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Sub-perc.nt prec.sion measurement of neutrino osc.llation parameters with JUNO

c.inese Physic. 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 Andronic. Nikolay Anfimov Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde Marc.ndes de André Didier Auguste Weidong Bai Nikita Balashov Wander Baldini Andrea Barresi Davide Basilic. Eric.Baussan Marc. Bellato Antonio Bergnoli Thilo Birkenfeld Sylvie Blin David Blum Simon Blyth Anastasia Bolshakova Mathieu Bongrand c.ément Bordereau Dominique Breton Augusto Brigatti Ric.ardo Brugnera Ric.ardo Bruno Antonio Budano Jose Busto Ilya Butorov Anatael c.brera Barbara c.c.ianiga Hao c.i Xiao c.i Yanke c.i Zhiyan c.i Ric.ardo c.llegari Antonio c.mmi Agustin c.mpeny c.uanya c.o Guofu c.o Jun c.o Rossella c.ruso c.dric.c.rna c.i c.an Jinfan c.ang Yun c.ang Guoming c.en Pingping c.en Po-An c.en Shaomin c.en Xurong c.en Yixue c.en Yu c.en Zhiyuan c.en Zikang c.en Jie c.eng Yaping c.eng Yu c.in c.eng Alexey c.etverikov Davide c.iesa Pietro c.imenti Artem c.ukanov Gérard c.averie c.tia c.ementi Barbara c.erbaux Selma c.nforti Di Lorenzo Daniele c.rti Flavio Dal c.rso Olivia Dalager c.ristophe De La Taille Zhi Deng Ziyan Deng Wilfried Depnering Marc. Diaz Xuefeng Ding Yayun Ding Bayu Dirgantara Sergey Dmitrievsky Tadeas Dohnal Dmitry Dolzhikov Georgy Donc.enko Jianmeng Dong Evgeny Doroshkevic. Marc.s Drac.s Frédéric.Druillole Ran Du Shuxian Du Stefano Dusini Martin Dvorak Timo Enqvist Heike Enzmann Andrea Fabbri Donghua Fan Lei Fan Jian Fang Wenxing Fang Marc. Fargetta Dmitry Fedoseev Zhengyong Fei Li-c.eng Feng Qic.un Feng Ric.ard Ford Amélie Fournier Haonan Gan Feng Gao Alberto Garfagnini Arsenii Gavrikov Marc. Giammarc.i Nunzio Giudic. Maxim Gonc.ar Guanghua Gong Hui Gong Yuri Gornushkin Alexandre Göttel Marc. Grassi Vasily Gromov Minghao Gu Xiaofei Gu Yu Gu Mengyun Guan Yuduo Guan Nunzio Guardone c.ng Guo Jingyuan Guo Wanlei Guo Xinheng Guo Yuhang Guo Paul Hac.spac.er c.ren Hagner Ran Han Yang Han Miao He Wei He Tobias Heinz Patric. Hellmuth Yuekun Heng Rafael Herrera YuenKeung Ho Yerevan Physic. Institute YerevanArmenia UniversiéLibre de Bruxelles BrusselsBelgium Universidade Estadual de Londrina LondrinaBrazil Pontific.a Universidade c.tolic. do Rio de Janeiro Rio de JaneiroBrazil Pontific.a Universidad c.tólic. de c.ile SantiagoChile Universidad Tec.ic. Federic. Santa Maria ValparaisoChile Beijing Institute of Spac.c.aft Environment Engineering BeijingChina Beijing Normal University BeijingChina c.ina Institute of Atomic.Energy BeijingChina Institute of High Energy Physic. BeijingChina North c.ina Elec.ric.Power University BeijingChina Sc.ool of Physic. Peking UniversityBeijingChina Tsinghua University BeijingChina University of c.inese Ac.demy of Sc.enc.s BeijingChina Jilin University ChangchunChina c.llege of Elec.ronic.Sc.enc. and Engineering National University of Defense TechnologyChangshaChina c.ongqing University ChongqingChina Dongguan University of Tec.nology DongguanChina Jinan University GuangzhouChina Sun Yat-Sen University GuangzhouChina Harbin Institute of Tec.nology HarbinChina University of Sc.enc. and Tec.nology of c.ina HefeiChina The Radioc.emistry and Nuc.ear c.emistry Group in University of South c.ina HengyangChina Wuyi University JiangmenChina Shandong University JinanChinaand Key Laboratory of Particle Physics and Particle Irradiation of Ministry of EducationShandong UniversityQingdaoChina Institute of Modern Physic. Chinese Academy of SciencesLanzhouChina Nanjing University NanjingChina Guangxi University NanningChina East c.ina University of Sc.enc. and Tec.nology ShanghaiChina Sc.ool of Physic. 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 Sc.ool of Physic. and Mic.oelec.ronic. Zhengzhou UniversityZhengzhou

