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不同方法获得的脂肪来源干细胞再生能力比较：超声辅助吸脂与传统脂肪抽吸对比

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中国美容整形外科杂志 2015年第8期26卷 J0011-J0011页

作者： David Atashroo Dominik Duscher Zeshaan N. Maan Elizabeth R. Zielins Kevin Paik alexander Whittam Michelle Lin Adrian McArdle christopher Duldulao t Graham G. Walmsley Michael S.Hu Ruth Tevlin Derrick c. Wan Geoffrey c. Gurtner Michael T. Longaker 朱利娜高景恒张晨袁继龙不详《中国美容整形外科杂志》编辑部大连大学附属新华医院整形外科辽宁省人民医院整形外科

背景与目的超声辅助吸脂（ultrasound assisted liposuction，UAL）因其获取脂肪容易，且可让创伤和失血最小化，受到整形外科医师的青睐。但是，很少有研究报道这种方法获取的脂肪来源干细胞（adipose derived stromal cells，ADScs）... 详细信息

背景与目的超声辅助吸脂（ultrasound assisted liposuction，UAL）因其获取脂肪容易，且可让创伤和失血最小化，受到整形外科医师的青睐。但是，很少有研究报道这种方法获取的脂肪来源干细胞（adipose derived stromal cells，ADScs）的质量。ADScs在基于细胞的治疗方法中的作用也在急剧增长。因此，本研究比较了传统脂肪抽吸（suctionassistedliposuction，SAL）方法获得的ADScs与UAL方法获得的ADScs之间再生能力的差异。方法分别采用SAL和UAL方法，从健康人中获取脂肪并培养ADScs；采用荧光辅助细胞分选（fluorescent assisted cell sorting，FAcS）方法，分析ADScs的产量。利用MTT比色法分析ADScs的增殖能力，并在培养基中进行成脂和成骨分化诱导。将基因表达谱与qPcR进行对比。利用细胞染色比较成脂和成骨分化标记物。建立小鼠创伤愈合模型，在水凝胶支架上，分别播种采用SAL方法获取的ADScs（SAL组）和采用UAL方法获取的ADScs（UAL组），水凝胶组只加入水凝胶作为对照，同时比较3组的组织再生能力。结果UAL与SAL方法获得的ADScs相比，在细胞数量和增殖能力方面的差异无统计学意义。油红O染色显示两者成脂分化能力没有差异，分化7d时，PPAR-γ受体和LPL的表达差异无统计学意义也证实了这一点（P〉0．05）。同样，碱性磷酸酶和茜素红染色也显示了两者相似的成骨分化能力，而且成骨标志物Runx-2、骨桥蛋白和骨钙蛋白的表达差异也无统计学意义（P〉0．05）。SAL组和UAL组的愈合速度明显大于水凝胶组（P〈0．05），SAL和UAL两组之间差异无统计学意义（P〉0．05）。结论与传统SAL方法相比，UAL方法可获得相等增殖能力的ADScs，并用于以细胞疗法为基础的治疗。

关键词：细胞再生能力脂肪抽吸吸脂超声 ADScs 脂肪来源干细胞成骨分化整形外科医师

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

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结肠直肠癌姑息治疗的改进

德国医学 2001年第4期18卷 220-221页

作者： A.Wein c.Riedel B.Hanke S.Lampert W.Brückl B.Reingruber W.Hohenberger E.G.Hahn 张林 MedizinischeKlinik I mit Poliklinik Friedrich-Alexander-Universitat Erlangen-NumbergKrankenhausstrabe 12D-91054 ErlangenGermany MedizinischeKlinik I mit Poliklinik Friedrich-Alexander-Universitat Erlangen-Numberg 华中科技大学同济医学院附属同济医院

结肠直肠癌的发病率约为50/100?000,占女性肿瘤的第二位和男性肿瘤的第三位.约20?000例病人可以形成同时或异时的转移,最常见为肝转移.这类病人是行转移灶切除术的绝对适应证,因为根治手术的5年生存率可以达到25%～38%.如果不能切除的话... 详细信息

结肠直肠癌的发病率约为50/100?000,占女性肿瘤的第二位和男性肿瘤的第三位.约20?000例病人可以形成同时或异时的转移,最常见为肝转移.这类病人是行转移灶切除术的绝对适应证,因为根治手术的5年生存率可以达到25%～38%.如果不能切除的话,应该进行其他的姑息治疗,本文对此综述如下.

