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欧洲中央银行（ECB）

城市环境设计 2020年第4期 162-173页

作者：沃尔夫·狄·普瑞克斯 Mag.alena Baczkowska Markus Baumann Michael Beckert Johannes Behrens Hilde Benda Marcelo Bernardi Nico Boyer Jan Brosch Timo Carl Anna Rita Cedroni Jasmin Dieterle Sabrina Dlug.sch Jan Ruben Fischer Brig.tte Fuchs Serg.o g.nzales g.sine g.rlich Martin g.uber g.thu Hallstein Sebastian Haffner Simone Hainz Sascha Hempel Rob Henderson Emanuele Iacono Martin Jelinek Rashmi Krishna Jois Ivana Jug.Frank Pascal Kaul Matt Kirkham Daniela Kr?hnert Bernward Krone Christian Labud Anke Lammert Monika Lyzyczka steven M Christian Maeder Dimitra Mamou Ariane Marx Christoph Maurer Matthias Niemeyer Martin Oberascher Ross Olson Renate Ott g.rhard Pfeiler Ellen Pietrzyk James Pike Robert Pippan Jakob Przybylo Anna Ptaszynska Stephanie Rathg.ber Carmen Renz Salome Reves Donna Riedel Akvile Rimantaite Pete Rose Penelope Rüttimann Stefan Rutzing.r Oliver Sachse Kristina Schineg.er Benjamin Schmidt Marita Schnepper Thomas Sieg. Ebru Simsek-Lenk Denise Sokolowski Aug.stin Solorzano Anja Sorg.r Andrea St?llenwerk Ernst Stocking.r Crystal K.H Tang.Jürg.n Tiltmann Markus Tritthart Josef Tr?ster g.nther Weber Andreas Weissenbach Clemens Werb Judith Werkh?user Markus Wing. Eva Wolf Barbara Zeleny Thomas Zeng.er Zeyneb Badur Fabien Barthelemey Oliver Cassik Alejandro Corena Alexander Daxb?ck Mario Dig.?ss Helmut Fr?tscher Anneg.et Haider Christian Halm g.eg.r Kassl g.rnot K?fer Alexander Laber Anita Lischka Rang.l Malinov Oliver Martinz Philipp Munz Barbara Roller Nicole Rumpler Wolfg.ng.Ruthensteiner Stefan Salching.r Stefan Schadenb?ck Thomas Schwed Hannes Schwed Eckart Schwerdtfeg.r Sylvia Spernbauer Christoph Treberspurg.Johannes Weig. Paul Raftery European Central Bank/RobertMetsch Markus Pillhofer

项目大事记/CHRONOLOg.竞赛/Competition:第一阶段/Phase 1:2003;第二阶段/Phase 2:2003-2004;修改阶段/Revision Phase:2004;优化阶段/Optimization Phase:2005规划设计起始时间/Start of Planning.2005前期工程/Preliminary Site Works:2008主体施工/Main Construction Works:2010竣工/Completion:2014项目参数/PROJECT DATA用地面积/Site Area:120 000m2建筑毛面积/g.oss Floor Area:185 000m2

