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Agricultural Sciences in China 2008年第12期7卷 1445-1450页

作者： li jin gao dong-sheng zhao kai yu qin xu chen-shan State Key Laboratory of Crop Biology College of Horticulture Science and Engineering Shandong Agricultural University Tai＇an271018 P.R.China

The responses of dormancy induction to illumination and the characteristics of respiratory rate were studied with the nectarine peach bud in this article. The trial was conducted with nectarine （Prunus persica var. nectariana cv. Shuguang） and involved three treatments： a short day treatment （8 h）, a long day treatment （16 h）, and the normal condition as the control. The dormancy status was determined with the growth of shoot and the sprouting ability, and the respiratory rate was mensurated with oxygen electrode. Short day treatment could induce the growth stopping of peach shoots ahead, promote the development of dormancy, and induce buds into dormancy with 21 d previous to control. Long day treatment postponed the growth stopping and the induction and development of dormancy. The respiratory rate decreased according to the development of dormancy induction. The minimum respiratory rate appeared about 7 days after the start of dormancy induction. Bud respiratory rate increased during this period and then declined and remained at low level during dormancy period. Long day reduced buds respiratory rate slightly. Short day could induce dormancy obviously, and long day postponed dormancy induction. The changes of respiratory rate were correlated with the development of dormancy induction, and the bud respiratory rate was also affected by photoperiod.

关键词： peach dormancy induction photoperiod respiratory rate

Diagnosis,treatment and prevention of severe acute respiratory syndrome coronavirus 2 infection in children:experts'consensus statement updatedforthe Omicron variant

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World Journal of Pediatrics 2024年第3期20卷 272-286页

作者： Rong-Meng Jiang Zheng-De Xie Yi Jiang Xiao-Xia Lu Run-Ming jin yue-Jie Zheng yun-Xiao shang Bao-Ping xu Zhi-sheng liu Gen Lu Ji-Kui Deng Guang-Hua liu Xiao-Chuan Wang Jian-She Wang Lu-zhao Feng Wei liu Yi Zheng Sai-Nan Shu Min Lu Wan-Jun Luo Miao liu yu-Xia Cui Le-Ping Ye A-dong Shen Gang liu li-Wei gao li-Juan Xiong Yan Bai li-kai lin Zhuang Wei Feng-Xia xue Tian-You Wang dong-Chi zhao Jian-Bo Shao Daniel Kwok-keung Ng Gary Wing-kin Wong Zheng-Yan zhao Xing-Wang li Yong-Hong Yang Kun-ling Shen Diagnosis and Treatment Center of Infectious Diseases Beijing Ditan HospitalCapital Medical UniversityBeijing 100015China Beijing Key Laboratory of Pediatric Respiratory Infection Diseases Key Laboratory of Major Diseases in ChildrenMinistry of EducationNational Clinical Research Center for Respiratory DiseasesResearch Unit of Critical Infection in ChildrenChinese Academy of Medical Sciences2019RU016Laboratory of Infection and VirologyBeijing Pediatric Research InstituteBeijing Children's HospitalCapital Medical UniversityNational Center for Children's HealthBeijing 100045China Department of Pediatrics Renmin Hospital of Wuhan UniversityWuhan 430060China Department of Respiratory Wuhan Children's HospitalTongji Medical CollegeHuazhong University of Science and TechnologyWuhan 430016China Department of Pediatrics Union HospitalTongji Medical CollegeHuazhong University of Science and TechnologyWuhan 430022China Department of Respiratory Shenzhen Children's HospitalShenzhen 518038China Department of Pediatric Respiratory Shengjing Hospital Affiliated to China Medical UniversityShenyang 110004China Department of Respiratory Beijing Children's HospitalCapital Medical UniversityNational Clinical Research Center for Respiratory DiseasesNational Center for Children's HealthBeijing 100045China Department of Neurology Wuhan Children's HospitalTongji Medical CollegeHuazhong University of Science and TechnologyWuhan 430016China Department of Respiratory Guangzhou Women and Children's Medical CenterGuangzhou 510623China Department of Infectious Diseases Shenzhen Children's HospitalShenzhen 518038China Department of Pediatrics Fujian Branch of Shanghai Children's Medical CenterFujian Children's HospitalFuzhou350005China Department of Clinical Immunology and Allergy Children's Hospital of Fudan UniversityNational Center for Children's HealthShanghai 201102China Department of Infectious Diseases Children's Hospital of Fudan UniversityNational Center for Children's Health.Shanghai