关键词：结肠直肠癌外科切除术治疗方法药物治疗化疗

急性缺血性卒中静脉阿替普酶溶栓治疗的纳入和排除标准的科学依据美国心脏协会/美国卒中协会对医疗卫生专业人员发布的声明(续前)

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国际脑血管病杂志 2016年第5期 385-406页

作者： Demaerschalk Bart M. Kleindorfer Dawn O. Adeoye Opeolu M. Demchuk Andrew M. Fugate Jennifer E. Grotta James c. Khalessi alexander A. Levy Elad I. Palesch Yuko Y. Prabhakaran Shyam Saposnik Gustavo Saver Jeffrey L. Smith Eric E. 南京大学医学院附属鼓楼医院神经内科

19颅内出血史根据最初的FDA标签和2013年AHA/ASA指南[24],颅内出血史是静脉阿替普酶治疗缺血性卒中的一项额外禁忌证或排除标准。最近修订后的标签仅将近期IcH列为一项警告,并且在禁忌证中删除了IcH史。与前面讨论的静脉阿替普酶治疗排...

19颅内出血史根据最初的FDA标签和2013年AHA/ASA指南[24],颅内出血史是静脉阿替普酶治疗缺血性卒中的一项额外禁忌证或排除标准。最近修订后的标签仅将近期IcH列为一项警告,并且在禁忌证中删除了IcH史。与前面讨论的静脉阿替普酶治疗排除标准相似,文献回顾仅在大样本回顾性研究中发现了少量这类病例。缺乏相关数据可能是修订后的

关键词：

公共卫生监测的过去、现在和未来:(一)过去

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疾病监测 2015年第9期30卷 706-716页

作者：蔡智强李丽萍白雲屛汕头大学医学院伤害预防中心广东汕头515041 渥太华大学流行病学与社区医学教研室渥太华大学院校研究与规划办公室

本文描述通过公共卫生行动的计划、实施和评价对卫生数据不断地系统地进行收集、分析、解释和利用公共卫生信息的过程,对公共卫生监测发展的历史进行了全面地综述。公共卫生监测最早要追溯到公元前3180年埃及第一次记录的传染病。希波... 详细信息

本文描述通过公共卫生行动的计划、实施和评价对卫生数据不断地系统地进行收集、分析、解释和利用公共卫生信息的过程,对公共卫生监测发展的历史进行了全面地综述。公共卫生监测最早要追溯到公元前3180年埃及第一次记录的传染病。希波克拉底(Hippocrates)(公元前460 370年)记录了地方病和流行病;约翰·格兰特(John Graunt)(1620 1674年)提出了系统数据分析;塞缪尔·皮普斯(Samuel Pepys)(1633 1703年)开始了流行病学现场调查;威廉·法尔(William Farr)(1807 1883年)创建了现代监测的概念;约翰·斯诺(John Snow)(1813 1858年)将数据资料和随后的干预活动联系在一起;亚历山大·朗缪尔(alexander Langmuir)(19101993年)首次提出了监测的全面定义,如今已形成系统的理论和大量的监测方法,并在全球范围内建立了公共卫生监测机构。学习公共卫生监测的发展历程,用以反思当前的发展现状,提高和促进公共卫生监测,为人类健康提供理论依据。

