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Efficacy of pegylated interferon-alpha-2a plus ribavirin for patients aged at least 60 years with chronic hepatitis C

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chinese Medical Journal 2012年第11期125卷 1852-1856页

作者： ZHENG ying-ying fan xiao-hong wang li-feng TIAN Di huo na lu hai-ying wu chi-hong xu xiao-yuan WEI Lai Department of Infectious Diseases Peking University First Hospital Beijing 100034 China Hepatology Institute Peking University People＇s Hospital Beijing 100044 China

Background In china, patients with hepatitis C virus （HCV）-associated liver disease are getting older, and thus the number of deaths due to such disease is increasing. The efficacy of combination therapy with ribavirin and interferon for chronic HCV infection in elderly patients has not been fully clarified. The aim of the present study was to evaluate the efficacy and tolerability of the combination therapy in the elderly patients. Methods Sixty-eight chronic hepatitis C patients, who received the combination therapy, were classified into two age groups： elderly group （〉60 years, n=25） and non-elderly group （〈60 years, n=43）. Rapid virological response, complete early virological response, sustained virological response, relapse, non-response rate, and safety were compared between the elderly group and non-elderly group. Results Overall sustained virological response was lower in the elderly group than non-elderly group （44% vs. 75%, P=0.012, OR=0.270, and 95% CI 0.095-0.768）. Among patients with HCV genotype 1, sustained virological response was lower in the elderly group than non-elderly group （45% vs. 77%, P=0.015, OR=0.247, 95% CI 0.078-0.781）. The proportions of dose reduction due to laboratory abnormalities were significantly higher in the elderly group than non-elderly group （60.0% vs. 32.6%, P=0.027）. Multiple binary Logistic regression analysis confirmed that patient age was an associated factor for sustained virological response. Conclusion Among patients with HCV genotype 1, the elderly patients had lower sustained virological response than non-elderly patients during pegylated interferon-alpha-2a plus ribavirin combination therapy.

关键词： interferon, therapeutics, hepatit& C aged

CEPC Technical Design Report

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Radiation Detection Technology and Methods 2024年第1期8卷 I0003-I0016,1-1091页