It has been more than 3 years since the novel coronavirus(SARS-CoV-2)pandemic raged *** coronavirus disease 2019(COVID-19)has greatly influenced human *** to data from the World Health Organization(WHO),there were ove... 详细信息

关键词： prevention infection statement

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

光周期处理对油桃芽休眠诱导效应及呼吸速率的影响

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中国农业科学 2009年第1期42卷 210-215页

作者：李瑾高东升于芹徐臣善赵锴山东农业大学园艺科学与工程学院/作物学国家重点实验室

【目的】分析光周期处理对油桃芽休眠诱导及发展进程的影响,并探讨休眠诱导期内桃芽呼吸速率的变化规律。【方法】以曙光油桃(Prunus persica *** ***)为材料,设置3个光周期处理:短日照(8h)、长日照(16h)和自然日照,结合测定枝梢的生长... 详细信息

【目的】分析光周期处理对油桃芽休眠诱导及发展进程的影响,并探讨休眠诱导期内桃芽呼吸速率的变化规律。【方法】以曙光油桃(Prunus persica *** ***)为材料,设置3个光周期处理:短日照(8h)、长日照(16h)和自然日照,结合测定枝梢的生长和桃芽萌芽能力界定桃芽休眠状态,利用氧电极测定桃芽呼吸速率的变化。【结果】短日照能够诱导曙光油桃新梢提前停长,使桃芽提前7d进入休眠诱导期,且促进休眠迅速向深度发展,较对照提前21d进入自然休眠期;长日照明显延迟油桃新梢停长,并且延缓桃芽休眠诱导及发展的进程。呼吸速率随着休眠诱导而降低,桃芽进入休眠诱导期7d后出现呼吸速率低谷,休眠诱导期内呼吸速率出现回升后降低并在休眠诱导期结束时维持在较低水平。另外,短日照明显减弱芽体的呼吸速率,并维持其在较低水平,长光照略使呼吸速率上升。【结论】短日照对休眠的产生具有明显诱导效应,长日照可推迟休眠诱导的发生,呼吸速率变化与休眠的诱导与发展进程相关,也与光周期有关。

关键词：桃休眠诱导光周期呼吸速率

Paired quasi-periodic pulsations of hard X-ray emission in a solar flare

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Science China(Physics,Mechanics & Astronomy) 2023年第5期66卷 195-206页

作者： Hai-sheng zhao dong li Shao-lin Xiong Yan-Qiu Zhang Yang Su Wei chen Yi zhao Xiao-Bo li Jia-Cong liu Wen-Xi Peng Rui Qiao Xin-Qiao li Xiang-Yang Wen li-Ming Song Shi-Jie Zheng Xin-Ying Song Xiao-yun zhao yue Huang Shuang-Nan Zhang Shuo Xiao Ce Cai Zheng-Hua An Can chen Gang chen Wei chen Yan-Qi Du Min gao Ke Gong dong-Ya Guo Zhi-Wei Guo Jian-Jian He Bin li Chao li Chao-Yang li Gang li Jian-Hui li Lu li qing-Xin li Yan-Guo li jing liang Xiao-Hua liang jin-yuan liao Xiao-jing liu Ya-qing liu Qi Luo Xiang Ma Bin Meng Ge Ou dong-li Shi jing-Yan Shi Gong-Xing Sun Xi-Lei Sun You-li Tuo chen-Wei Wang Hui Wang jin Wang jin-Zhou Wang Ping Wang Wen-Shuai Wang Hong Wu sheng-Lun Xie Yan-Bing xu yu-Peng xu Wang-chen xue sheng Yang Min Yao Jian-Ying Ye Qi-Bin Yi Chao-yue Zhang Da-li Zhang Fan Zhang Fei Zhang Hong-Mei Zhang kai Zhang Peng Zhang Xiao-Lu Zhang Zhen Zhang Guo-Ying zhao Shi-Yi zhao Chao Zheng Xing Zhou yue Zhu Key Laboratory for Particle Astrophysics Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China Purple Mountain Observatory Chinese Academy of SciencesNanjing 210023China University of Chinese Academy of Sciences Beijing 100049China Department of Astronomy Beijing Normal UniversityBeijing 100875China School of Computing and Artificial Intelligence Southwest Jiaotong UniversityChengdu 611756China Physics and Space Science College China West Normal UniversityNanchong 637002China Key Laboratory of Stellar and Interstellar Physics and Department of Physics Xiangtan UniversityXiangtan 411105China Institute of Astrophysics Central China Normal UniversityWuhan 430079China School of Physics Changchun University of Science and TechnologyChangchun 130022China College of Physics and Engineering Qufu Normal UniversityQufu 273165China College of Physics Sciences&Technology Hebei UniversityBaoding 071002China

