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Endovenous laser ablation of great saphenous vein with ultrasound-guided perivenous tumescence： early and midterm results

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Chinese Medical Journal 2013年第3期126卷 421-425页

作者： chen jia-quan xie hui deng hao-yu yuan kai zhang ji-wei zhang hao zhang lan Department of Vascular Surgery Renji Hospital School of Medicine Shanghai Jiao Tong University Shanghai 200127 China

Background Endovenous laser ablation （EVLA） is an improved method to treat varicose great saphenous veins （GSV） with a high satisfactory rate. This study aimed to evaluate the efficiency and safety of treatment by EVLA procedures with ultrasound-guided perivenous tumescence. Methods Thirty-one patients （31 limbs） with symptomatic varicose vein primary to chronic venous insufficiency （CVI） treated with EVLA were prospectively studied. The entire procedure was performed under ultrasound-guided tumescent local anesthesia. The patients were evaluated with a 18 month follow-up postoperation using clinical examination and venous duplex ultrasonography. Pain scores and quality of life （QOL） were recorded using visual analog scale （VAS） and the chronic venous insufficiency questionnaire （CIVIQ） at 1 week, 1 month, and 12 months after operation. Results All patients tolerated EVLA procedure well. The overall success occlusion rates of GSV were 92%, 94%, and 94% at 1, 12, and 18 months follow-up, respectively. The score of CIVIQ one week preoperation was 69.14±11.44 while that of CIVIQ one month postoperation was 85.32±4.89. The life quality has significantly improved after the operation of EVLA （t=12.71, P 〈0.05）. The VAS one month after treatment was lower than 1 week before therapy （t=8.048, P 〈0.05）. Major complications such as deep vein thrombosis and skin burns were not found. Most of the complications were minor and improved quickly. Conclusions This refinement type of EVLA procedure is a safe and effective treatment with a high satisfaction rate; it displayed noteworthy features including shortening hospitalization, early ambulant activity, and preferable occlusion rates.

关键词： endovenous laser ablation great saphenous vein occlusion tumescent anaesthesia

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重症肢体缺血的缺血性溃疡患者足部动脉弓病变的影响因素分析

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上海交通大学学报（医学版） 2014年第10期34卷 1519-1524页

作者：谢辉叶猛陈佳佺吕磊袁凯张纪蔚张岚上海交通大学医学院附属仁济医院血管外科上海200127

目的分析影响重症肢体缺血（CLI）的缺血性溃疡患者足部动脉弓病变的因素。方法对152例CLI缺血性溃疡患者的临床资料进行回顾性研究,记录患者的年龄、性别、吸烟史、高血压病史、糖尿病病程、体质量以及血液生化指标等。根据足部动脉弓... 详细信息

目的分析影响重症肢体缺血（CLI）的缺血性溃疡患者足部动脉弓病变的因素。方法对152例CLI缺血性溃疡患者的临床资料进行回顾性研究,记录患者的年龄、性别、吸烟史、高血压病史、糖尿病病程、体质量以及血液生化指标等。根据足部动脉弓造影结果将患者分为2组：足部动脉弓良好组（n=37）和足部动脉弓不良组（n=115）。采用单因素和多因素Logistic回归模型分析影响足部动脉弓病变的因素。结果足部动脉弓不良组的空腹血糖（FBG）浓度和平均血小板体积（MPV）均显著高于足部动脉弓良好组（P〈0.05,P〈0.01）。足部动脉弓不良组患者中糖尿病病程≥10年者所占比例显著高于足部动脉弓良好组（P〈0.001）。Logistic回归分析发现FBG、MPV、糖尿病病程≥10年是足部动脉弓不良的独立危险因素（P〈0.05）。根据受试者工作特征（ROC）曲线获得FBG预测足部动脉弓不良的最佳临界值为6.60 mmol/L,曲线下面积为0.805（P〈0.05）。MPV的最佳临界值为11.70 fl,曲线下面积为0.907（P〈0.05）。再分别以FBG、MPV临界点以及糖尿病病程≥10年为条件,将患者分为2组,Logistic回归分析结果显示FBG浓度≥6.60 mmol/L、MPV≥11.70 fl和糖尿病病程≥10年患者发生足部动脉弓不良的危险度分别是FBG浓度〈6.60 mmol/L、MPV〈11.70 fl和糖尿病病程〈10年患者的8.684倍（95%CI=3.496～21.571,P〈0.05）、12.737倍（95%CI=5.358～30.232,P〈0.05）和7.75倍（95%CI=2.996～20.048,P〈0.05）。结论 FBG浓度升高、MPV增大、糖尿病病程≥10年分别是预测CLI缺血性溃疡患者足部动脉弓不良的独立危险因素。