作者： Waleed Abdallah Tiago Carlos Adorno de Freitas Konstantin Afanaciev Shakeel Ahmad Ijaz Ahmed xiaocong Ai Abid Aleem Wolfgang Altmannshofer Fabio Alves Weiming An Rui An Daniele Paolo Anderle Stefan Antusch Yasuo Arai Andrej Arbuzov Abdesslam Arhrib Mustafa Ashry Sha Bai Yu Bai Yang Bai Vipul Bairathi Csaba Balazs Philip Bambade Yong Ban Tripamo Bandyopadhyay Shou-shan Bao Desmond P.Barber Ayse Bat Varvara Batozskaya Subash Chandra Behera Alexander Belyaev Michele Bertucci xiao-Jun Bi yuanjie Bi Tianjian Bian Fabrizio Bianchi Thomas Biekotter Michela Biglietti Shalva Bilanishvili Deng Binglin Denis Bodrov Anton Bogomyagkov Serge Bondarenko Stewart Boogert Maarten Boonekamp Marcello Borri Angelo Bosotti Vincent Boudry Mohammed Boukidi Igor Boyko Ivanka Bozovic Giuseppe Bozzi Jean-Claude Brient Anastasiia Budzinskaya Masroor Bukhari Vladimir Bytev Giacomo Cacciapaglia Hua Cai Wenyong Cai wujun Cai Yijian Cai Yizhou Cai Yuchen Cai haiying Cai Huacheng Cai Lorenzo Calibbi Junsong Cang Guofu Cao Jianshe Cao Antoine Chance xuejun Chang Yue Chang Zhe Chang Xinyuan Chang Wei Chao Auttakit Chatrabhuti Yimin Che Yuzhi Che Bin Chen Danping Chen Fuqing Chen Fusan Chen Gang Chen Guoming Chen Hua-Xing Chen Huirun Chen Jinhui Chen Ji-yuan Chen Kai Chen Mali Chen Mingjun Chen Mingshui Chen Ning Chen shanhong Chen shanzhen Chen Shao-Long Chen Shaomin Chen Shiqiang Chen Tianlu Chen Wei Chen Xiang Chen xiaoyu Chen Xin Chen xun Chen xurong Chen Ye Chen ying Chen Yukai Chen Zelin Chen Zilin Chen Gang Chen Boping Chen Chunhui Chen Hok Chuen Cheng Huajie Cheng shan Cheng Tongguang Cheng Yunlong chi Pietro chimenti Wen Han chiu Guk Cho Ming-Chung Chu xiaotong Chu Ziliang Chu Guglielmo Coloretti Andreas Crivellin Hanhua Cui xiaohao Cui Zhaoyuan Cui Brunella D'Anzi ling-Yun Dai Xinchen Dai xuwen Dai Antonio De Maria Nicola De Filippis Christophe De La Taille Francesca De Mori chiara De Sio Elisa Del Core Shuangxue Deng Wei-Tian Deng Zhi Deng Ziyan Deng Bhupal Dev Tang Dewen Biagio Di Micco Ran Ding Siqin Dingl Yadong Ding haiyi Dong Jianin AGH University of Science and Technology Faculty of Physics and Applied Computer ScienceKrakow Anhui University HefeiAnhui Applied Physics Department Federal Urdu University of ArtsScience and TechnologyIslamabad Banaras Hindu University Institute of ScienceVaranasi Bandirma Onyedi Eylul University Bandirma Beihang University Beijing Beijing Computational Science Research Center Beijing Beijing Conveyi LTD Beijing Beijing Glass Research Institute Co. LtdBeijing Beijing Institute of Technology Beijing Beijing Normal University Beijing Brown University ProvidenceRI Budker Institute of Nuclear Physics Novosibirsk Cadi Ayyad University Laboratory of Fundamental and Applied PhysicsPolydisciplinary FacultyMarrakech Cairo University Giza Center for Theory and Computation National Tsing Hua UniversityHsinchu Central china Normal University WuhanHubei Central South University ChangshaHunan Centro de Fisica Teorica de Particulas Universidade Tecnica de LisboaLisboa Chengdu KaitengSifang Digital Radio&TV Equipment Co. LtdChengduSichuan china academy of engineering physics MianyangSichuan china building materials academy Beijing china Center of Advanced Science and Technology Beijing china Institute of Atomic Energy Beijing china Jiliang University HangzhouZhejiang china Nuclear Instrument CO. LTDBeijing china University of Geosciences Beijing china University of Geosciences WuhanHubei china University of Mining and Technology XuzhouJiangsu china West Normal University NanchongSichuan Chongqing University Department of PhysicsChongqing Chulalongkorn University Bangkok City University of hong Kong Department of PhysicsHong Kong Cockcroft Institute Daresbury Cornell University IthacaNY CPPM(AMU/IPhU&CNRS/INP) Marseille Dalian Minzu University DalianLiaoning Dalian University of Technology Department of PhysicsDalian Deutsches Elektronen-Synchrotron DESY Hamburg Dzhelepov Laboratory of Nuclear Problems of Joint Institute for Nuclear Research(DLNP JINR) Dubna East china University Of Science And Technol

The Circular Electron Positron Collider(CEPC)is a large scientific project initiated and hosted by china,fostered through extensive collaboration with international *** complex comprises four accelerators:a 30 GeV linac,a 1.1 GeV Damping Ring,a Booster capable of achieving energies up to 180 GeV,and a Collider operating at varying energy modes(Z,W,H,and tt).The linac and Damping Ring are situated on the surface,while the subterranean Booster and Collider are housed in a 100 km circumference underground tunnel,strategically accommodating future expansion with provisions for a potential Super Proton Proton Collider(SPPC).The CEPC primarily serves as a Higgs *** its baseline design with synchrotron radiation(SR)power of 30 MW per beam,it can achieve a luminosity of 5×10^(34)cm^(-2)s^(-1)per interaction point(IP),resulting in an integrated luminosity of 13 ab^(-1)for two IPs over a decade,producing 2.6 million Higgs *** the SR power to 50 MW per beam expands the CEPC's capability to generate 4.3 million Higgs bosons,facilitating precise measurements of Higgs coupling at sub-percent levels,exceeding the precision expected from the HL-LHC by an order of *** Technical Design Report(TDR)follows the Preliminary Conceptual Design Report(Pre-CDR,2015)and the Conceptual Design Report(CDR,2018),comprehensively detailing the machine's layout,performance metrics,physical design and analysis,technical systems design,R&D and prototyping efforts,and associated civil engineering ***,it includes a cost estimate and a preliminary construction timeline,establishing a framework for forthcoming engineering design phase and site selection *** is anticipated to begin around 2027-2028,pending government approval,with an estimated duration of 8 *** commencement of experiments and data collection could potentially be initiated in the mid-2030s.