We investigate high time resolution data obtained by the Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor(GECAM)during the flare event on 2022 April 21 at 01:52 *** subpeaks with durations of 4-6 s have been detected in the hard X-ray precursor phase,and the key feature is that they appear in pairs and seem like double-peak *** subpeaks are rarely observed in hard X-ray band and confirmed by the microwave obtained by Nobeyama Radio Polarimeters(NoRP)and Radio Solar Telescope Network(RSTN).While an exponential function can describe the continuum component of the time profile from the precursor to part of the impulsive *** periods of quasi-periodic pulsations(QPPs)are detected to be about 7.3 and 12.8 s for the precursor and impulsive phase,respectively,with at least 95%confidence *** paired QPPs are assumed to be double-peak QPPs and then the scenario of current loop coalescence model is found to be in good agreement with our *** precursor phase can be interpreted as the oscillating coalescence of two islands,while the impulsive phase can be interpreted as more islands to coalesce one by one to form larger islands.

关键词： solar flare QPPs loop coalescence circular-ribbon flare

Measurement of Br(n,γ)cross sections up to stellar s-process temperatures at the CSNS Back‑n

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Nuclear Science and Techniques 2023年第11期34卷 226-241页

作者： gao‑Le Yang Zhen‑dong An Wei Jiang Xian‑kai li Wei‑Wei Qiu Zheng‑Fa liao Zi‑yue Zhuang Xiao‑Ping Zhang sheng‑li chen chen‑chen Guo Er‑Xi Xiao Xiao Fang Xin‑Xiang li Xin‑Rong Hu Bing Jiang jin‑cheng Wang Jie Ren Wen Luo Zhi‑Chao Zhu Hao‑Yang Lan Zong‑Wei Cao xu Ma Ying‑Du liu Pu‑Sen Wang Yi Yang Ping Su Xian‑Gai Deng Wan‑Bing He Chun‑Wang Ma yu‑Ting Wang Zhi‑Tao Dai Peng‑qin He Ren‑Guang Tang Tao Zhou jing Wang Han Yi yue Zhang Yong‑Hao chen Rui‑Rui Fan Ke‑qing gao Qiang li Kang Sun Zhi‑Xin Tan Min‑Hao Gu Han‑Tao jing jing‑yu Tang School of Physics and Astronomy Sun Yat-sen UniversityZhuhai 519082China shanghai Institute of Applied Physics Chinese Academy of SciencesShanghai 201800China State Key Laboratory of Lunar and Planetary Sciences Macao University of Science and TechnologyMacao 999078China CNSA Macao Center for Space Exploration and Science Macao 999078China Institute of High Energy Physics Chinese Academy of SciencesBeijing 100049China Spallation Neutron Source Science Center Dongguan 523803China School of Nuclear Science and Technology University of South ChinaHengyang 421001China Sino‑French Institute of Nuclear Engineering and Technology Sun Yat-sen UniversityZhuhai 519082China University of Chinese Academy of Sciences Beijing 100049China Key Laboratory of Nuclear Data China Institute of Atomic EnergyBeijing 102413China School of Materials Science and Engineering Xiangtan UniversityXiangtan 411100China Key Laboratory of Nuclear Physics and Ion‑beam Application(MOE) Institute of Modern PhysicsDepartment of Nuclear Science and TechnologyFudan UniversityShanghai 200433China Institute of Particle and Nuclear Physics Henan Normal UniversityXinxiang 453007China School of Physics Henan Normal UniversityXinxiang 453007China Shenzhen Center Cancer hospitalChinese Academy of Medical SciencesShenzhen 518100China School of Nuclear Science and Technology University of Science and Technology of ChinaHefei 230027China