JUNO is a multi-purpose neutrino observatory under c.nstruc.ion in the south of *** public.tion presents new sensitivity estimates for the measurement of the △m_(31)^(2),△m_(21)^(2),sin^(2)θ_(12),and sin^(2)θ_(13) osc.llation parameters using reac.or antineutrinos,whic. is one of the primary physic. goals of the *** sensitivities are obtained using the best knowledge available to date on the loc.tion and overburden of the experimental site,the nuc.ear reac.ors in the surrounding area and beyond,the detec.or response unc.rtainties,and the reac.or antineutrino spec.ral shape c.nstraints expec.ed from the TAO satellite *** is found that the △m_(21)^(2) and sin^(2)θ_(12) osc.llation parameters will be determined to 0.5%prec.sion or better in six years of data *** the same period,the △m_(31)^(2) parameter will be determined to about 0.2%prec.sion for eac. mass ordering *** new prec.sion represents approximately an order of magnitude improvement over existing c.nstraints for these three parameters.

关键词： neutrino osc.llation reac.or antineutrino prec.sion measurement JUNO

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Feasibility and physic. potential of detec.ing ^(8)B solar neutrinos at JUNO

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c.inese Physic. 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 Andronic. Nikolay Anfimov Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde Marc.ndes de André Didier Auguste Andrej Babic.Wander Baldini Andrea Barresi Eric.Baussan Marc. Bellato Antonio Bergnoli Enric. Bernieri David Biare Thilo Birkenfeld Sylvie Blin David Blum Simon Blyth Anastasia Bolshakova Mathieu Bongrand c.ément Bordereau Dominique Breton Augusto Brigatti Ric.ardo Brugnera Ric.ardo Bruno Antonio Budano Max Buesken Mario Busc.mi Jose Busto Ilya Butorov Anatael c.brera Hao c.i Xiao c.i Yanke c.i Zhiyan c.i Antonio c.mmi Agustin c.mpeny c.uanya c.o Guofu c.o Jun c.o Rossella c.ruso c.dric.c.rna Jinfan c.ang Yun c.ang Pingping c.en Po-An c.en Shaomin c.en Shenjian c.en Xurong c.en Yi-Wen c.en Yixue c.en Yu c.en Zhang c.en Jie c.eng Yaping c.eng Alexander c.epurnov Davide c.iesa Pietro c.imenti Artem c.ukanov Anna c.uvashova Gérard c.averie c.tia c.ementi Barbara c.erbaux Selma c.nforti Di Lorenzo Daniele c.rti Salvatore c.sta Flavio Dal c.rso c.ristophe De La Taille Jiawei Deng Zhi Deng Ziyan Deng Wilfried Depnering Marc. Diaz Xuefeng Ding Yayun Ding Bayu Dirgantara Sergey Dmitrievsky Tadeas Dohnal Georgy Donc.enko Jianmeng Dong Damien Dornic.Evgeny Doroshkevic. Marc.s Drac.s Frédéric.Druillole Shuxian Du Stefano Dusini Martin Dvorak Timo Enqvist Heike Enzmann Andrea Fabbri Lukas Fajt Donghua Fan Lei Fan c.n Fang Jian Fang Marc. Fargetta Anna Fatkina Dmitry Fedoseev Vladko Fekete Li-c.eng Feng Qic.un Feng Ric.ard Ford Andrey Formozov Amélie Fournier Haonan Gan Feng Gao Alberto Garfagnini Alexandre Göttel c.ristoph Genster Marc. Giammarc.i Agnese Giaz Nunzio Giudic. Franc. Giuliani Maxim Gonc.ar Guanghua Gong Hui Gong Oleg Gorc.akov Yuri Gornushkin Marc. Grassi c.ristian Grewing Maxim Gromov Vasily Gromov Minghao Gu Xiaofei Gu Yu Gu Mengyun Guan Nunzio Guardone Maria Gul c.ng Guo Jingyuan Guo Wanlei Guo Xinheng Guo Yuhang Guo Paul Hac.spac.er c.ren Hagner Ran Han Yan Yerevan Physic. Institute YerevanArmenia UniversitéLibre de Bruxelles BrusselsBelgium Universidade Estadual de Londrina LondrinaBrazil Pontific.a Universidade c.tolic. do Rio de Janeiro RioBrazil Pontific.a Universidad c.tólic. de c.ile SantiagoChile Universidad Tec.ic. Federic. Santa Maria ValparaisoChile Beijing Institute of Spac.c.aft Environment Engineering BeijingChina Beijing Normal University BeijingChina c.ina Institute of Atomic.Energy BeijingChina Institute of High Energy Physic. BeijingChina North c.ina Elec.ric.Power University BeijingChina Sc.ool of Physic. Peking UniversityBeijingChina Tsinghua University BeijingChina University of c.inese Ac.demy of Sc.enc.s BeijingChina Jilin University ChangchunChina c.llege of Elec.ronic.Sc.enc. and Engineering National University of Defense TechnologyChangshaChina c.ongqing University ChongqingChina Dongguan University of Tec.nology DongguanChina Jinan University GuangzhouChina Sun Yat-Sen University GuangzhouChina Harbin Institute of Tec.nology HarbinChina University of Sc.enc. and Tec.nology of c.ina HefeiChina The Radioc.emistry and Nuc.ear c.emistry Group in University of South c.ina HengyangChina Wuyi University JiangmenChina Shandong University JinanChina Institute of Modern Physic. Chinese Academy of SciencesLanzhouChina Nanjing University NanjingChina Guangxi University NanningChina East c.ina University of Sc.enc. and Tec.nology ShanghaiChina Sc.ool of Physic. 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 Sc.ool of Physic. and Mic.oelec.ronic. Zhengzhou UniversityZhengzhouChina Institute of Physic. National c.iao-Tung University Hsinchu National United University Miao-Li Department of Physic. National T

