检索结果-南通市图书馆

维普期刊数据库博看期刊

重庆市主城区首起家庭聚集性新型冠状病毒肺炎疫情分析

在线全文

学校读者我要写书评

暂无评论

医学动物防制 2020年第10期36卷 1014-1016页

作者：黄轲张英曹培明李晓旭严晓峰田清树朱玮洁李雨婷向明利丁月旭安凤朱建锋重庆市公共卫生医疗救治中心重庆400036

目的对重庆市主城片区首起家庭聚集性新型冠状病毒肺炎(Corona Virus Disease 2019,COVID-19)疫情开展流行病学调查,总结疫情特征规律。方法按COVID-19《防控方案(第二版)》要求,开展现场流行病学调查,收集病例信息、发病诊疗过程、临... 详细信息

目的对重庆市主城片区首起家庭聚集性新型冠状病毒肺炎(Corona Virus Disease 2019,COVID-19)疫情开展流行病学调查,总结疫情特征规律。方法按COVID-19《防控方案(第二版)》要求,开展现场流行病学调查,收集病例信息、发病诊疗过程、临床表现、实验室检测、暴露史以及人群接触情况等信息,制作疫情报告诊疗经过时间轴。结果此次COVID-19疫情由输入性病例导致,共报告6例确诊病例。主要以生活方式等近距离接触方式传播,其中4例由密切接触者中筛查出。6例病例临床症状以发热、咳嗽为主;病例年龄最大70岁、最小11岁,已全部临床治愈,住院日最长39天、最短10天,平均19.3天。结论病例发现越早,越利于治疗,越利于处置疫情;密切接触者筛查可能是发现新冠病例/感染者的主要途径之一。

关键词：新型冠状病毒肺炎输入病例确诊病例密切接触者聚集性疫情分析防制

在线全文

学校读者我要写书评

暂无评论

玉米、小麦、油菜对不同光照强度处理的响应

南方农业 2023年第15期17卷 6-11页

作者：蔡欣李晓旭王青张鑫冯金钰李静四川水利职业技术学院四川成都611130 四川大学生命科学学院四川成都611230

在条件可控的培养室中,从单子叶和双子叶作物,C3和C4作物的角度考虑,培养玉米、小麦、油菜幼苗,设置700、320和200μmol·(m^(-2)·s^(-1))三种光强,分别处理1周和2周后,检测玉米、小麦、油菜幼苗的生物量、叶绿素、花青素及叶绿素荧光... 详细信息

在条件可控的培养室中,从单子叶和双子叶作物,C3和C4作物的角度考虑,培养玉米、小麦、油菜幼苗,设置700、320和200μmol·(m^(-2)·s^(-1))三种光强,分别处理1周和2周后,检测玉米、小麦、油菜幼苗的生物量、叶绿素、花青素及叶绿素荧光特性。结果表明:油菜的生物量随着光强的减弱而减少,玉米和小麦的生物量在中等光强条件下积累最多,增加光强不会影响玉米和小麦的叶绿素含量,但是却使油菜的叶绿素含量降低,玉米和小麦在生物量、叶绿素含量的积累上有相似变化,但是这两种植物幼苗的叶绿素荧光特性却不同,这说明,C3植物与C4植物,单子叶植物与双子叶植物,对光强变化的响应存在敏感性差异。

关键词：光照强度玉米小麦油菜生长叶绿素

同方期刊数据库博看期刊评论

在线全文

学校读者我要写书评

暂无评论

碧护对水稻种子萌发及幼苗生长的研究

天津农林科技 2023年第1期 1-3页

作者：李争侯海鹏王妍卿李翔胡晓旭冯学良天津市农业发展服务中心天津300061 天津市优质农产品开发示范中心天津301500

碧护是一种植物生长调节剂,为明确其对水稻种子萌发和幼苗生长的影响,试验共设6个处理,分别为清水对照(CK)、碧护用量分别为0.1、0.15、0.2、0.25、0.3 g,分别加入25 mL清水。结果表明,碧护对水稻种子发芽率、发芽势具有抑制作用,但效... 详细信息