The neutron capture cross sections(n,γ)of bromine were obtained using the time-of-flight technique at the Back-n facility of the China Spallation Neutron ***γ-rays originating from neutron-induced capture events were detected using four C_(6)D_(6) *** pulse-height weighting technique and double-bunch unfolding method based on Bayesian theory were used in the data *** deductions,normalization,and corrections were carefully considered to obtain reliable measurement *** multilevel R-matrix Bayesian code SAMMY was used to extract the resonance parameters in the resolved resonance region(RRR).The average cross sections in the unresolved resonance region(URR)were obtained from 10 to 400 *** experimental results were compared with data from several evaluated libraries and previous experi-ments in the RRR and *** TALYS code was used to describe the average cross sections in the *** astrophysical Maxwell average cross sections(MACSs)of ^(79,81)Br from kT=5 to 100 keV were calculated over a sufficiently wide range of neutron *** a thermal energy of kT=30 keV,the MACS value for ^(79)Br 682±68 mb was in good agreement with the KADoNiS v1.0 recommended *** contrast,the value of 293±29 mb for ^(81)Br was substantially higher than that of the evaluated database and the KADoNiS v1.0 recommended value.

关键词： Time-of-flight technique Neutron capture cross sections Maxwell average cross sections

抗菌药物临床应用信息化辅助决策系统专家共识

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中华医院感染学杂志 2024年第12期34卷 1761-1766页

作者：高晓东张尧金文婷杜明梅陈璋璋陈佰义丁昉胡付品黄文祥李家斌李军李六亿李晓宇林丽开刘丁刘晓琳刘运喜刘正印倪语星王辉吴安华肖永红徐英春杨帆杨文杰杨小强俞云松张浩军赵彩彦赵烁卓超宗志勇李太生王贵强王明贵胡必杰复旦大学附属中山医院感染管理科上海200032 复旦大学附属中山医院感染科上海200032 中国人民解放军总医院第一医学中心疾病预防控制科北京100853 复旦大学附属中山医院药剂科上海200032 北京大学第一医院感染疾病科北京100034 复旦大学附属华山医院抗生素研究所上海200040 中国医学科学院北京协和医院感染科北京100730 中国医科大学附属第一医院感染病科辽宁沈阳110001 复旦大学附属中山医院医务处上海200032 重庆医科大学附属第一医院感染科重庆400042 江苏省人民医院感染科江苏南京210029 安徽医科大学第一附属医院感染科安徽合肥230022 北京大学第一医院感染管理科北京100034 武汉大学医院管理研究所湖北武汉430071 重庆市医院感染控制中心重庆408107 国家卫生健康委合理用药专家委员会北京100044 上海交通大学医学院附属瑞金医院感染管理科上海200025 北京大学人民医院检验科北京100044 中南大学湘雅医院感染科湖南长沙410008 浙江大学医学院附属第一医院传染病诊治国家重点实验室浙江杭州310003 中国医学科学院北京协和医学院北京协和医院检验科北京100730 天津市第一中心医院感染科天津300190 国家卫健委医院管理研究所药事管理研究部北京100044 浙江大学医学院附属邵逸夫医院感染科浙江杭州310003 甘肃省人民医院感染科甘肃兰州730099 河北医科大学第三医院感染科河北石家庄050051 国家卫生健康委医院管理研究所医疗服务与安全研究部北京100044 广州医科大学附属第一医院感染科广东广州510120 四川大学华西医院四川成都610041

目的规范我国抗菌药物临床应用信息化辅助决策系统的开发和应用,以促进我国抗菌药物管理的信息化建设.方法组织感染病学、感染防控、临床药学等抗菌药物临床应用管理小组的相关专家,在深入研究国内外抗菌药物临床应用信息化建设最新... 详细信息

目的规范我国抗菌药物临床应用信息化辅助决策系统的开发和应用,以促进我国抗菌药物管理的信息化建设.方法组织感染病学、感染防控、临床药学等抗菌药物临床应用管理小组的相关专家,在深入研究国内外抗菌药物临床应用信息化建设最新进展的基础上,结合我国临床实际需求,共同制定本共识.结果形成有关抗菌药物临床应用信息化辅助决策系统的17条专家共识.结论此专家共识供医疗机构抗菌药物临床应用管理小组在研发和应用信息系统进行临床决策支持时参考.