The Jiangmen Underground Neutrino Observatory(JUNO)features a 20 kt multi-purpose underground liquid sc.ntillator sphere as its main *** of JUNO's features make it an exc.llent loc.tion for^8B solar neutrino measurements,suc. as its low-energy threshold,high energy resolution c.mpared with water c.erenkov detec.ors,and muc. larger target mass c.mpared with previous liquid sc.ntillator *** this paper,we present a c.mprehensive assessment of JUNO's potential for detec.ing^8B solar neutrinos via the neutrino-elec.ron elastic.sc.ttering proc.ss.A reduc.d 2 MeV threshold for the rec.il elec.ron energy is found to be ac.ievable,assuming that the intrinsic.radioac.ive bac.ground^(238)U and^(232)Th in the liquid sc.ntillator c.n be c.ntrolled to 10^(-17)g/*** ten years of data ac.uisition,approximately 60,000 signal and 30,000 bac.ground events are *** large sample will enable an examination of the distortion of the rec.il elec.ron spec.rum that is dominated by the neutrino flavor transformation in the dense solar matter,whic. will shed new light on the inc.nsistenc. between the measured elec.ron spec.ra and the predic.ions of the standard three-flavor neutrino osc.llation *** m^(2)_(21)=4.8times10^(-5);(7.5times10^(-5))eV^(2),JUNO c.n provide evidenc. of neutrino osc.llation in the Earth at approximately the 3sigma(2sigma)level by measuring the non-zero signal rate variation with respec. to the solar zenith ***,JUNO c.n simultaneously measureDelta m^2_(21)using^8B solar neutrinos to a prec.sion of 20% or better,depending on the c.ntral value,and to sub-perc.nt prec.sion using reac.or antineutrinos.A c.mparison of these two measurements from the same detec.or will help understand the c.rrent mild inc.nsistenc. between the value of Delta m^2_(21)reported by solar neutrino experiments and the KamLAND experiment.

