰鹏安琪 Giuseppe Andronico Nikolay Anf.mov Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde Marcondes de André Didier Auguste Nikita Balashov Wander Baldini Andrea Barresi Davide Basilico Eric Baussan Marco Bellato Antonio Bergnoli Thilo Birkenf.ld Sylvie Blin David Blum Simon Blyth Anastasia Bolshakova Mathieu Bongrand Clément Bordereau Dominique Breton Augusto Brigatti Riccardo Brugnera Riccardo Bruno Antonio Budano Mario Buscemi Jose Busto Ilya Butorov Anatael Cabrera Barbara Caccianiga 蔡浩蔡啸蔡严克蔡志岩 Riccardo Callegari Antonio Cammi Agustin Campeny 曹传亚曹国富曹俊 Rossella Caruso Cédric Cerna 常劲帆 Yun Chang 陈平平 Po-An Chen 陈少敏陈旭荣 Yi-Wen Chen 陈义学陈羽陈长程捷程雅苹 Alexey Chetverikov Davide Chiesa Pietro Chimenti Artem Chukanov Gérard Claverie Catia Clementi Barbara Clerbaux Selma Conf.rti Di Lorenzo Daniele Corti f.avio Dal Corso Olivia Dalager Christophe De La Taille 邓智邓子艳 Wilf.ied Depnering Marco Diaz Xuef.ng Ding 丁雅韵 Bayu Dirgantara Sergey Dmitrievsky Tadeas Dohnal Dmitry Dolzhikov Georgy Donchenko 董建蒙 Evgeny Doroshkevich Marcos Dracos f.édéric Druillole 杜然杜书先 Stef.no Dusini Martin Dvorak Timo Enqvist Heike Enzmann Andrea f.bbri Ulrike f.hrendholz 范东华樊磊方建方文兴 Marco f.rgetta Dmitry f.doseev Li-Cheng f.ng 冯启春 Richard f.rd Amélie f.urnier 甘浩男 f.ng Gao Alberto Garf.gnini Arsenii Gavrikov Marco Giammarchi Agnese Giaz Nunzio Giudice Maxim Gonchar 龚光华宫辉 Yuri Gornushkin Alexandre Göttel Marco Grassi Christian Grewing Vasily Gromov 顾旻皓谷肖飞古宇关梦云 Nunzio Guardone Maria Gul 郭聪郭竞渊郭万磊郭新恒郭宇航 Paul Hackspacher Caren Hagner 韩然 Yang Han Muhammad Sohaib Hassan 何苗何伟 Tobias Heinz Patrick Hellmuth 衡月昆 Raf.el Herrera 贺远强侯少静 Yee Hsiung Bei-Zhen Hu 胡航胡健润胡俊胡守扬胡涛胡宇翔胡焯钧黄春豪黄桂鸿黄翰雄黄文昊黄鑫黄性涛黄永波惠加琪霍雷霍文驹 Cédric Huss Saf.er Hussain Ara Ioannisian Roberto Isocrate Beatrice Jelmini Kuo-Lun Jen Ignacio Jeria 季筱璐吉星曌贾慧慧贾俊基蹇司玉蒋荻蒋炜江晓山金如意荆小平 Cécile Jollet Jari Joutsenvaara Sirichok Jungthawan Leonidas Kalousis Philipp Ka Pontif.cia Universidad Católica de Chile SantiagoChile IPHC Universitéde StrasbourgCNRS/IN2P3F-67037 StrasbourgFrance Pakistan Institute of.Nuclear Science and Technology IslamabadPakistan INf. Catania and Dipartimento di f.sica e Astronomia dell Universitàdi Catania CataniaItaly East China University of.Science and Technology ShanghaiChina University of.Science and Technology of.China HefeiChina Joint Institute f.r Nuclear Research DubnaRussia INf. Sezione di Milano and Dipartimento di f.sica dell Universitàdi Milano MilanoItaly Department of.Physics Faculty of ScienceChulalongkorn UniversityBangkokThailand IJCLab UniversitéParis-SaclayCNRS/IN2P391405 OrsayFrance Department of.Physics and Earth Science University of Ferrara and INFN Sezione di FerraraFerraraItaly INf. Milano Bicocca and University of.Milano Bicocca MilanoItaly INf. Sezione di Padova PadovaItaly III.Physikalisches Institut B RWTH Aachen UniversityAachenGermany Eberhard Karls Universität Tübingen Physikalisches InstitutTübingenGermany Institute of.High Energy Physics BeijingChina SUBATECH Universitéde NantesIMT AtlantiqueCNRS-IN2P3NantesFrance Univ.Bordeaux CNRSLP2IUMR 5797F-33170 GradignanFrance Department of.Physics National Taiwan UniversityTaipei Dipartimento di f.sica e Astronomia dell’Universitàdi Padova and INf. Sezione di Padova PadovaItaly University of.Roma Tre and INf. Sezione Roma Tre RomaItaly Aix Marseille Univ CNRS/IN2P3CPPMMarseilleFrance Wuhan University WuhanChina INf. Milano Bicocca and Politecnico of.Milano MilanoItaly National United University Miao-Li Dongguan University of.Technology DongguanChina Tsinghua University BeijingChina Institute of.Modern Physics Chinese Academy of SciencesLanzhouChina Institute of.Physics National Yang Ming Chiao Tung UniversityHsinchu North China Electric Power University BeijingChina Sun Yat-Sen University GuangzhouChina Beijing Institute of.Spacecraf. Environment Engineering BeijingChina Universidade Estadual de Londrina LondrinaBrazil INf. Sez

The Jiangmen Underground Neutrino Observatory(JUNO)is a large liquid scintillator detector designed to explore many topics in f.ndamental *** this study,the potential of.searching f.r proton decay in the p→νK^(+)mode with JUNO is *** kaon and its decay particles f.ature a clear three-f.ld coincidence signature that results in a high ef.iciency f.r ***,the excellent energy resolution of.JUNO permits suppression of.the sizable background caused by other delayed *** on these advantages,the detection ef.iciency f.r the proton decay via p→νK^(+)is 36.9%±4.9%with a background level of.0.2±0.05(syst)±0.2(stat)events af.er 10 years of.data *** estimated sensitivity based on 200 kton-years of.exposure is 9.6×1033 years,which is competitive with the current best limits on the proton lif.time in this channel and complements the use of.dif.erent detection technologies.

关键词： proton decay grand unif.ed theories JUNO liquid scintillator detector