关键词： initiated exceeding precise

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慢性丙型肝炎患者的糖代谢异常及其危险因素

首都医科大学学报 2009年第6期30卷 791-794页

作者：王力芬张爱秋单媛霍娜陆海英吴赤红徐小元北京大学第一医院感染疾病科河北省玉田县医院感染疾病科

目的明确慢性丙型肝炎患者糖代谢异常(空腹血糖升高与Ⅱ型糖尿病)的发生率,探讨其临床特征及相关危险因素。方法用荧光定量聚合酶链反应(fluorogenic quantitative polymerase chain reaction,PCR)法对152例慢性丙型肝炎(chronic hepati... 详细信息

目的明确慢性丙型肝炎患者糖代谢异常(空腹血糖升高与Ⅱ型糖尿病)的发生率,探讨其临床特征及相关危险因素。方法用荧光定量聚合酶链反应(fluorogenic quantitative polymerase chain reaction,PCR)法对152例慢性丙型肝炎(chronic hepatitis C,CHC)(其中54例合并丙型肝炎性肝硬化)患者与82例慢性乙型肝炎(chronic hepatitis B,CHB)(其中30例合并乙型肝炎性肝硬化)患者进行血清丙型肝炎病毒(hepatitis Cvirus,HCV)Rna和HCV基因型的检测。将肝硬化患者按child-pugh分级标准分为child A、B、C3组。比较CHC与CHB2组患者Ⅱ型糖尿病发病率的差异,探讨HCV感染易发生糖代谢异常的相关危险因素。结果①CHC患者空腹血糖升高的发生率为24.8%,Ⅱ型糖尿病发病率为19.2%,肝硬化患者合并Ⅱ型糖尿病的发病率为25.9%;childpugh A、B、C3型患者分别为17.4%,29.2%和42.9%。②CHB患者的Ⅱ型糖尿病发生率为9.7%,肝硬化患者占6.7%,childpugh A、B、C3型患者分别为0%,0%和6.7%。③CHC患者Ⅱ型糖尿病发生率高于CHB患者,差异有统计学意义(P<0.01)。④多元回归分析表明,基因1b型、年龄、高血压、肝硬化是慢性丙型肝炎患者合并Ⅱ型糖尿病的危险因素(P<0.01)。结论CHC患者易发生糖代谢异常,是否合并Ⅱ型糖尿病与基因1b型、肝硬化、高血压和年龄相关。

关键词：丙型肝炎病毒糖尿病基因型肝硬化患者糖代谢异常相关危险因素发生率胰岛素抵抗慢性乙型肝炎荧光定量聚合酶链反应

Timing analysis of the black hole candidate EXO 1846–031 with Insight-HXMT monitoring

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Research in Astronomy and Astrophysics 2021年第3期21卷 193-204页