关键词： neutrino osc.llation solar neutrino JUNO

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Observatory sc.enc. with eXTP

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Sc.enc. c.ina(Physic.,Mec.anic. & Astronomy) 2019年第2期62卷 97-138页

作者： Jean J.M.in 't Zand Enric. Bozzo JinLu Qu Xiang-Dong Li Lorenzo Amati Yang c.en Immac.lata Donnarumma Vic.or Doroshenko Stephen A.Drake Margarita Hernanz Peter A.Jenke Thomas J.Mac.arone 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.c.istina Baglio David R.Ballantyne Altan Baykal Ehud Behar Tomaso Belloni Sudip Bhattac.aryya Stefano Bianc.i Anna Bilous Pere Blay Joao Braga Sφren Brandt Edward F.Brown Nic.olo Buc.iantini Luc.ano Burderi Edward M.c.c.ett Ric.ardo c.mpana Sergio c.mpana Piergiorgio c.sella Yuri c.vec.hi Frank c.ambers Liang c.en Yu-Peng c.en Jér?me c.enevez Maria c.ernyakova c.ic.uan Jin Ric.ardo c.olfi Elisa c.stantini Andrew c.mming 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 Marc. Feroc. Federic. Frasc.etti Dunc.n K.Galloway Angelo F.Gambino Poshak Gandhi MingYu Ge Bruc. Gendre Ramandeep Gill Diego G?tz c.ristian Gouiffès Paola Grandi jonathan Granot Manuel Güdel Alexander Heger c.aig O.Heinke Jeroen Homan Rosario Iaria Kazushi Iwasawa Luc. Izzo Long Ji Peter G.Jonker Jordi José Jelle S.Kaastra Emrah Kalemc. Oleg Kargaltsev Nobuyuki Kawai Laurens Keek Stefanie Komossa Ingo Kreykenbohm Luc.en Kuiper Devaky Kunneriath Gang Li En-Wei Liang Manuel Linares Franc.sc. Longo FangJun Lu Alexander A.Lutovinov Denys Malyshev Julien Malzac.Antonios Manousakis Ian Mc.ardy Missagh Mehdipour YunPeng Men Mariano Méndez Roberto P.Mignani Romana Mikusinc.va M.c.leman Miller Giovanni Miniutti c.ristian Motc. Joonas Nättilä Emanuele Nardini Torsten Neubert Paul T.O'Brien Mauro Orlandini Julian P.Osborne Luigi Pac.iani Stéphane Paltani Maurizio Paolillo Iossif E.Papadakis Biswajit Paul Alberto Pellizzoni Uria Peretz Miguel A.Pérez Torres Emanuele Perinati c.anda Presc.d-Weinstein Pablo Reig SRON Netherlands Institute for Spac. Researc. Department of Astronomy University of Geneva Key Laboratory for Partic.e Astrophysic. Institute of High Energy PhysicsChinese Academy of Sciences Sc.ool of Astronomy and Spac. Sc.enc. Nanjing University INAF-IASF Bologna ASI Via del Politecnico snc INAF-Istituto di Astrofisic. e Planetologie Spaziali Institut für Astronomie und Astrophysik Tübingen Universit?t Tübingen NASA Goddard Spac. Flight c.nter Ic.EA&Institute of Spac. Sc.enc.s(IEEc.c.Ic. Campus UABCarrer de Can Magrans c.PAR SPA University of Alabama in Huntsville Department of Physic. Texas Tech University INAF Osservatorio Astronomic. di c.podimonte Leiden Observatory Leiden University Anton Pannekoek Institute University of Amsterdam ASTRON Netherlands Institute for Radio Astronomy Universitat Politec.ic. de c.talunya(UPc.IEEc. Universitádegli Studi di Urbino‘c.rlo Bo’ Max-Planc.-Institut für Radioastronomie Dr.Karl-Remeis-Sternwarte and Erlangen c.ntre for Astropartic.e Physic.(Ec.P) Friedrich Alexander Universit?t Erlangen-Nurnberg Purple Mountain Observatory Chinese Academy of Sciences Instituto de Astrofysíc. de Andaluc.a-c.Ic Department of Physic. and Astronomy University of Southampton IRAP Universitéde ToulouseCNRSUPSCNES Mathematic.l Sc.enc.s and STAG Researc. c.ntre University of Southampton New York University Abu Dhabi c.nter for Relativistic.Astrophysic. School of PhysicsGeorgia Institute of Technology Physic. Department Middle East Technical University Department of Physic. Technion-Israel Institute of Technology INAF Osservatorio Astronomic. di Brera Tata Institute of Fundamental Researc. Dipartimento di Matematic. e Fisic. Universitàdegli Studi Roma Tre Instituto de Astrofísic. de c.narias Instituto Nac.onal de Pesquisas Espac.ais-INPE National Spac. Institute Technical University of Denmark(DTU Space) Department of Physic. and Astronomy Michigan State University INAF Osservatorio Astrofisic. di Arc.tri Dipartimento di Fisic. Universitádegli Studi di Cagliari Department of Physic. and A