关键词：公共卫生监测历史发展流行病

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阿尔泰山地区全新世植被和气候变化（英文）

阿尔泰山地区全新世植被和气候变化（英文）

Observatory science with eXTP

中国古生物学会第十二次全国会员代表大会暨第29届学术年会

作者：黄小忠彭卫 Natalia Rudaya Eric c.Grimm 陈雪梅曹现勇张军潘小多刘思丝陈春珠陈发虎 Key Laboratory of Western china's Environmental System(Ministry of Education) College of Earth and Environmental SciencesLanzhou University Kazan State University Alfred Wegener Institute Helmholtz center for Polar and Marine Research Department of Periglacial Research Institute of Earth and Environmental Science University of Potsdam Department of Earth Sciences University of Minnesota Northwest Institute of Eco-Environment and Resources Chinese Academy of Sciences Institute of Tibetan Plateau Research Chinese Academy of Sciences School of Geographic Science Nantong University

A comprehensive understanding of the regional vegetation responses to long-term climate change will help forecast earth system *** on a new well-dated pollen dataset from Kanas Lake and a review of published pollen records from in and around the Altai Mountains,the regional vegetation dynamics and forcing mechanisms are *** the Altai Mountains,the forest optimum occurred during 10-7 ka for the upper forest zone and a tree line decline and/or ecological shifts were caused by climatic cooling from around 7 *** the lower forest zone,the forest reached an optimum in the middle Holocene,and then increased openness of the forest,possibly caused by both climatic cooling and human activities,occurred in the late *** the lower basins or plains around the Altai Mountains,the development of proto-grassland or forest benefited from increasing humidity in the middle to late *** Points:A new pollen data set from a large deep lake was used to interpret the regional vegetation and climate of the southern Altai *** vegetation showed different long-term responses to climate change in and around the Altai *** dynamics and their impact on geophysical processes should be incorporated into coupled vegetation-climate models.

关键词： Altai Mountains Kanas Lake Holocene vegetation climate change

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Science china(Physics,Mechanics & Astronomy) 2019年第2期62卷 97-138页