作者： He-Xin liu Yue Huang Guang-Cheng xiao Qing-Cui Bu Jin-lu Qu Shu Zhang Shuang-nan Zhang Shu-Mei Jia fang-Jun lu Xiang Ma lian Tao Wei Zhang li Chen li-Ming Song Ti-Pei li Yu-Peng xu xue-Lei Cao Yong Chen Cong-Zhan liu Ce Cai Zhi Chang Gang Chen Tian-Xiang Chen Yi-Bao Chen Yu-Peng Chen Wei Cui Wei-Wei Cui Jing-Kang Deng Yong-Wei Dong yuan-yuan Du Min-xue Fu Guan-Hua Gao He Gao Min Gao Ming-Yu Ge Yu-Dong Gu Ju Guan Cheng-Cheng Guo Da-Wei Han Jia huo lu-Hua Jiang Wei-Chun Jiang Jing Jin Yong-Jie Jin ling-Da Kong Bing li Cheng-Kui li Gang li Mao-Shun li Wei li Xian li xiao-Bo li xu-fang li Yang-Guo li Zheng-Wei li xiao-Hua liang Jing-yuan liao Bai-Sheng liu Guo-Qing liu hong-Wei liu xiao-Jing liu Yi-Nong liu Bo lu xue-feng lu Qi luo Tao luo Bin Meng Yi nang Jian-Yin Nie Ge Ou na Sai Ren-Cheng shang Xin-ying Song liang Sun ying Tan You-li Tuo Chen wang Guo-feng wang Juan wang ling-Jun wang Weng-Shuai wang Yu-Sa wang Xiang-Yang Wen Bai-Yang wu Bo-Bing wu Mei wu Shuo xiao Shao-lin Xiong He xu Jia-Wei Yang Sheng Yang Yan-Ji Yang Yi-Jung Yang Qi-Bin Yi Qian-Qing Yin yuan You Ai-Mei Zhang Cheng-Mo Zhang fan Zhang hong-Mei Zhang Juan Zhang Tong Zhang Wan-Chang Zhang Wen-Zhao Zhang Yi Zhang Yi-Fei Zhang Yong-Jie Zhang yuan-Hang Zhang Yue Zhang Zhao Zhang Zhi Zhang Zi-liang Zhang hai-Sheng Zhao xiao-fan Zhao Shi-Jie Zheng Yao-Guang Zheng Deng-Ke Zhou Jian-feng Zhou Yu-xuan Zhu Ren-lin Zhuang Yue Zhu Key Laboratory of Particle Astrophysics Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China University of chinese Academy of Sciences Chinese Academy of SciencesBeijing 100049China Institut fur Astronomie und Astrophysik Kepler Center for Astro and Particle PhysicsEberhard Karls Universität72076 TubingenGermany Department of Astronomy Beijing Normal UniversityBeijing 100088China Department of Astronomy Tsinghua UniversityBeijing 100084China Department of Physics Tsinghua UniversityBeijing 100084China Department of Engineering Physics Tsinghua UniversityBeijing 100084China Key Laboratory of Space Astronomy and Technology National Astronomical ObservatoriesChinese Academy of SciencesBeijing 100101China College of Physics Sciences&Technology Hebei UniversityBaoding 071002Hebei ProvinceChina

We present the observational results from a detailed timing analysis of the black hole candidate EXO 1846-031 during its outburst in 2019 with the observations of Insight-HXMT,NICER and *** outburst can be classified roughly into four different ***-C quasi-periodic oscillations(QPOs)observed by NICER(about 0.1-6 Hz)and Insight-HXMT(about 0.7-8 Hz)are also reported in this ***,we study various physical quantities related to QPO *** QPO rms-frequency relationship in the energy band 1-10 keV indicates that there is a turning pointing in frequency around2 Hz,which is similar to that of GRS 1915+105.A possible hypothesis for the relationship above may be related to the inclination of the source,which may require a high inclination to explain *** relationships between QPO frequency and QPO rms,hardness,total fractional rms and count rate have also been found in other transient sources,which can indicate that the origin of type-C QPOs is non-thermal.