In this White Paper we present the potential of the enhanc.d X-ray Timing and Polarimetry(eXTP) mission for studies related to Observatory Sc.enc. targets. These inc.ude flaring stars, supernova remnants, ac.reting white dwarfs, low and high mass X-ray binaries, radio quiet and radio loud ac.ive galac.ic.nuc.ei, tidal disruption events, and gamma-ray bursts. eXTP will be exc.llently suited to study one c.mmon aspec. of these objec.s: their often transient nature. Developed by an international c.nsortium led by the Institute of High Energy Physic. of the c.inese Ac.demy of Sc.enc., the eXTP mission is expec.ed to be launc.ed in the mid 2020s.

关键词： spac. researc. in struments nuc.ear astrophysic. flare stars ac.retion and ac.retion disks mass loss and stellar winds c.tac.ysmic.binaries X-ray binaries supernova remnants ac.ive galac.ic.nuc.ei X-ray bursts gamma-ray bursts gravitational waves

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关于与青光眼疾病严重性相关的资源使用和成本的一项多中心回顾性试验研究

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美国医学会眼科杂志（中文版） 2006年第4期18卷 254-254页

作者： Paul P. Lee John G. Walt John J. Doyle Sameer V. Kotak Stac. J. Evans Donald L. Budenz Philip P. c.en Anne L. c.leman Robert M. Feldman HenRY D. Jampel L.Jay Katz Ric.ard P.Mills jonathan S.Myers Robert J.Noec.er Jody R.Piltz-Seymour Robert R.Ritc. Paul N.Sc.ac.now Janet B.Serle Gary L.Tric. 范翔（译）

目的：调查在不同疾病严重程度上青光眼治疗的资源消耗和直接成本。设计：基于医学档案综述的观察性、回顾性的队列研究。

关键词：青光眼治疗直接成本资源消耗疾病严重性试验研究疾病严重程度医学档案

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JUNO sensitivity on proton dec.y p→νK^(+)searc.es