关键词：重症肢体缺血缺血性溃疡足部动脉弓糖尿病空腹血糖平均血小板体积

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The first data release(DR1) of the LAMOST regular survey

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Research in Astronomy and Astrophysics 2015年第8期15卷 1095-1124页

作者： A-Li Luo Yong-Heng Zhao Gang Zhao Li-Cai deng Xiao-wei Liu Yi-Peng jing Gang Wang hao-Tong zhang jian-Rong Shi Xiang-Qun Cui Yao-quan Chu Guo-Ping Li Zhong-Rui Bai yue Wu Yan Cai Shu-yun Cao Zi-Huang Cao Jeffrey L.Carlin Hai-yuan chen jian-Jun chen Kun-Xin chen Li chen Xue-Lei chen Xiao-Yan chen Ying chen Norbert Christlieb jia-Ru Chu chen-Zhou Cui Yi-Qiao Dong Bing Du Dong-wei Fan Lei Feng jian-Ning Fu Peng Gao Xue-Fei Gong Bo-Zhong Gu Yan-Xin Guo Zhan-Wen Han Bo-Liang He jin-Liang Hou Yong-hui Hou Wen Hou Hong-Zhuan Hu Ning-Sheng Hu Zhong-Wen Hu Zhi-Ying Huo Lei jia Fang-Hua jiang Xiang jiang Zhi-Bo jiang Ge jin Xiao Kong Xu Kong Ya-Juan Lei Ai-Hua Li Chang-Hua Li Guang-wei Li Hai-Ning Li jian Li Qi Li Shuang Li Sha-Sha Li Xin-Nan Li Yan Li Yin-Bi Li Ye-Ping Li yuan Liang Chien-cheng Lin Chao Liu Gen-Rong Liu Guan-Qun Liu Zhi-Gang Liu Wen-Zhi Lu yu Luo Yin-Dun Mao Heidi Newberg ji-Jun Ni Zhao-Xiang Qi Yong-Jun Qi Shi-Yin Shen Huo-Ming Shi jing Song Yi-Han Song Ding-Qiang Su Hong-Jun Su Zheng-Hong Tang Qing-Sheng Tao yuan Tian Dan Wang Da-Qi Wang Feng-Fei Wang Guo-Min Wang Hai Wang Hong-Chi Wang jian Wang jia-Ning Wang jian-Ling Wang jian-Ping Wang Jun-Xian Wang Lei Wang Meng-Xin Wang Shou-Guan Wang Shu-Qing Wang Xia Wang Ya-Nan Wang You Wang yue-Fei Wang You-Fen Wang Peng wei Ming-Zhi wei Hong Wu Ke-Fei Wu Xue-Bing Wu yu-Zhong Wu Xiao-Zheng Xing Ling-Zhe Xu Xin-Qi Xu Yan Xu Tai-Sheng Yan De-Hua Yang Hai-Feng Yang hui-Qin Yang Ming Yang Zheng-Qiu Yao Yong yu hui yuan Hai-Bo yuan Hai-Long yuan wei-Min yuan Chao Zhai En-Peng zhang Hua-wei zhang jian-Nan zhang Li-Pin zhang wei zhang Yong zhang Yan-Xia zhang Zheng-Chao zhang Ming Zhao Fang Zhou Xu Zhou jie Zhu Yong-Tian Zhu Si-cheng Zou Fang Zuo National Astronomical Observatories Chinese Academy of Sciences Department of Astronomy Peking University Shanghai Astronomical Observatory Chinese Academy of Sciences Nanjing Institute of Astronomical Optics & Technology National Astronomical ObservatoriesChinese Academy of Sciences University of Science and Technology of China Department of Physics Applied Physics and AstronomyRensselaer Polytechnic InstituteTroyNY 12180USA Department of Physics and Astronomy Earlham CollegeRichmondIN 47374USA Universitt Heidelberg Zentrum für AstronomieLandessternwarteKnigstuhl 1269117 HeidelbergGermany Department of Astronomy Beijing Normal University yunnan Observatories Chinese Academy of Sciences Purple Mountain Observatory Chinese Academy of Sciences