关键词： X-ray binaries black hole candidate QPO EXO 1846–031

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遗传性耳聋基因治疗临床指南

实用医院临床杂志 2024年第2期21卷 39-44页

作者：齐洁玉谈方志张李燕陆玲王洪阳李文妍刘闻闻付小龙贺祖宏丁小琼孙珊方巧军董耀东朱学伟童步升曹现宝郭敏范欣淼汪芹马璐张天虹于亚峰李永新樊建刚崔勇吴佩娜张宏征唐杰郭维维查定军叶放蕾何双八曹卫杨见明钱晓云赵宇孙敬武陈晓巍孙宇夏明王秋菊袁慧军冯永孔维佳杨仕明王海波高下李华伟徐磊柴人杰东南大学数字医学工程全国重点实验室附属中大医院耳鼻咽喉头颈外科生命科学与技术学院生命与健康高等研究院江苏省生物医学高新技术研究重点实验室江苏南京210096 南通大学神经再生联合创新中心江苏南通226001 北京理工大学航天中心医院神经内科生命学院北京10081 南京大学医学院附属鼓楼医院耳鼻喉头颈外科江苏省医学重点学科(实验室)江苏南京210008 中国人民解放军总医院耳鼻咽喉头颈外科医学部北京100853 听觉与平衡觉全国重点实验室北京100853 国家耳鼻咽喉疾病临床医学研究中心北京100853 聋病教育部重点实验室北京100853 聋病防治北京市重点实验室北京100853 复旦大学附属眼耳鼻喉科医院医学神经生物学国家重点实验室教育部脑科学前沿研究中心上海200031 复旦大学生物医学研究所上海200032 国家卫健委听觉医学重点实验室上海200031 复旦大学脑科学研究院和脑科学协同创新中心上海200032 山东大学山东省耳鼻喉医院耳鼻咽喉头颈外科山东济南250022 山东省耳鼻喉研究所山东济南250022 山东第一医科大学/山东省医学科学院医学科技创新中心山东济南250000 武汉大学中南医院耳鼻咽喉头颈外科湖北武汉430071 东南大学附属中大医院耳鼻咽喉头颈外科江苏南京210009 复旦大学附属眼耳鼻喉科医院耳鼻喉科上海200032 安徽医科大学第二附属医院耳鼻咽喉头颈外科安徽合肥230601 中国医科大学附属盛京医院耳鼻咽喉头颈外科辽宁沈阳110004 吉林大学中日联谊医院耳鼻咽喉头颈外科吉林长春130033 安徽医科大学第一附属医院耳鼻咽喉头颈外科安徽合肥230022 云南省第一人民医院耳鼻喉科云南昆明650032 昆明医科大学第一附属医院耳鼻喉科云南昆明650032 中国医学科学院北京协和医学院北京协和医院耳鼻咽喉科北京100730 中南大学湘雅二医院耳鼻咽喉头颈外科湖南长沙410008 南华大学衡阳医学院基础医学院细胞生物学与遗传学教研室细胞应激生物学衡阳市重点实验室湖南衡阳421001 哈尔滨医科大学附属第一医院黑龙江哈尔滨150001 苏州大学附属第一医院耳鼻咽喉科江苏苏州215006 首都医科大学附属北京同仁医院耳鼻咽喉头颈外科北京100730 四川省医学科学院·四川省人民医院/电子科技大学附属医院耳鼻咽喉头颈外科四川成都610072 广东省人民医院耳鼻咽喉头颈外科/广东省医学科学院/南方医科大学广东广州510080 南方医科大学珠江医院耳鼻咽喉头颈外科广东广州510282 空军军医大学西京医院耳鼻咽喉-头颈外科陕西西安710032 郑州大学第一附属医院耳科河南郑州450000 东南大学医学院附属南京同仁医院耳鼻咽喉头颈外科江苏南京211102 四川大学华西医院耳鼻咽喉头颈外科四川成都610041 中国科学技术大学附属第一医院耳鼻咽喉头颈外科安徽合肥230001 华中科技大学同济医学院附属协和医院耳鼻咽喉头颈外科湖北武汉430022 山东第一医科大学附属山东省立医院耳鼻咽喉科山东济南250021 山东省医学科学院医学科技创新中心山东济南250021 山东大学附属山东省立医院耳鼻咽喉科山东济南250021 国家卫生健康委耳鼻咽喉重点实验室山东济南250021 四川大学华西医院罕见病研究院四川成都6010041 南华大学衡阳医学院南华大学附属妇幼保健院湖南长沙410008 中南大学湘雅医院耳鼻咽喉头颈外科湖南长沙410008 上海人工耳蜗工程技术研究中心上海200031 东南大学深圳研究院广东深圳518063

遗传性耳聋是一种常见的遗传性疾病,新生儿的发病率为1‰~3‰。患者终身携带致病突变,导致不可逆性耳聋,至今尚无临床可用的治疗药物。在部分遗传性耳聋动物模型中,基因治疗已被证实为潜在有效的治疗方法。国内外已开展了多项遗传性耳... 详细信息