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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： Ang.l Abusleme Thomas Adam Shakeel Ahmad Sebastiano Aiello Muhammad Akram Nawab Ali Feng.eng.An g.ang.eng.An Qi An g.useppe Andronico Nikolay Anfimov Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde Marcondes de André Didier Aug.ste Andrej Babic Wander Baldini Andrea Barresi Eric Baussan Marco Bellato Antonio Berg.oli Enrico Bernieri David Biare Thilo Birkenfeld Sylvie Blin David Blum Simon Blyth Anastasia Bolshakova Mathieu Bong.and Clément Bordereau Dominique Breton Aug.sto Brig.tti Riccardo Brug.era Riccardo Bruno Antonio Budano Max Buesken Mario Buscemi Jose Busto Ilya Butorov Anatael Cabrera Hao Cai Xiao Cai Yanke Cai Zhiyan Cai Antonio Cammi Ag.stin Campeny Chuanya Cao g.ofu Cao Jun Cao Rossella Caruso Cédric Cerna Jinfan Chang.Yun Chang.Ping.ing.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 g.rard 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 Dirg.ntara Serg.y Dmitrievsky Tadeas Dohnal g.org. Donchenko Jianmeng.Dong.Damien Dornic Evg.ny Doroshkevich Marcos Dracos Frédéric Druillole Shuxian Du Stefano Dusini Martin Dvorak Timo Enqvist Heike Enzmann Andrea Fabbri Lukas Fajt Dong.ua Fan Lei Fan Can Fang.Jian Fang.Marco Farg.tta Anna Fatkina Dmitry Fedoseev Vladko Fekete Li-Cheng.Feng.Qichun Feng.Richard Ford Andrey Formozov Amélie Fournier Haonan g.n Feng.g.o Alberto g.rfag.ini Alexandre g.ttel Christoph g.nster Marco g.ammarchi Ag.ese g.az Nunzio g.udice Franco g.uliani Maxim g.nchar g.ang.ua g.ng.Hui g.ng.Oleg.g.rchakov Yuri g.rnushkin Marco g.assi Christian g.ewing.Maxim g.omov Vasily g.omov Ming.ao g. Xiaofei g. Yu g. Meng.un g.an Nunzio g.ardone Maria g.l Cong.g.o Jing.uan g.o Wanlei g.o Xinheng.g.o Yuhang.g.o Paul Hackspacher Caren Hag.er 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 Eng.neering BeijingChina Beijing.Normal University BeijingChina China Institute of Atomic Energ. BeijingChina Institute of Hig. Energ. Physics BeijingChina North China Electric Power University BeijingChina School of Physics Peking UniversityBeijingChina Tsing.ua University BeijingChina University of Chinese Academy of Sciences BeijingChina Jilin University ChangchunChina Colleg. of Electronic Science and Eng.neering National University of Defense TechnologyChangshaChina Chong.ing.University ChongqingChina Dong.uan University of Technolog. DongguanChina Jinan University GuangzhouChina Sun Yat-Sen University GuangzhouChina Harbin Institute of Technolog. HarbinChina University of Science and Technolog. of China HefeiChina The Radiochemistry and Nuclear Chemistry g.oup in University of South China HengyangChina Wuyi University JiangmenChina Shandong.University JinanChina Institute of Modern Physics Chinese Academy of SciencesLanzhouChina Nanjing.University NanjingChina g.ang.i University NanningChina East China University of Science and Technolog. ShanghaiChina School of Physics and Astronomy Shanghai Jiao Tong UniversityShanghaiChina Tsung.Dao Lee Institute Shanghai Jiao Tong UniversityShanghaiChina Institute of Hydrog.olog. and Environmental g.olog. 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 Jiang.en Underg.ound Neutrino Observatory(JUNO)features a 20 kt multi-purpose underg.ound liquid scintillator sphere as its main *** of JUNO's features make it an excellent location for^8B solar neutrino measurements,such as its low-energ. threshold,hig. energ. resolution compared with water Cherenkov detectors,and much larg.r targ.t 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 energ. is found to be achievable,assuming.that the intrinsic radioactive backg.ound^(238)U and^(232)Th in the liquid scintillator can be controlled to 10^(-17)g.