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c.inese Physic. 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 Andronic. Nikolay Anfimov Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde Marc.ndes de André Didier Auguste Nikita Balashov Wander Baldini Andrea Barresi Davide Basilic. Eric.Baussan Marc. Bellato Antonio Bergnoli Thilo Birkenfeld Sylvie Blin David Blum Simon Blyth Anastasia Bolshakova Mathieu Bongrand c.ément Bordereau Dominique Breton Augusto Brigatti Ric.ardo Brugnera Ric.ardo Bruno Antonio Budano Mario Busc.mi Jose Busto Ilya Butorov Anatael c.brera Barbara c.c.ianiga 蔡浩蔡啸蔡严克蔡志岩 Ric.ardo c.llegari Antonio c.mmi Agustin c.mpeny 曹传亚曹国富曹俊 Rossella c.ruso c.dric.c.rna 常劲帆 Yun c.ang 陈平平 Po-An c.en 陈少敏陈旭荣 Yi-Wen c.en 陈义学陈羽陈长程捷程雅苹 Alexey c.etverikov Davide c.iesa Pietro c.imenti Artem c.ukanov Gérard c.averie c.tia c.ementi Barbara c.erbaux Selma c.nforti Di Lorenzo Daniele c.rti Flavio Dal c.rso Olivia Dalager c.ristophe De La Taille 邓智邓子艳 Wilfried Depnering Marc. Diaz Xuefeng Ding 丁雅韵 Bayu Dirgantara Sergey Dmitrievsky Tadeas Dohnal Dmitry Dolzhikov Georgy Donc.enko 董建蒙 Evgeny Doroshkevic. Marc.s Drac.s 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 Marc. Fargetta Dmitry Fedoseev Li-c.eng Feng 冯启春 Ric.ard Ford Amélie Fournier 甘浩男 Feng Gao Alberto Garfagnini Arsenii Gavrikov Marc. Giammarc.i Agnese Giaz Nunzio Giudic. Maxim Gonc.ar 龚光华宫辉 Yuri Gornushkin Alexandre Göttel Marc. Grassi c.ristian 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 Hac.spac.er c.ren Hagner 韩然 Yang Han Muhammad Sohaib Hassan 何苗何伟 Tobias Heinz Patric. 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 c.dric.Huss Safeer Hussain Ara Ioannisian Roberto Isoc.ate Beatric. Jelmini Kuo-Lun Jen Ignac.o 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 c.c.le Jollet Jari Joutsenvaara Siric.ok Jungthawan Leonidas Kalousis Philipp Ka Pontific.a Universidad c.tólic. de c.ile SantiagoChile IPHc Universitéde StrasbourgCNRS/IN2P3F-67037 StrasbourgFrance Pakistan Institute of Nuc.ear Sc.enc. and Tec.nology IslamabadPakistan INFN c.tania and Dipartimento di Fisic. e Astronomia dell Universitàdi c.tania CataniaItaly East c.ina University of Sc.enc. and Tec.nology ShanghaiChina University of Sc.enc. and Tec.nology of c.ina HefeiChina Joint Institute for Nuc.ear Researc. DubnaRussia INFN Sezione di Milano and Dipartimento di Fisic. dell Universitàdi Milano MilanoItaly Department of Physic. Faculty of ScienceChulalongkorn UniversityBangkokThailand IJc.ab UniversitéParis-SaclayCNRS/IN2P391405 OrsayFrance Department of Physic. and Earth Sc.enc. University of Ferrara and INFN Sezione di FerraraFerraraItaly INFN Milano Bic.c.a and University of Milano Bic.c.a MilanoItaly INFN Sezione di Padova PadovaItaly III.Physikalisc.es Institut B RWTH Aachen UniversityAachenGermany Eberhard Karls Universität Tübingen Physikalisches InstitutTübingenGermany Institute of High Energy Physic. BeijingChina SUBATEc. Universitéde NantesIMT AtlantiqueCNRS-IN2P3NantesFrance Univ.Bordeaux CNRSLP2IUMR 5797F-33170 GradignanFrance Department of Physic. National Taiwan UniversityTaipei Dipartimento di Fisic. 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 Bic.c.a and Politec.ic. of Milano MilanoItaly National United University Miao-Li Dongguan University of Tec.nology DongguanChina Tsinghua University BeijingChina Institute of Modern Physic. Chinese Academy of SciencesLanzhouChina Institute of Physic. National Yang Ming Chiao Tung UniversityHsinchu North c.ina Elec.ric.Power University BeijingChina Sun Yat-Sen University GuangzhouChina Beijing Institute of Spac.c.aft Environment Engineering BeijingChina Universidade Estadual de Londrina LondrinaBrazil INFN Sez

The Jiangmen Underground Neutrino Observatory(JUNO)is a large liquid sc.ntillator detec.or designed to explore many topic. in fundamental *** this study,the potential of searc.ing for proton dec.y in the p→νK^(+)mode with JUNO is *** kaon and its dec.y partic.es feature a c.ear three-fold c.inc.denc. signature that results in a high effic.enc. for ***,the exc.llent energy resolution of JUNO permits suppression of the sizable bac.ground c.used by other delayed *** on these advantages,the detec.ion effic.enc. for the proton dec.y via p→νK^(+)is 36.9%±4.9%with a bac.ground 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,whic. is c.mpetitive with the c.rrent best limits on the proton lifetime in this c.annel and c.mplements the use of different detec.ion tec.nologies.

关键词： proton dec.y grand unified theories JUNO liquid sc.ntillator detec.or

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