遗传性耳聋是一种常见的遗传性疾病,新生儿的发病率为1‰~3‰。患者终身携带致病突变,导致不可逆性耳聋,至今尚无临床可用的治疗药物。在部分遗传性耳聋动物模型中,基因治疗已被证实为潜在有效的治疗方法。国内外已开展了多项遗传性耳聋基因治疗的临床试验。其中,由东南大学附属中大医院牵头,联合国内多家医院成功开展的遗传性耳聋基因治疗临床试验,取得了显著的疗效,并积累了丰富的经验。为规范遗传性耳聋基因治疗并提供临床研究指导,全国多家医院的耳科专家讨论制定了遗传性耳聋基因治疗临床指南,内容涵盖了伦理审查、遗传性耳聋的诊断和入组标准、临床前准备、药物、疗效与安全性评估标准、术后言语康复等。本指南将为耳聋基因治疗的临床诊疗提供规范的理论和技术指导。

关键词：遗传性耳聋基因治疗临床指南

Overview to the Hard X-ray Modulation Telescope (Insight-HXMT) Satellite

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Science china(Physics,Mechanics & Astronomy) 2020年第4期63卷 2-19页

作者： Shuang-nan Zhang TiPei li fangJun lu liMing Song YuPeng X u CongZhan liu Yong Chen xueLei Cao QingCui Bu Zhi Chang Gang Chen li Chen TianXiang Chen YiBao Chen YuPeng Chen Wei Cui WeiWei Cui JingKang Deng YongWei Dong yuan yuan Du Minxue Fu GuanHua Gao He Gao Min Gao MingYu Ge YuDong Gu Ju Guan Can Gungor ChengCheng Guo DaWei Han Wei Hu Yue Huang Jia huo ShuMei Jia luHua Jiang WeiChun Jiang Jing Jin YongJie Jin Bing li ChengKui li Gang li MaoShun li Wei li Xian li xiaoBo li xufang li YanGuo li ZiJian li ZhengWei li xiaoHua liang Jinyuan liao GuoQing liu hongWei liu ShaoZhen liu xiaoJing liu yuan liu YiNong liu Bo lu xuefeng lu Tao luo Xiang Ma Bin Meng Yi nang JianYin Nie Ge Ou Jinlu Qu na Sai RenCheng shang Guohong Shen liang Sun ying Tan lian Tao Youli Tuo Chen wang ChunQin wang Guofeng wang HuanYu wang Juan wang WenShuai wang YuSa wang XiangYang Wen BaiYang wu BoBing wu Mei wu GuangCheng xiao Shaolin Xiong linli Yan JiaWei Yang Sheng Yang YanJi Yang QiBin Yi Bin yuan AiMei Zhang ChunLei Zhang ChengMo Zhang fan Zhang hongMei Zhang Juan Zhang Qiang Zhang ShenYi Zhangs Shu Zhang Tong Zhang WanChang Zhang Wei Zhang WenZhao Zhang Yi Zhang YiFei Zhang YongJie Zhang Yue Zhang Zhao Zhang Zhi Zhang Ziliang Zhang haiSheng Zhao xiaofan Zhao ShiJie Zheng Jianfeng Zhou Yuxuan Zhu Yue Zhu Renlin Zhuang Key Laboratory of Particle Astrophysics Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China University of chinese Academy of Sciences Beijing 100049China Department of Astronomy Tsinghua UniversityBeijing 100084China Department of Physics Tsinghua UniversityBeijing 100084China Department of Astronomy Beijing Normal UniversityBeijing 100088China Department of Engineering Physics Tsinghua UniversityBeijing 100084China national Astronomical Observatories Chinese Academy of SciencesBeijing 100101China national Space Science Center Chinese Academy of SciencesBeijing 100190China

As china’s first X-ray astronomical satellite, the Hard X-ray Modulation Telescope (HXMT), which was dubbed as Insight-HXMT after the launch on June 15, 2017, is a wide-band(1-250 ke V) slat-collimator-based X-ray astronomy satellite with the capability of all-sky monitoring in 0.2-3 Me V. It was designed to perform pointing, scanning and gamma-ray burst(GRB)observations and, based on the Direct Demodulation Method (DDM), the image of the scanned sky region can be *** we give an overview of the mission and its progresses, including payload, core sciences, ground calibration/facility, ground segment, data archive, software, in-orbit performance, calibration, background model, observations and some preliminary results.