关键词：抗菌药物抗菌药物临床应用信息化辅助决策系统专家共识

Evidence for particle acceleration approaching PeV energies in the W51 complex

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Science Bulletin 2024年第18期69卷 2833-2841页

作者： LHAASO Collaboration Zhen Cao F.Aharonian Axikegu Y.X.Bai Y.W.Bao D.Bastieri X.J.Bi Y.J.Bi W.Bian A.V.Bukevich Q.Cao W.Y.Cao Zhe Cao J.Chang J.F.Chang A.M.chen E.S.chen H.X.chen liang chen lin chen Long chen M.J.chen M.L.chen Q.H.chen S.chen S.H.chen S.Z.chen T.L.chen Y.chen N.cheng Y.D.cheng M.Y.Cui S.W.Cui X.H.Cui Y.D.Cui B.Z.Dai H.L.Dai Z.G.Dai Danzengluobu X.Q.dong K.K.Duan J.H.Fan Y.Z.Fan J.Fang J.H.Fang K.Fang C.F.Feng H.Feng L.Feng S.H.Feng X.T.Feng Y.Feng Y.L.Feng S.Gabici B.gao C.D.gao Q.gao W.gao W.K.gao M.M.Ge L.S.Geng G.Giacinti G.H.Gong Q.B.Gou M.H.Gu F.L.Guo X.L.Guo Y.Q.Guo Y.Y.Guo Y.A.Han M.Hasan H.H.He H.N.He J.Y.He Y.He Y.K.Hor B.W.Hou C.Hou X.Hou H.B.Hu Q.Hu S.C.Hu D.H.Huang T.Q.Huang W.J.Huang X.T.Huang X.Y.Huang Y.Huang X.L.Ji H.Y.Jia K.Jia K.Jiang X.W.Jiang Z.J.Jiang M.jin M.M.Kang I.Karpikov D.Kuleshov K.Kurinov B.B.li C.M.li cheng li Cong li D.li F.li H.B.li H.C.li Jian li Jie li K.li S.D.li W.L.li W.L.li X.R.li Xin li Y.Z.li Zhe li Zhuo li E.W.liang Y.F.liang S.J.lin B.liu C.liu D.liu D.B.liu H.liu H.D.liu J.liu J.L.liu M.Y.liu R.Y.liu S.M.liu W.liu Y.liu Y.N.liu Q.Luo Y.Luo H.K.Lv B.Q.Ma L.L.Ma X.H.Ma J.R.Mao Z.Min W.Mitthumsiri H.J.Mu Y.C.Nan A.Neronov L.J.Ou P.Pattarakijwanich Z.Y.Pei J.C.Qi M.Y.Qi B.Q.Qiao J.J.qin A.Raza D.Ruffolo A.Sáiz M.Saeed D.Semikoz L.Shao O.Shchegolev X.D.sheng F.W.Shu H.C.Song yu.V.Stenkin V.Stepanov Y.Su D.X.Sun Q.N.Sun X.N.Sun Z.B.Sun J.Takata P.H.T.Tam Q.W.Tang R.Tang Z.B.Tang W.W.Tian C.Wang C.B.Wang G.W.Wang H.G.Wang H.H.Wang J.C.Wang kai Wang kai Wang L.P.Wang L.Y.Wang P.H.Wang R.Wang W.Wang X.G.Wang X.Y.Wang Y.Wang Y.D.Wang Y.J.Wang Z.H.Wang Z.X.Wang Zhen Wang Zheng Wang D.M.Wei J.J.Wei Y.J.Wei T.Wen C.Y.Wu H.R.Wu Q.W.Wu S.Wu X.F.Wu Y.S.Wu S.Q.Xi J.Xia G.M.Xiang D.X.Xiao G.Xiao Y.L.Xin Y.Xing D.R.Xiong Z.Xiong D.L.xu R.F.xu R.X.xu W.L.xu L.xue D.H.Yan J.Z.Yan T.Yan C.W.Yang C.Y.Yang F.Yang F.F.Yang L.L.Yang M.J.Yang R.Z.Yang W.X.Yang Y.H.Yao Z.G.Yao L.Q.Yin N.Yin X.H.You Z.Y.You Y.H.yu Q.yuan H.yue H.D.Zeng T.X.Zeng W.Zeng M.Zha B.B.Zhang F.Zhang H.Zhang 不详 Key Laboratory of Particle Astrophysics&Experimental Physics Division&Computing Center Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China University of Chinese Academy of Sciences Beijing 100049China TIANFU Cosmic Ray Research Center ChengduChina Dublin Institute for Advanced Studies 31 Fitzwilliam Place2 DublinIreland Max-Planck-Institut for Nuclear Physics P.O.Box 103980Heidelberg 69029Germany School of Physical Science and Technology&School of Information Science and Technology Southwest Jiaotong UniversityChengdu 610031China School of Astronomy and Space Science Nanjing UniversityNanjing 210023China Center for Astrophysics Guangzhou UniversityGuangzhou 510006China Tsung-Dao Lee Institute&School of Physics and Astronomy Shanghai Jiao Tong UniversityShanghai 200240China Institute for Nuclear Research of Russian Academy of Sciences Moscow 117312Russia Hebei Normal University Shijiazhuang 050024China University of Science and Technology of China Hefei 230026China State Key Laboratory of Particle Detection and Electronics China Key Laboratory of Dark Matter and Space Astronomy&Key Laboratory of Radio Astronomy Purple Mountain ObservatoryChinese Academy of SciencesNanjing 210023China Research Center for Astronomical Computing Zhejiang LaboratoryHangzhou 311121China Key Laboratory for Research in Galaxies and Cosmology Shanghai Astronomical ObservatoryChinese Academy of SciencesShanghai 200030China School of Physics and Astronomy Yunnan UniversityKunming 650091China Key Laboratory of Cosmic Rays(Tibet University) Ministry of EducationLhasa 850000China National Astronomical Observatories Chinese Academy of SciencesBeijing 100101China School of Physics and Astronomy(Zhuhai)&School of Physics(Guangzhou)&Sino-French Institute of Nuclear Engineering and Technology(Zhuhai) Sun Yat-sen UniversityZhuhai 519000&Guangzhou 510275GuangdongChina Institute of Frontier and Interdisciplinary Science Shandong UniversityQingdao 266237China APC UniversitéParis Cité