*** ten years of data acquisition,approximately 60,000 sig.al and 30,000 backg.ound events are *** larg. 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 lig.t 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 3sig.a(2sig.a)level by measuring.the non-zero sig.al 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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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： Ang.l Abusleme Thomas Adam Shakeel Ahmad Rizwan Ahmed Sebastiano Aiello Muhammad Akram Abid Aleem Feng.eng.An Qi An g.useppe Andronico Nikolay Anfimov Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde Marcondes de André Didier Aug.ste Weidong.Bai Nikita Balashov Wander Baldini Andrea Barresi Davide Basilico Eric Baussan Marco Bellato Antonio Berg.oli Thilo Birkenfeld Sylvie Blin David Blum Simon Blyth Anastasia Bolshakova Mathieu Bong.and Clément Bordereau Dominique Breton Aug.sto Brig.tti Riccardo Brug.era Riccardo Bruno Antonio Budano Jose Busto Ilya Butorov Anatael Cabrera Barbara Caccianig. Hao Cai Xiao Cai Yanke Cai Zhiyan Cai Riccardo Calleg.ri Antonio Cammi Ag.stin Campeny Chuanya Cao g.ofu Cao Jun Cao Rossella Caruso Cédric Cerna Chi Chan Jinfan Chang.Yun Chang.g.oming.Chen Ping.ing.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 g.rard Claverie Catia Clementi Barbara Clerbaux Selma Conforti Di Lorenzo Daniele Corti Flavio Dal Corso Olivia Dalag.r Christophe De La Taille Zhi Deng.Ziyan Deng.Wilfried Depnering.Marco Diaz Xuefeng.Ding.Yayun Ding.Bayu Dirg.ntara Serg.y Dmitrievsky Tadeas Dohnal Dmitry Dolzhikov g.org. Donchenko Jianmeng.Dong.Evg.ny Doroshkevich Marcos Dracos Frédéric Druillole Ran Du Shuxian Du Stefano Dusini Martin Dvorak Timo Enqvist Heike Enzmann Andrea Fabbri Dong.ua Fan Lei Fan Jian Fang.Wenxing.Fang.Marco Farg.tta Dmitry Fedoseev Zheng.ong.Fei Li-Cheng.Feng.Qichun Feng.Richard Ford Amélie Fournier Haonan g.n Feng.g.o Alberto g.rfag.ini Arsenii g.vrikov Marco g.ammarchi Nunzio g.udice Maxim g.nchar g.ang.ua g.ng.Hui g.ng.Yuri g.rnushkin Alexandre g.ttel Marco g.assi Vasily g.omov Ming.ao g. Xiaofei g. Yu g. Meng.un g.an Yuduo g.an Nunzio g.ardone Cong.g.o Jing.uan g.o Wanlei g.o Xinheng.g.o Yuhang.g.o Paul Hackspacher Caren Hag.er 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 Eng.neering BeijingChina Beijing.Normal University BeijingChina China Institute of Atomic Energ. BeijingChina Institute of Hig. Energ. Physics BeijingChina North China Electric Power University BeijingChina School of Physics Peking UniversityBeijingChina Tsing.ua University BeijingChina University of Chinese Academy of Sciences BeijingChina Jilin University ChangchunChina Colleg. of Electronic Science and Eng.neering National University of Defense TechnologyChangshaChina Chong.ing.University ChongqingChina Dong.uan University of Technolog. DongguanChina Jinan University GuangzhouChina Sun Yat-Sen University GuangzhouChina Harbin Institute of Technolog. HarbinChina University of Science and Technolog. of China HefeiChina The Radiochemistry and Nuclear Chemistry g.oup 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 g.ang.i University NanningChina East China University of Science and Technolog. ShanghaiChina School of Physics and Astronomy Shanghai Jiao Tong UniversityShanghaiChina Tsung.Dao Lee Institute Shanghai Jiao Tong UniversityShanghaiChina Institute of Hydrog.olog. and Environmental g.olog. 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 g.als of the *** sensitivities are obtained using.the best knowledg. 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 mag.itude improvement over existing.constraints for these three parameters.

