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鏡湖醫院急診科“ACS快速通道”執行現狀分析

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镜湖医学 2015年第1期15卷 16-20页

作者：王惠儀盧正烽梁俊鏗施養育澳門鏡湖醫院急診科中國

目的以"Door-to-Door"時間為指標,評價本院急性冠脈綜合症(ACS)快速通道的執行狀況,分析ACS患者行介入治療延誤的原因並提出相關改善措施,提高快速通道的執行率。方法對本院2010年9月~2012年03月期間,經急診診斷ACS並進行經皮冠脈介入治... 详细信息

目的以"Door-to-Door"時間為指標,評價本院急性冠脈綜合症(ACS)快速通道的執行狀況,分析ACS患者行介入治療延誤的原因並提出相關改善措施,提高快速通道的執行率。方法對本院2010年9月~2012年03月期間,經急診診斷ACS並進行經皮冠脈介入治療(PCI)患者作回顧性分析。記錄患者自急診掛號就診,再經會診確定需行PCI,至出急診送往導管室的各段時間,簡稱急診進門-出門時間(Door to Door time,D2D)。將D2D以60min為界線,分為D2D≦60min組及D2D>60min組。監測D2D、心電圖時間、心電圖識別時間的達標率。對餘下的組成環節作兩兩對比,找出導致D2D延誤的組成環節、延誤原因。結果所收集啟動“ACS快速通道”接受的患者有103例。中位急診進門-出門時間是94min。D2D≦60min組有22例,達標率為21.4%(22/103)。急診判讀心電圖、急診總住院醫生、內科醫生、家屬商議時間、導管室準備等為主要延誤環節。結論D2D達標率的改善有很大的空間。通過加強急診科醫生培訓、改革導管室的啓動方式、完善導管室及人員配置、普及醫學知識的推廣教育可以縮短D2D時間。

关键词：急性冠脈綜合症快速通道進門-出門時間門-囊時間延誤原因

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

硬膜外鎮痛對不同孕期增重初產婦分娩結局的影響

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镜湖医学 2023年第1期23卷 36-38页

作者：李濤羅英浛廖婧潘慧王美冰曹麗勤澳門鏡湖醫院麻醉科中國澳門

目的探討硬膜外分娩鎮痛(LEA)與不同孕期增重(GWG)初產婦分娩結局的關係。方法回顧分析經陰道分娩的共801位產婦分娩記錄。以GWG正常、孕期超重及是否接受LEA將其分為四組。Ⅰ組:GWG正常不接受LEA。Ⅱ組:GWG正常接受LEA。Ⅲ組:孕期超重... 详细信息

目的探討硬膜外分娩鎮痛(LEA)與不同孕期增重(GWG)初產婦分娩結局的關係。方法回顧分析經陰道分娩的共801位產婦分娩記錄。以GWG正常、孕期超重及是否接受LEA將其分為四組。Ⅰ組:GWG正常不接受LEA。Ⅱ組:GWG正常接受LEA。Ⅲ組:孕期超重不接受LEA。Ⅳ組:孕期超重接受LEA。分別記錄孕婦分娩方式、產程時間、出血量、新生兒體重、新生兒Apgar評分、產婦的鎮痛時間和順產率等。結果GWG正常產婦中,接受LEA組產婦的第一、二產程時間均長於無LEA產婦;GWG超重產婦中,接受LEA的產婦第二產程時間明顯長於無LEA產婦,其順產率顯著高於無LEA組。GWG正常且接受LEA組產婦所產新生兒的5min Apgar評分顯著低其他三組。結論產婦順產率與GWG無關。雖然接受LEA產婦的產程延長,但其順產率明顯升高。所以,對於所有初產婦,尤其對於GWG超重初產婦,值得推廣LEA。

关键词：孕期增重分娩鎮痛順產率

經內鏡支架置入聯合腹腔鏡手術治療左側大腸癌性梗阻的臨床價值

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镜湖医学 2017年第2期17卷 55-57页

作者：羅光輝朱文立何家駒余漢濠黃炳紅澳門鏡湖醫院普外科中国澳門鏡湖醫院消化内科中国

目的探討運用術前腸道支架減壓聯合腹腔鏡手術,在治療梗阻性左側大腸癌Ⅰ期切除吻合術中的安全性和有效性。方法回顧性分析中国澳門鏡湖醫院胃腸外科2015年3月~2017年6月期間梗阻性左側大腸癌16例患者資料,術前行結腸鏡下腸道支架置入... 详细信息

目的探討運用術前腸道支架減壓聯合腹腔鏡手術,在治療梗阻性左側大腸癌Ⅰ期切除吻合術中的安全性和有效性。方法回顧性分析中国澳門鏡湖醫院胃腸外科2015年3月~2017年6月期間梗阻性左側大腸癌16例患者資料,術前行結腸鏡下腸道支架置入解除腸梗阻,10~14d後行腹腔鏡下大腸癌根治性切除術。結果16例患者腹腔鏡手術成功,1例因腫瘤侵犯左側輸尿管而中轉開腹;手術時間170~280mi n,平均210m in;術後腸功能恢復時間2~5d,平均3d;無吻合口漏發生。結論術前腸道支架減壓聯合腹腔鏡Ⅰ期手術是治療梗阻性左側大腸癌安全有效的方法。

关键词：大腸癌腸梗阻腸道支架腹腔鏡

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

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

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