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圖像引導放療糾正肺癌擺位誤差頻率研究

镜湖医学 2015年第2期15卷 44-47页

作者：丘熹彬李田芊肖光莉吳釗平朱向尚王漢陽龍慧娟黃積韻黃美云澳門鏡湖醫院腫瘤科中國

目的分析本院放療中心肺癌擺位誤差分佈規律,為明確本科所需圖像引導放療频率提供参考依據。方法回顧性分析本科近5年來167例肺癌放療患者的擺位誤差,分析不同精度擺位誤差分佈的規律。結果左右、腹背、頭脚方向,≤2mm的摆位誤差出現的... 详细信息

目的分析本院放療中心肺癌擺位誤差分佈規律,為明確本科所需圖像引導放療频率提供参考依據。方法回顧性分析本科近5年來167例肺癌放療患者的擺位誤差,分析不同精度擺位誤差分佈的規律。結果左右、腹背、頭脚方向,≤2mm的摆位誤差出現的频率分別為71%、82%、64%,大於5m m的摆位誤差出現的频率分別為4%、2%、5%。大於5m m的摆位誤差高度集中於少數身體精神狀態差的患者。結論本科擺位精度較高,非迫切需要借助每天IgRT糾正擺位誤差。如患者首三次放療,擺位誤差誤差≤2mm,可沿用目前的IgRT頻率;如患者首三次放療,摆位誤差大於5mm,建議每次放療前行IgRT。IgRT如需每日進行,建議採用二维照片的形式。

关键词：肺癌圖像引導放療治療擺位誤差

儿童新型冠状病毒感染诊断、治疗和预防专家共识(第四版)

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中华实用儿科临床杂志 2022年第14期37卷 1053-1065页

作者：蒋荣猛谢正德姜毅陆小霞金润铭郑跃杰尚云晓徐保平刘智胜卢根邓继岿刘光华王晓川王建设冯录召刘薇郑毅舒赛男陆敏罗万军刘苗崔玉霞叶乐平申阿东刘钢高立伟熊莉娟白燕林丽开魏庄薛凤霞王天有赵东赤赵正言邵剑波吴国强黄永坚李兴旺杨永弘申昆玲首都医科大学附属北京地坛医院感染性疾病诊疗中心北京100015 国家儿童医学中心(北京) 首都医科大学附属北京儿童医院北京市儿科研究所中国医学科学院儿童危重感染诊治创新单元国家呼吸系统疾病临床医学研究中心儿科重大疾病研究教育部重点实验室儿童呼吸道感染性疾病研究北京市重点实验室北京100045 武汉大学人民医院儿科武汉430060 华中科技大学同济医学院附属武汉儿童医院呼吸科武汉430016 华中科技大学同济医学院附属协和医院儿科武汉430022 深圳市儿童医院呼吸科深圳518038 中国医科大学附属盛京医院小儿呼吸内科沈阳110004 国家儿童医学中心(北京) 国家呼吸系统疾病临床医学研究中心首都医科大学附属北京儿童医院呼吸科北京100045 华中科技大学同济医学院附属武汉儿童医院神经内科武汉430016 广州市妇女儿童医疗中心呼吸科广州510623 深圳市儿童医院感染科深圳518038 上海儿童医学中心福建医院福建省儿童医院儿科福州350005 国家儿童医学中心(上海) 复旦大学附属儿科医院临床免疫/过敏科上海201102 国家儿童医学中心(上海) 复旦大学附属儿科医院感染传染科上海201102 中国医学科学院北京协和医学院群医学及公共卫生学院北京100730 天津大学儿童医院天津市儿童医院天津300134 首都医科大学附属北京安定医院国家精神心理疾病临床医学研究中心精神疾病诊断与治疗北京市重点实验室北京100088 华中科技大学同济医学院附属同济医院儿科武汉430030 上海市儿童医院呼吸科上海200062 华中科技大学同济医学院附属武汉儿童医院感染管理办公室武汉430016 贵州省人民医院儿科贵阳550002 北京大学第一医院儿科北京100034 国家儿童医学中心(北京) 国家呼吸系统疾病临床医学研究中心首都医科大学附属北京儿童医院北京市儿科研究所北京100045 国家儿童医学中心(北京) 首都医科大学附属北京儿童医院感染科北京100045 华中科技大学同济医学院附属协和医院感染性疾病科武汉430022 武汉大学中南医院武汉大学医院管理研究所武汉430071 国家儿童医学中心(北京) 首都医科大学附属北京儿童医院儿童保健中心北京100045 国家儿童医学中心(北京) 首都医科大学附属北京儿童医院血液肿瘤中心北京100045 武汉大学中南医院儿科武汉430071 浙江大学医学院附属儿童医院发育行为科杭州310051 华中科技大学同济医学院附属武汉儿童医院放射影像中心武汉430016 香港养和医院儿科中国香港999077 香港中文大学威尔斯亲王医院儿科中国香港999077