The Large sky Area Multi-Object Fiber Spectroscopic Telescope（LAMOST） general survey is a spectroscopic survey that will eventually cover approximately half of the celestial sphere and collect 10 million spectra of stars, galaxies and QSOs. Objects in both the pilot survey and the first year regular survey are included in the LAMOST DR1. The pilot survey started in October 2011 and ended in June 2012, and the data have been released to the public as the LAMOST Pilot Data Release in August 2012. The regular survey started in September 2012, and completed its first year of operation in June 2013. The LAMOST DR1 includes a total of 1202 plates containing 2 955 336 spectra, of which 1 790 879 spectra have observed signalto-noise ratio（SNR） ≥ 10. All data with SNR ≥ 2 are formally released as LAMOST DR1 under the LAMOST data policy. This data release contains a total of 2 204 696 spectra, of which 1 944 329 are stellar spectra, 12 082 are galaxy spectra and 5017 are quasars. The DR1 not only includes spectra, but also three stellar catalogs with measured parameters： late A,FGK-type stars with high quality spectra（1 061 918 entries）, A-type stars（100 073 entries）, and M-type stars（121 522 entries）. This paper introduces the survey design, the observational and instrumental limitations, data reduction and analysis, and some caveats. A description of the FITS structure of spectral files and parameter catalogs is also provided.

关键词： techniques: spectroscopic survey—data release—catalog

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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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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

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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

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严重创伤患者紧急救治血液保障模式与输血策略中国专家共识(2024版)

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中华创伤杂志 2024年第10期40卷 865-881页

作者：卢尧李阳张雷英唐昊敬慧丹王耀丽贾向志巴立卞茂红蔡丹蔡辉蔡晓红查占山陈秉宇陈大庆陈凤陈国安陈海鸣陈静陈敏陈青陈舒陈玺程金凤褚晓凌崔红旺崔欣达珍戴莹邓素容董伟群范为民冯珂付丹晖付涌水傅奇傅雪梅甘佳甘新宇高伟巩怀证桂嵘郭庚韩宁郝一文何武兵洪强侯瑞琴侯卫胡婕胡培阳胡熙胡晓玉黄光斌黄婕黄象艳黄远帅浑守永蒋学兵金平赖冬乐爱平黎红梅李碧娟李翠莹李代红李海宏李贺李辉李剑平李宁李喜莹李湘民李小飞李晓娟李志强李忠俊李尊严梁华钦梁晓华廖冬发廖群廖燕林甲进刘春霞刘凤华刘培贤刘铁梅刘小信刘志伟刘中砥陆华栾建凤骆建军骆群吕定丰吕琪吕先萍马爱军马立强马曙轩马现君马小刚马晓莉毛国庆穆士杰聂少林欧阳淑娟欧阳锡林潘春球潘健潘晓华彭磊彭涛钱宝华乔姝秦莉任颖任召祺戎瑞明苏常山孙明伟孙文武孙振威唐海平唐晓峰唐长玖陶翠华田志彬汪娟王宝燕王春燕王革非王海燕王鸿捷王鹏王鹏里王秋实王晓宁王新华王学锋王勇王勇军王远杰王志华韦少俊魏亚明文键波文军吴江吴巨峰夏爱军夏飞夏荣谢珏邢颜超熊雁徐峰徐永柱许永安晏永和燕备战杨江杨江存杨军杨新文杨勇毅姚春艳叶明亮尹昌林尹明尹文于连玲于淑红余泽波郁毅刚喻安永袁红袁燚张婵张进军张军张凯张磊冰张泉张荣江张三明张生吉张硕张伟张伟东张晰张兴文章桂喜章晓军赵国庆赵建鹏赵树铭郑蓓蓓郑山根周华友周吉成周砺宏周谋周小玉周雪莲周源周政周祖皇朱海燕朱培元朱长举祝丽丽王正国蒋建新汪德清兰炯采王全立于洋张连阳文爱清中华医学会临床输血学分会中华医学会创伤学分会创伤急救与多发伤学组中华医学会灾难医学分会青年学组陆军军医大学陆军特色医学中心重庆400042 陆军军医大学陆军特色医学中心创伤与化学中毒全国重点实验室重庆400042 中国人民解放军总医院第一医学中心北京100853 军事医学研究院卫生勤务与血液研究所北京100850 浙江大学医学院附属第二医院杭州310009 安徽医科大学第一附属医院合肥230022 湘潭市中心医院湘潭411100 中国医学科学院北京协和医学院输血研究所成都610052 上海交通大学医学院附属瑞金医院上海200025 海军军医大学第一附属医院上海200433 浙江省人民医院杭州310014 温州医科大学附属第二医院温州325027 内蒙古自治区人民医院呼和浩特010017 武汉市血液中心武汉430030 南昌大学第一附属医院南昌330006 河北医科大学第三医院石家庄050051 乌鲁木齐市血液中心乌鲁木齐830000 南京大学医学院附属鼓楼医院南京210008 浙江省血液中心杭州310052 重庆两江新区人民医院重庆401121 株洲市中心医院株洲412000 福建省疾病预防控制中心福州350012 海南医学院第一附属医院海口570102 贵州省血液中心贵阳550001 西藏自治区血液中心拉萨850000 中国人民解放军联勤保障部队第九二〇医院昆明650000 重庆医科大学附属永川医院重庆402160 昆明医科大学第一附属医院昆明650032 江西省血液中心南昌330052 宁夏医科大学总医院银川750001 福建医科大学附属协和医院福州350001 广州市第一人民医院广州510080 重庆市血液中心重庆400015 成都市血液中心成都610042 中国医学科学院北京协和医院北京100730 中国人民解放军西部战区总医院成都610083 华中科技大学同济医学院附属同济医院武汉430030 山东省血液中心济南250014 中南大学湘雅三医院长沙410013 山西医科大学第一医院太原030001 上海同济大学附属东方医院上海200120 中国医科大学附属第一医院沈阳110001 福建省立医院福州350001 厦门大学附属第一医院厦门361003 北京大学人民医院北京100044 青海省血液中心西宁810007 浙江省天台县人民医院天台317200 昆明市儿童医院昆明650228 安徽省血液中心合肥230031 重庆大学附属中心医院重庆市急救医疗中心重庆400014 湖南省人民医院(湖南师范大学附属第一医院) 长沙410001 中国人民解放军联勤保障部队第九六〇医院济南250031 西南医科大学附属医院泸州646000 山东第一医科大学附属省立医院济南250021 中国人民解放军总医院第六医学中心北京100048 余姚市人民医院余姚315400 厦门医学院附属第二医院厦门361005 重庆市垫江县人民医院重庆408300 中南大学湘雅医院长沙410008 空军军医大学空军特色医学中心北京100142 天津市第一中心医院天津300192 山西省中西医结合医院太原030013 安徽医科大学第二附属医院合肥230601 辽宁省血液中心沈阳110044 中国医学科学院肿瘤医院北京100021 首都医科大学附属北京友谊医院北京100050 兰州大学第二医院兰州730030 上海市第六人民医院上海201599 陆军军医大学第二附属医院重庆400037 北华大学附属医院吉林132000 广州血液中心广州510095 大连市血液中心大连116001 广西医科大学第三附属医院南宁530007 兰州大学第一医院兰州730030 哈尔滨医科大学附属第一医院哈尔滨150010 山西医科大学第二医院太原030000 吉林大学中日联谊医院长春130062 山东第一医科大学第一附属医院(山东省千佛山医院) 济南250013 浙江大学医学院附属邵逸夫医院杭州310016 重庆医科大学附属第二医院重庆400010 中国人民解放军东部战区总医院南京210002 中国人民解放军联勤保障部队第九〇三医院杭州310013 中国人民解放军总医院第五医学中心北京100071 宁波大学附属第一医院宁波315010 天津大学应急医学研究院天津300072 郑州大学第一附属医院郑州450052 河北省血液中心石家庄050004 中国人民解放军联勤保障部队第九〇〇医院福州350025 首都医科大学附属北京儿童医院北京100045 山东大学齐鲁医院济南250012 西藏自治区人民医院拉萨850000 河南省红十字血液中心郑州450012 荆州市中心血站荆州434099 空军军医大学第二附属医院西安710038 株洲市中心血站株洲412007 湖南省肿瘤医院/中南大学湘雅医