碧护是一种植物生长调节剂,为明确其对水稻种子萌发和幼苗生长的影响,试验共设6个处理,分别为清水对照(CK)、碧护用量分别为0.1、0.15、0.2、0.25、0.3 g,分别加入25 mL清水。结果表明,碧护对水稻种子发芽率、发芽势具有抑制作用,但效果不显著;对水稻幼苗根冠比有调节作用,用量以0.15 g碧护加25 mL清水配制的溶液效果最好。

关键词：碧护水稻发芽试验

维普期刊数据库博看期刊

在线全文

学校读者我要写书评

暂无评论

《化工基础》课程开放教与学

广东化工 2018年第15期45卷 234-234页

作者：彭浩郭静徐建华高枫腾晓旭时建伟长江师范学院化学化工学院重庆408102

化工基础课程是化学专业本科学生知识结构和能力结构培养中必不可少的组成部分。本文结合长江师范学院化学化工学院的实际情况,通过对《化工基础》课程教学方式和考核方式的改革,有效地增强了学生对知识点的掌握,提高了教学质量。

关键词：开放教学教学改革教学质量

在线全文

学校读者我要写书评

暂无评论

用混凝-微电解预处理工艺处理豆制品废水

沈阳大学学报（自然科学版） 2019年第2期31卷 95-100页

作者：赵晓旭张忠懿牛青鄢继翱郭智垒余艳槟冯如萍宋雪英莆田学院环境与生物工程学院福建莆田351100 莆田学院福建省新型污染物生态毒理效应与控制重点实验室福建莆田351100 莆田学院生态环境及其信息图谱福建省高等学校重点实验室福建莆田351100 沈阳大学环境学院辽宁沈阳110044

采用混凝-微电解法作为预处理工艺,与生物处理工艺联用处理豆制品废水.实验结果表明,本实验处理豆制品废水的最佳初始pH值为3.5～4.0,混凝剂最佳选择为聚合氯化铝(PAC),其与助凝剂聚丙烯酰胺(PAM)的投放质量浓度分别为0.5 g·L^(-1)和10... 详细信息

采用混凝-微电解法作为预处理工艺,与生物处理工艺联用处理豆制品废水.实验结果表明,本实验处理豆制品废水的最佳初始pH值为3.5～4.0,混凝剂最佳选择为聚合氯化铝(PAC),其与助凝剂聚丙烯酰胺(PAM)的投放质量浓度分别为0.5 g·L^(-1)和10 mg·L^(-1),可去除废水中27.5%的COD,微电解处理效果最佳的反应时间为6 h,有效去除废水中53.6%的COD.

关键词：豆制品废水预处理混凝微电解

按照基线氧合指数诊断的中度和重度急性呼吸窘迫综合征婴幼儿的临床特点和预后比较

在线全文

学校读者我要写书评

暂无评论

中国小儿急救医学 2023年第8期30卷 561-565页

作者：方伯梁李科纯许峰陆国平任晓旭张育才靳有鹏王莹刘春峰成怡冰杨巧芝肖曙芳杨镒宇霍习敏雷智贤党红星刘霜武志远曾健生钱素云国家儿童医学中心首都医科大学附属北京儿童医院重症医学科100045 重庆医科大学附属儿童医院重症医学科 400014 复旦大学附属儿科医院重症医学科上海201102 首都儿科研究所附属儿童医院重症医学科北京100020 上海市儿童医院重症医学科 200062 山东第一医科大学附属省立医院小儿重症医学科济南250012 上海交通大学医学院附属上海儿童医学中心重症医学科 200127 中国医科大学附属盛京医院小儿急诊急救内科沈阳110004 郑州大学附属儿童医院重症医学科 450052 聊城市人民医院重症医学科 252000 昆明市儿童医院重症医学科 650034 广州妇女儿童医学中心重症医学科 510623 河北省儿童医院重症医学科石家庄050031 海南省妇女儿童医学中心重症医学科海口570206

目的分析儿童重症监护病房(PICU)内按基线氧合指数(OI)诊断中度和重度儿童急性呼吸窘迫综合征(PARDS)婴幼儿的临床特点和预后差异。方法对"肺表面活性物质治疗婴幼儿中重度ARDS疗效分析"研究所建立的临床数据库资料进行二次分析。回顾... 详细信息