自2019年12月以来,新型冠状病毒(SARS-CoV-2)感染在全球肆虐已2年余。我国始终采取科学有效的防控措施并取得一定成功,但随着SARS-CoV-2的不断变异和境外输入病例,导致疫情防控工作更加艰巨、复杂。随着变异株的变化,儿童病例数量也出... 详细信息

自2019年12月以来,新型冠状病毒(SARS-CoV-2)感染在全球肆虐已2年余。我国始终采取科学有效的防控措施并取得一定成功,但随着SARS-CoV-2的不断变异和境外输入病例,导致疫情防控工作更加艰巨、复杂。随着变异株的变化,儿童病例数量也出现了变化,并且出现了一些新的特殊症候和并发症,这为我国儿童SARS-CoV-2感染的防治提出了新的课题。本共识在《儿童新型冠状病毒感染诊断、治疗和预防专家共识(第三版)》的基础上,根据新变异株的特点,对其病原学、病理学、发病机制等进行阐述,总结儿童病例的临床特点和诊疗经验,就儿童病例实验室检查、诊断、治疗和防控等提出建议,为进一步加强对我国儿童SARS-CoV-2感染的防治提供参考。

关键词：新型冠状病毒感染儿童诊断治疗预防共识

家蚕(Bombyx mori)全基因组框架图

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蚕学通讯 2008年第4期28卷 1-16页

作者：夏庆友周泽扬鲁成程道军代方银李斌赵萍查幸福程廷才柴春利潘国庆许金山刘春林英钱吉凤侯勇吴正理李关荣潘敏慧李春峰沈以红蓝希钳袁联伟李田徐汉福杨光伟万永继朱勇余茂德沈卫德吴大洋向仲怀于军王俊李瑞强石剑萍李恒李光远苏建宁王晓玲李国庆张增金吴清发李俊张庆鹏韦宁徐建哲孙海波董乐刘东源赵胜利赵晓兰孟庆顺兰锋镝黄显刚李源哲方林李昌锋李大为孙永巧张振鹏杨峥黄艳清奚艳亓秋辉贺丹丹黄海燕张晓伟王智强李文杰曹玉竹余迎朴俞鸿李金宏叶杰华陈欢周雁刘斌王晶叶葭纪海李胜霆倪培相张建国张勇郑洪坤毛炳宇王文叶辰李松岗汪建 gane Ka-Shu wong 杨焕明西南大学北京中国科学院基因组研究所北京基因组研究所北京蛋白质组研究所浙江大学基因组科学James D.Watson研究所杭州基因组研究所浙江省生物信息学重点实验室华盛顿大学基因组中心华盛顿大学医学院

我们在此报告了家蚕(Bombyx mori)的基因组序列框架图,它覆盖了所有已知家蚕基因的90.9%。我们估计的基因数是18510,超过黑腹果蝇报道的13379个基因。我们将家蚕基因组与果蝇、蚊子、蜘蛛和蝴蝶等进行了比较分析,揭示了它们在基因组成... 详细信息

我们在此报告了家蚕(Bombyx mori)的基因组序列框架图,它覆盖了所有已知家蚕基因的90.9%。我们估计的基因数是18510,超过黑腹果蝇报道的13379个基因。我们将家蚕基因组与果蝇、蚊子、蜘蛛和蝴蝶等进行了比较分析,揭示了它们在基因组成上同时具有相似性和差异性。

关键词：全基因组框架图家蚕黑腹果蝇基因组序列基因组成基因数差异性

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

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

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： Angel Abusleme Thomas Adam Shakeel Ahmad Rizwan Ahmed Sebastiano Aiello Muhammad Akram 安丰鹏安琪 giuseppe Andronico Nikolay Anfimov 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 Birkenfeld 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 Conforti Di Lorenzo Daniele Corti Flavio Dal Corso Olivia Dalager Christophe De La Taille 邓智邓子艳 Wilfried Depnering Marco Diaz Xuefeng Ding 丁雅韵 Bayu Dirgantara Sergey Dmitrievsky Tadeas Dohnal Dmitry Dolzhikov georgy Donchenko 董建蒙 Evgeny 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 Fargetta Dmitry Fedoseev Li-Cheng Feng 冯启春 Richard Ford Amélie Fournier 甘浩男 Feng gao Alberto garfagnini 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 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 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 Pontificia Universidad Católica de Chile SantiagoChile IPHC Universitéde StrasbourgCNRS/IN2P3F-67037 StrasbourgFrance Pakistan Institute of Nuclear Science and Technology IslamabadPakistan INFN Catania and Dipartimento di Fisica e Astronomia dell Universitàdi Catania CataniaItaly East China University of Science and Technology ShanghaiChina University of Science and Technology 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 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 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 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 Spacecraft Environment Engineering BeijingChina Universidade Estadual de Londrina LondrinaBrazil INFN Sez

The Jiangmen Underground Neutrino Observatory(JUNO)is a large liquid scintillator detector designed 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 signature that results in a high efficiency for ***,the excellent energy resolution of JUNO permits suppression of the sizable background caused by other delayed *** on these advantages,the detection efficiency for 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 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 technologies.

关键词： proton decay grand unified theories JUNO liquid scintillator detector