严重创伤患者对救治时效性要求极高,输血在此类患者的紧急救治阶段发挥着不可替代的作用。越来越多的循证医学证据和临床经验表明,早期输注低效价O型全血或平衡比例红细胞、血浆和血小板等成分血的止血复苏策略将使严重创伤大出血患者... 详细信息

严重创伤患者对救治时效性要求极高,输血在此类患者的紧急救治阶段发挥着不可替代的作用。越来越多的循证医学证据和临床经验表明,早期输注低效价O型全血或平衡比例红细胞、血浆和血小板等成分血的止血复苏策略将使严重创伤大出血患者获益。然而,当前国内血液保障模式不能完全满足临床对严重创伤患者紧急救治输血的时效性和有效性需求。针对我国严重创伤紧急救治血液保障模式与输血策略中存在的关键问题,中华医学会临床输血学分会、中华医学会创伤学分会创伤急救与多发伤学组和中华医学会灾难医学分会青年学组组织国内输血医学和创伤救治专家,基于循证医学证据并结合Delphi法专家咨询投票,共同制订《严重创伤患者紧急救治血液保障模式与输血策略中国专家共识(2024版)》,从血液保障模式和输血策略两个方面共提出10条推荐意见,为严重创伤紧急救治阶段的输血复苏提供参考,以期进一步提高严重创伤患者的救治成功率。

关键词：创伤和损伤急救输血专家共识

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JUNO sensitivity on proton decay p→νK^(+)searches

引用

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

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