关键词： X-and γ-ray telescopes and instrumentation neutron stars black holes X-ray binaries γ-ray bursts

Insight-HXMT observations of the first binary neutron star merger GW170817

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Science china(Physics,Mechanics & Astronomy) 2018年第3期61卷 26-33页

作者： TiPei li Shaolin Xiong Shuangnan Zhang fangJun lu liMing Song xueLei Cao Zhi Chang Gang Chen li Chen TianXiang Chen Yong Chen YiBao Chen YuPeng Chen Wei Cui WeiWei Cui JingKang Deng YongWei Dong yuanyuan Du Minxue Fu GuanHua Gao He Gao Min Gao MingYu Ge YuDong Gu Ju Guan ChengCheng Guo DaWei Han Wei Hu Yue Huang Jia huo ShuMei Jia luHua Jiang WeiChun Jiang Jing Jin YongJie Jin Bing li ChengKui li Gang li MaoShun li Wei li Xian li xiaoBo li xufang li YanGuo li ZiJian li ZhengWei li xiaoHua liang Jinyuan liao CongZhan liu GuoQing liu hongWei liu ShaoZhen liu xiaoJing liu yuan liu YiNong liu Bo lu xuefeng lu Tao luo Xiang Ma Bin Meng Yi nang JianYin Nie Ge OU Jinlu Qu na Sai liang Sun Yin Tan lian Tao WenHui Tao Youli Tuo Guofeng wang HuanYu wang Juan wang WenShuai wang YuSa wang XiangYang Wen BoBing wu Mei wu GuangCheng xiao He xu YuPeng xu linli Yan JiaWei Yang Sheng Yang YanJi Yang AiMei Zhang ChunLei Zhang ChengMo Zhang fan Zhang hongMei Zhang Juan Zhang Qiang Zhang Shu Zhang Tong Zhang Wei Zhang WanChang Zhang WenZhao Zhang Yi Zhang Yue Zhang YiFei Zhang YongJie Zhang Zhao Zhang Ziliang Zhang haiSheng Zhao Jianling Zhao xiaofan Zhao ShiJie Zheng Yue Zhu Yuxuan Zhu Changlin Zou Key Laboratory of Particle Astrophysics Institute of High Energy Physics Chinese Academy of Sciences Beijing 100049 China Department of Physics Tsinghua University Beijing 100084 China University of chinese Academy of Sciences Chinese Academy of Sciences Beijing 100049 China Department of Astronomy Beijing Normal University Beijing 100088 China Department of Engineering Physics Tsinghua University Beijing 100084 China

Finding the electromagnetic （EM） counterpart of binary compact star merger, especially the binary neutron star （BNS） merger, is critically important for gravitational wave （GW） astronomy, cosmology and fundamental physics. On Aug. 17, 2017, Advanced liGO and Fermi/GBM independently triggered the first BNS merger, GW170817, and its high energy EM counterpart, GRB 170817A, respectively, resulting in a global observation campaign covering gamma-ray, X-ray, UV, optical, IR, radio as well as neutrinos. The High Energy X-ray telescope （HE） onboard Insight-HXMT （Hard X-ray Modulation Telescope） is the unique high-energy gamma-ray telescope that monitored the entire GW localization area and especially the optical counterpart （SSS17a/AT2017gfo） with very large collection area （M000 cm2） and microsecond time resolution in 0.2-5 MeV. In addition, Insight-HXMT quickly implemented a Target of Opportunity （TOO） observation to scan the GW localization area for potential X-ray emission from the GW source. Although Insight-HXMT did not detect any significant high energy （0.2-5 MeV） radiation from GW170817, its observation helped to confirm the unexpected weak and soft nature of GRB 170817A. Meanwhile, Insight-HXMT/HE provides one of the most stringent constraints （-10-7 to 104 erg/cm2/s） for both GRB170817A and any other possible precursor or extended emissions in 0.2-5 MeV, which help us to better understand the properties of EM radiation from this BNS merger. Therefore the observation of Insight-HXMT constitutes an important chapter in the full context of multi-wavelength and multi-messenger observation of this historical GW event.