Theγ-ray emission from the W51 complex is widely acknowledged to be attributed to the interaction between the cosmic rays(CRs)accelerated by the shock of supernova remnant(SNR)W51C and the dense molecular clouds in the adjacent star-forming region,***,the maximum acceleration capability of W51C for CRs remains *** on observations conducted with the Large High Altitude Air Shower Observatory(LHAASO),we report a significant detection ofγrays emanating from the W51 complex,with energies from 2 to 200 *** LHAASO measurements,for the first time,extend theγ-ray emission from the W51 complex beyond 100 TeV and reveal a significant spectrum bending at tens of *** combining the"π^(0)-decay bump"featured data from Fermi-LAT,the broadbandγ-ray spectrum of the W51 region can be well-characterized by a simple pp-collision *** observed spectral bending feature suggests an exponential cutoff at~400 TeV or a power-law break at~200 TeV in the CR proton spectrum,most likely providing the first evidence of SNRs serving as CR accelerators approaching the PeV ***,two young star clusters within W51B could also be theoretically viable to produce the most energeticγrays observed by *** findings strongly support the presence of extreme CR accelerators within the W51 complex and provide new insights into the origin of Galactic CRs.

关键词： UHE c-ray Cosmic rays SNR W51C Star clusters

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Science Bulletin 2024年第4期69卷 449-457页

作者： LHAASO Collaboration Zhen Cao Chuandong gao Cong li Ruo-yu liu Ruizhi Yang 不详 Key Laboratory of Particle Astrophyics&Experimental Physics Division&Computing Center Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China University of Chinese Academy of Sciences Beijing 100049China TIANFU Cosmic Ray Research Center ChengduChina Institute of Frontier and Interdisciplinary Science Shandong UniversityQingdao 266237China School of Astronomy and Space Science Nanjing UniversityNanjing 210023China University of Science and Technology of China Hefei 230026China

We report the detection of aγ-ray bubble spanning at least 100deg2 in ultra-high energy(UHE)up to a few PeV in the direction of the star-forming region Cygnus X,implying the presence super PeVatron(s)accelerating protons to at least 10 PeV.A log-parabola form with the photon indexΓ(E)=(2.71±0.02)+(0.11±0.02)×log10(E/10 TeV)is found fitting the gamma-ray energy spectrum of the bubble *** sources,“hot spots”correlated with very massive molecular clouds,and a quasi-spherical amorphousγ-ray emitter with a sharp central brightening are observed in the *** the core of~0.5°,spatially associating with a region containing massive OB association(Cygnus OB2)and a microquasar(Cygnus X-3),as well as previously reported multi-TeV sources,an enhanced concentration of UHEγ-rays is observed with 2 photons at energies above 1 *** general feature of the bubble,the morphology,and the energy spectrum,are reasonably reproduced by the assumption of a particle accelerator in the core,continuously injecting protons into the ambient medium.