目的分析儿童重症监护病房(PICU)内按基线氧合指数(OI)诊断中度和重度儿童急性呼吸窘迫综合征(PARDS)婴幼儿的临床特点和预后差异。方法对"肺表面活性物质治疗婴幼儿中重度ARDS疗效分析"研究所建立的临床数据库资料进行二次分析。回顾性比较2016年12月至2021年12月收住中国14家三级甲等医院PICU的101例按基线OI诊断的中度和重度PARDS婴幼儿在一般情况、基础疾病、OI、机械通气、肺表面活性物质应用、预后等临床资料方面的差异。结果101例患儿中,中度和重度PARDS患儿分别为55例(54.5%)和46例(45.5%)。重度组男性比例(50.0%比72.7%,P=0.019)及小儿危重病例评分[72(68,78)分比76(70,80)分,P=0.019]均显著低于中度组,而年龄、体重、致PARDS病因、基础疾病等两组比较差异无统计学意义(P>0.05)。重度组患儿高频呼吸机使用率显著高于中度组(34.8%比10.9%,P=0.004),但肺表面活性物质使用情况、液体负荷及肺部并发症比较差异无统计学意义(P>0.05)。重度组患儿24 h OI改善程度[0.26±0.33比0.04±0.34,P=0.001]和72 h OI改善程度[0.34(-0.04,0.62)比0.15(-0.14,0.42),P=0.029]均显著优于中度组,但两组患儿间的病死率、确诊PARDS后住院时间和呼吸机治疗时间等比较差异无统计学意义(P>0.05)。结论在有创机械通气的中度和重度PARDS婴幼儿中,按基线OI诊断的重度PARDS患儿治疗早期氧合改善优于中度患儿,也更可能接受高频通气治疗。基线OI并不能敏感区分此类患儿预后,并非此类患儿PARDS分度的理想指标。

关键词：儿科重症监护病房机械通气急性呼吸窘迫综合征氧合指数

在线全文

学校读者我要写书评

暂无评论

等位菜豆凝集素含量与SSR标记的关联分析

黑龙江大学自然科学学报 2023年第4期40卷 415-424页

作者：李思旋冯国军杨晓旭刘畅宋承泽闫志山李洪梅刘大军黑龙江大学生命科学学院哈尔滨150086 黑龙江大学现代农业与生态环境学院哈尔滨150086 中国农业大学园艺学院北京100091 青岛市即墨区新兴中学青岛266200

菜豆豆荚中的凝集素(Phytohaem agglutinin,PHA)是其食用过程中致使人中毒的主要因素。为探究菜豆种质资源中PHA含量差异,挖掘与PHA含量显著相关的功能标记,测定了64份菜豆品种两年中PHA含量变化,设计并筛选出60对SSR(Simple sequence r... 详细信息

菜豆豆荚中的凝集素(Phytohaem agglutinin,PHA)是其食用过程中致使人中毒的主要因素。为探究菜豆种质资源中PHA含量差异,挖掘与PHA含量显著相关的功能标记,测定了64份菜豆品种两年中PHA含量变化,设计并筛选出60对SSR(Simple sequence repeats)标记,对菜豆种质进行群体遗传结构分析,并利用TASSEL 2.1软件中的一般线性模型(Generalized linear model,GLM)对菜豆凝集素的含量性状进行关联分析。结果表明,64份菜豆品种中,2018年凝集素含量为0.015~1.564 mg·g^(-1),平均值为0.721 mg·g^(-1),2019年凝集素含量为0.041~1.850 mg·g^(-1),平均值为0.737 mg·g^(-1);60对SSR标记共检测到219个等位位点;遗传相似系数(Genetic similar cofficient,GS)为0.694时,64份菜豆种质可聚为2个类群。关联分析显示,两个等位位点与菜豆凝集素含量性状显著相关(P<0.05),对表型的变异贡献率分别为15.23%和15.05%。

关键词：菜豆凝集素 SSR 遗传多样性关联分析

维普期刊数据库博看期刊

Feasibility and physics potential of detecting ^(8)B solar neutrinos at JUNO

在线全文

学校读者我要写书评

暂无评论

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

在线全文

学校读者我要写书评

暂无评论

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