关键词： GW170817 BNS merger gravitational wave electromagnetic counterpart

Consensus statement on layout and delivery of automatic external defibrillator in china

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Journal of hainan Medical University 2020年第15期26卷 18-23页

作者： Yu Cao Song Chen Yan-fen Chai xiao-Hui Chen Yu-Guo Chen Shao-Wen Cheng Wen-Wei Cheng Bang-Han Ding Yang Deng Jie Fu Bang-Jiang fang Mai-ying fan li Gui Ping Gong Wei Guo Shu-Bin Guo liang Huang Ji-yuan Han Zhong Ji Xian-Fei Ji Xin-Cai Ji hong-xu Jin Xin-Jun Jiang wang-Xiang Jiang Jia-liang liu xiao-Ran liu Zhi liu Chuan-Zhu Lv feng lu Tan-Shi li Xin li Yong li shang-lun li Shuang-Ming li xiao-Gang li Bao-Jun li Pei-wu li Chun-Sheng li Zhi-Jun li Chang-luo li Xiang-Min li Yin-Ping li Zong-Jun lu Zu-xun lu Zhong-Qiu lu Zhi-Qian luo xiao-Xing liao Jian-Bo Lei Tao Ma Yu Ma Yue-feng Ma Qing-Bian Ma lin-Hao Ma Jun-Qi Ma Shi-nan Nie Jie-Miao Ou-Yang Peng Peng Qiao Pei Shu-Ming Pan Guo-Zhong Qing li-Jie Qin wu-ying Qiao Fei Shao Wei Song Xing-Yue Song Zhen-Ju Song Rong-Ju Sun De-Ya shang Du-Juan Sha Gui-Lan Tao Guo-Gang Tian ying-Ping Tian Jian-Guang Tian Chao-Yang Tong Zi-Ren Tang Meng-Xiong Tang Guo-Ping wu Zhi Wan Tao wang Xin wang Peng wang Zhong wang Tong wang Ri-Xing wang Yi-Xin wang xiao-Dan wang ling wu Wei Wei Hua Xiang feng xu Jun xu Jie xu Miao-Rong Xie Shuo-Gui xu Tie xu feng Yu Wen Yi li-shan Yang Shi-Jiao Yan Jin-Jian Yao Shou-Chun Yan xue-Zhong Yu Xian-Zhi Ye Xian-liang Yan Fu-Bing Zhou Rong-Bin Zhou Ming Zhou Qiang Zhou Jin Zhou Ping Zhou Chang-Ju Zhu Hua-Dong Zhu Ji-hong Zhu hong Zhang Mao Zhang Hua Zhang na Zhang Guo-Qiang Zhang Guo-Xiu Zhang Jin-Song Zhang Wen-wu Zhang Wen-Zhong Zhang Jian-feng Zhang Yi-Min Zhu Jun Zeng yuan Zheng Zhi-Jie Zheng Shen Zhao Yan Zhao Min Zhao Bin Zhao xiao-Dong Zhao xiao-Jing Zhao hong-Ke Zeng Sheng-Qiang Zou The chinese Society of Emergency Medicine Research Unit of Island Emergency Medicine Chinese Academy of Medical SciencesHainan Medical University Key Laboratory of Emergency and Trauma of Ministry of Education Hainan Medical UniversityHaikouHainanChina Emergency and Trauma College Hainan Medical UniversityHaikouHainanChina Department of Emergency Hainan Clinical Research Center for Acute and Critical DiseasesThe Second Affiliated Hospital of Hainan Medical UniversityHaikouHainanChina Key Laboratory of hainan Trauma and Disaster Rescue Key Laboratory of Trauma of hainan Medical University

*** Sudden cardiac death(SCD)refers to sudden death due to a variety of cardiac *** is manifested as a sudden loss of consciousness,cardiac arrest,and respiratory arrest and generally shows early symptoms that are atypical and not easily detected[1].According to a recent study,nearly 544000 patients suffer from SCD every year in china[2].

关键词： cardiac death respiratory

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