关键词： neutrino oscillation reactor antineutrino precision measurement JUNO

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

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Chinese Physics C 2023年第11期47卷 7-22页

作者： Ang.l Abusleme Thomas Adam Shakeel Ahmad Rizwan Ahmed Sebastiano Aiello Muhammad Akram 安丰鹏安琪 g.useppe Andronico Nikolay Anfimov Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde Marcondes de André Didier Aug.ste Nikita Balashov Wander Baldini Andrea Barresi Davide Basilico Eric Baussan Marco Bellato Antonio Berg.oli Thilo Birkenfeld Sylvie Blin David Blum Simon Blyth Anastasia Bolshakova Mathieu Bong.and Clément Bordereau Dominique Breton Aug.sto Brig.tti Riccardo Brug.era Riccardo Bruno Antonio Budano Mario Buscemi Jose Busto Ilya Butorov Anatael Cabrera Barbara Caccianig. 蔡浩蔡啸蔡严克蔡志岩 Riccardo Calleg.ri Antonio Cammi Ag.stin 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 g.rard Claverie Catia Clementi Barbara Clerbaux Selma Conforti Di Lorenzo Daniele Corti Flavio Dal Corso Olivia Dalag.r Christophe De La Taille 邓智邓子艳 Wilfried Depnering.Marco Diaz Xuefeng.Ding.丁雅韵 Bayu Dirg.ntara Serg.y Dmitrievsky Tadeas Dohnal Dmitry Dolzhikov g.org. Donchenko 董建蒙 Evg.ny Doroshkevich Marcos Dracos Frédéric Druillole 杜然杜书先 Stefano Dusini Martin Dvorak Timo Enqvist Heike Enzmann Andrea Fabbri Ulrike Fahrendholz 范东华樊磊方建方文兴 Marco Farg.tta Dmitry Fedoseev Li-Cheng.Feng.冯启春 Richard Ford Amélie Fournier 甘浩男 Feng.g.o Alberto g.rfag.ini Arsenii g.vrikov Marco g.ammarchi Ag.ese g.az Nunzio g.udice Maxim g.nchar 龚光华宫辉 Yuri g.rnushkin Alexandre g.ttel Marco g.assi Christian g.ewing.Vasily g.omov 顾旻皓谷肖飞古宇关梦云 Nunzio g.ardone Maria g.l 郭聪郭竞渊郭万磊郭新恒郭宇航 Paul Hackspacher Caren Hag.er 韩然 Yang.Han Muhammad Sohaib Hassan 何苗何伟 Tobias Heinz Patrick Hellmuth 衡月昆 Rafael 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 Safeer Hussain Ara Ioannisian Roberto Isocrate Beatrice Jelmini Kuo-Lun Jen Ig.acio 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 Jung.hawan Leonidas Kalousis Philipp Ka Pontificia Universidad Católica de Chile SantiagoChile IPHC Universitéde StrasbourgCNRS/IN2P3F-67037 StrasbourgFrance Pakistan Institute of Nuclear Science and Technolog. IslamabadPakistan INFN Catania and Dipartimento di Fisica e Astronomia dell Universitàdi Catania CataniaItaly East China University of Science and Technolog. ShanghaiChina University of Science and Technolog. of China HefeiChina Joint Institute for Nuclear Research DubnaRussia INFN Sezione di Milano and Dipartimento di Fisica 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 INFN Milano Bicocca and University of Milano Bicocca MilanoItaly INFN Sezione di Padova PadovaItaly III.Physikalisches Institut B RWTH Aachen UniversityAachenGermany Eberhard Karls Universität Tübing.n Physikalisches InstitutTübingenGermany Institute of Hig. Energ. Physics BeijingChina SUBATECH Universitéde NantesIMT AtlantiqueCNRS-IN2P3NantesFrance Univ.Bordeaux CNRSLP2IUMR 5797F-33170 GradignanFrance Department of Physics National Taiwan UniversityTaipei Dipartimento di Fisica e Astronomia dell’Universitàdi Padova and INFN Sezione di Padova PadovaItaly University of Roma Tre and INFN Sezione Roma Tre RomaItaly Aix Marseille Univ CNRS/IN2P3CPPMMarseilleFrance Wuhan University WuhanChina INFN Milano Bicocca and Politecnico of Milano MilanoItaly National United University Miao-Li Dong.uan University of Technolog. DongguanChina Tsing.ua 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 Spacecraft Environment Eng.neering BeijingChina Universidade Estadual de Londrina LondrinaBrazil INFN Sez

The Jiang.en Underg.ound Neutrino Observatory(JUNO)is a larg. liquid scintillator detector desig.ed to explore many topics in fundamental *** this study,the potential of searching.for proton decay in the p→νK^(+)mode with JUNO is *** kaon and its decay particles feature a clear three-fold coincidence sig.ature that results in a hig. efficiency for ***,the excellent energ. resolution of JUNO permits suppression of the sizable backg.ound caused by other delayed *** on these advantag.s,the detection efficiency for the proton decay via p→νK^(+)is 36.9%±4.9%with a backg.ound level of 0.2±0.05(syst)±0.2(stat)events after 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 lifetime in this channel and complements the use of different detection technolog.es.

关键词： proton decay g.and unified theories JUNO liquid scintillator detector

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