关键词： Cosmic rays γ-rays Interstellar medium Star cluster

胶原酶治疗胶原蛋白(刺激剂)植入后结节并发症专家共识

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中国医疗美容 2024年第2期14卷 1-7页

作者：田宏伟石冰陈锦添高扬韩胜洪伟黄雅雯姬付康蒋威李嘉伦李健李勤李黠李远宏林合晟刘灯刘红梅刘宁刘争潘宝华彭程钱静苏红孙菁菁王晓阳王飏徐智慧许旭亮于晓春喻翔曾东张歌赵亮北京丽都医疗美容医院北京100101 上海洁铭医疗美容门诊部上海200120 重庆医科大学附属第三医院重庆401120 北京首玺丽格医疗美容门诊部北京100125 四川晶肤医学美容医院四川成都610014 重庆颜轻医医疗美容门诊部重庆401121 广州欧缇医疗美容美容部广东广州510075 西安高新医院陕西西安710077 武汉皮可立医疗美容诊所湖北武汉430022 上海华美医疗美容医院上海200135 成都爱思特整形美容医院四川成都610094 成都华美紫馨医疗美容医院四川成都610093 沈阳颜悦医疗美容诊所辽宁沈阳110069 上海光博士医疗美容门诊部上海200135 贵阳慧美倾城美容医院贵州贵阳550081 北京梅颜医疗美容诊所北京100027 杭州硕人医疗美容门诊部浙江杭州311215 杭州时光医疗美容医院浙江杭州310011 重庆华美整形外科医院重庆400015 中南大学湘雅三医院湖南长沙410205 昆明韩辰医疗美容医院云南昆明650034 新疆万橙医疗美容诊所新疆乌鲁木齐830018 上海伊美尔医疗美容医院上海200050 上海颜范医疗美容门诊部上海200030 北京仁德一美医疗美容诊所北京100020 西安艺星医疗美容医院陕西西安710003 华东医药浙江杭州310005 贵阳云岩瑞亚睿美医疗美容外科诊所贵州贵阳550004 广州紫馨医疗美容医院广东广州510627 郑州华领医疗美容医院河南郑州450003 苏州美贝尔医疗美容门诊部江苏苏州215011

1概述。2胶原蛋白(刺激剂)及其植入后结节并发症。2.1胶原蛋白。2.2胶原蛋白及胶原蛋白刺激剂在医疗美容中的应用。2.2.1胶原蛋白(刺激剂)植入适应证。2.2.2胶原蛋白(刺激剂)植入后常见的并发症。2.3胶原蛋白(刺激剂)植入后结节并发症。... 详细信息

1概述。2胶原蛋白(刺激剂)及其植入后结节并发症。2.1胶原蛋白。2.2胶原蛋白及胶原蛋白刺激剂在医疗美容中的应用。2.2.1胶原蛋白(刺激剂)植入适应证。2.2.2胶原蛋白(刺激剂)植入后常见的并发症。2.3胶原蛋白(刺激剂)植入后结节并发症。2.4胶原蛋白(刺激剂)植入后结节并发症的治疗。3胶原酶在胶原蛋白(刺激剂)植入术后结节并发症治疗中的应用。3.1胶原酶及其在临床中的应用。3.2胶原酶治疗胶原蛋白(刺激剂)植入术后结节并发症的理论基础及实验结果。3.3局部注射胶原酶治疗胶原蛋白(刺激剂)植入术后结节的操作方法。3.3.1适应证。3.3.2禁忌证。3.3.3注射方法。3.3.4操作注意事项。3.3.5治疗后护理。3.4局部注射胶原酶的不良反应及处理措施。4总结。

关键词：胶原酶胶原蛋白植入结节并发症专家共识