作者： Jean J.M.in 't Zand Enrico Bozzo JinLu Qu Xiang-Dong Li Lorenzo Amati Yang chen Immacolata Donnarumma Victor Doroshenko Stephen A.Drake Margarita Hernanz Peter A.Jenke Thomas J.Maccarone Simin Mahmoodifar Domitilla de Martino Alessandra De Rosa Elena M.Rossi Antonia Rowlinson Gloria Sala Giulia Stratta Thomas M.Tauris Joern Wilms XueFeng Wu Ping Zhou Iván Agudo Diego Altamirano Jean-Luc Atteia Nils A.andersson M.cristina Baglio David R.Ballantyne Altan Baykal Ehud Behar Tomaso Belloni Sudip Bhattacharyya Stefano Bianchi Anna Bilous Pere Blay Joao Braga Sφren Brandt Edward F.Brown Niccolo Bucciantini Luciano Burderi Edward M.cackett Riccardo campana Sergio campana Piergiorgio casella Yuri cavecchi Frank chambers Liang chen Yu-Peng chen Jér?me chenevez Maria chernyakova chichuan Jin Riccardo ciolfi Elisa costantini Andrew cumming Antonino D'Aì Zi-Gao Dai Filippo D'Ammando Massimiliano De Pasquale Nathalie Degenaar Melania Del Santo Valerio D'Elia Tiziana Di Salvo Gerry Doyle Maurizio Falanga XiLong Fan Robert D.Ferdman Marco Feroci Federico Fraschetti Duncan K.Galloway Angelo F.Gambino Poshak Gandhi MingYu Ge Bruce Gendre Ramandeep Gill Diego G?tz christian Gouiffès Paola Grandi Jonathan Granot Manuel Güdel alexander Heger craig O.Heinke Jeroen Homan Rosario Iaria Kazushi Iwasawa Luca Izzo Long Ji Peter G.Jonker Jordi José Jelle S.Kaastra Emrah Kalemci Oleg Kargaltsev Nobuyuki Kawai Laurens Keek Stefanie Komossa Ingo Kreykenbohm Lucien Kuiper Devaky Kunneriath Gang Li En-Wei Liang Manuel Linares Francesco Longo FangJun Lu alexander A.Lutovinov Denys Malyshev Julien Malzac Antonios Manousakis Ian McHardy Missagh Mehdipour YunPeng Men Mariano Méndez Roberto P.Mignani Romana Mikusincova M.coleman Miller Giovanni Miniutti christian Motch Joonas Nättilä Emanuele Nardini Torsten Neubert Paul T.O'Brien Mauro Orlandini Julian P.Osborne Luigi Pacciani Stéphane Paltani Maurizio Paolillo Iossif E.Papadakis Biswajit Paul Alberto Pellizzoni Uria Peretz Miguel A.Pérez Torres Emanuele Perinati chanda Prescod-Weinstein Pablo Reig SRON Netherlands Institute for Space Research Department of Astronomy University of Geneva Key Laboratory for Particle Astrophysics Institute of High Energy PhysicsChinese Academy of Sciences School of Astronomy and Space Science Nanjing University INAF-IASF Bologna ASI Via del Politecnico snc INAF-Istituto di Astrofisica e Planetologie Spaziali Institut für Astronomie und Astrophysik Tübingen Universit?t Tübingen NASA Goddard Space Flight center IcREA&Institute of Space Sciences(IEEc-cSIc) Campus UABCarrer de Can Magrans cSPAR SPA University of Alabama in Huntsville Department of Physics Texas Tech University INAF Osservatorio Astronomico di capodimonte Leiden Observatory Leiden University Anton Pannekoek Institute University of Amsterdam ASTRON Netherlands Institute for Radio Astronomy Universitat Politecnica de catalunya(UPc-IEEc) Universitádegli Studi di Urbino‘carlo Bo’ Max-Planck-Institut für Radioastronomie Dr.Karl-Remeis-Sternwarte and Erlangen centre for Astroparticle Physics(EcAP) Friedrich Alexander Universit?t Erlangen-Nurnberg Purple Mountain Observatory Chinese Academy of Sciences Instituto de Astrofysíca de Andalucia-cSIc Department of Physics and Astronomy University of Southampton IRAP Universitéde ToulouseCNRSUPSCNES Mathematical Sciences and STAG Research centre University of Southampton New York University Abu Dhabi center for Relativistic Astrophysics School of PhysicsGeorgia Institute of Technology Physics Department Middle East Technical University Department of Physics Technion-Israel Institute of Technology INAF Osservatorio Astronomico di Brera Tata Institute of Fundamental Research Dipartimento di Matematica e Fisica Universitàdegli Studi Roma Tre Instituto de Astrofísica de canarias Instituto Nacional de Pesquisas Espaciais-INPE National Space Institute Technical University of Denmark(DTU Space) Department of Physics and Astronomy Michigan State University INAF Osservatorio Astrofisico di Arcetri Dipartimento di Fisica Universitádegli Studi di Cagliari Department of Physics and A

In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry(eXTP) mission for studies related to Observatory Science targets. These include flaring stars, supernova remnants, accreting white dwarfs, low and high mass X-ray binaries, radio quiet and radio loud active galactic nuclei, tidal disruption events, and gamma-ray bursts. eXTP will be excellently suited to study one common aspect of these objects: their often transient nature. Developed by an international consortium led by the Institute of High Energy Physics of the chinese Academy of Science, the eXTP mission is expected to be launched in the mid 2020s.

关键词： space research in struments nuclear astrophysics flare stars accretion and accretion disks mass loss and stellar winds cataclysmic binaries X-ray binaries supernova remnants active galactic nuclei X-ray bursts gamma-ray bursts gravitational waves

超快TWIST-VIBE Dixon序列与扩散加权成像的联合成为准确且便于应用的乳腺MRI肿块分类工具

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国际医学放射学杂志 2020年第4期 497-497页

作者： S.c.Peter E.Wenkel E.Weiland M.Dietzel R.Janka A.Hartmann 马闻竟 Department of Radiology Erlangen University HospitalFriedrich-Alexander Universit?t Erlangen-Nürnberg (FAU)

目的本研究旨在开发一种联合超快TWISTVIBE-Dixon(TVD)动态序列与扩散加权成像(DWI)序列的乳腺MRI肿块分类工具。虽然TVD序列可以简化乳腺MRI

关键词：

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