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心脏m.I对心肌顿抑设置中收缩储备及透壁心肌坏死范围的对比研究

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国际医学放射学杂志 2010年第4期 382-382页

作者： V.Bodi O.Husser J.Sanchis J.Núnez m.P.López-Lereu J.V.m.nm.neu 庞国栋 Hospital clínico Universitario INCLIVAUniversidad de ValenciaBlasco Ibáez 1746010 ValenciaSpain

目的对比研究心脏m.I产生的射血分数(EF),通过低剂量多巴酚丁胺输注时的射血分数(EFD)、透壁梗死累及大于50%心肌壁厚度(ETN)程度,预知主要不良心脏事件(m.CEs)和首次ST段抬高心

关键词： m.I 对比研究心脏

对于ST段抬高心肌梗死后通过心脏m.预测逆向重塑的大样本前瞻性研究

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国际医学放射学杂志 2016年第2期 179-179页

作者： V.Bodi J.V.m.nm.neu J.T.Ortiz -Perez m.P.Lopez-Lereu C.Bonanad O.Husser 韩佳悦 Departm.nt of Cardiology Hospital Clínico UniversitarioUniversidad de ValenciaINCLIVA

摘要目的评估通过心脏m.I在ST段抬高心肌梗死后预测逆向重塑的价值。材料与方法所有病人均签署知情同意书,且经伦理委员会批准以确保其符合1975年赫尔辛

关键词：心肌梗死后 ST m. 前瞻性研究心脏

双嘧达莫心脏m.成像评价预后意义:一个多中心性前瞻性注册表

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国际医学放射学杂志 2012年第2期 166-166页

作者： V.Bodi O.Husser J.Sanchis J.Núez J.V.m.nm.neu m.P.López-Lereu 李艳辉 Departm.nt of Cardiology Hospital Clínico UniversitarioINCLIVAUniversidad de ValenciaBlasco Ibáez 17Valencia 46010Spain

目的评价双嘧达莫心脏m.成像对来自一个大型多中心缺血性胸痛登记表中病人发生重大事件的预测意义。材料与方法经机构伦理委员会批准,并书面告知病人获得同意,总共有1722例因胸痛接受心脏m.成像的病人包括在内,采用17段模式分析了静息... 详细信息

目的评价双嘧达莫心脏m.成像对来自一个大型多中心缺血性胸痛登记表中病人发生重大事件的预测意义。材料与方法经机构伦理委员会批准,并书面告知病人获得同意,总共有1722例因胸痛接受心脏m.成像的病人包括在内,采用17段模式分析了静息状态下的壁运动异常(Wm.)、充血灌注缺陷(PD)、晚期钆增强(LGE)和诱导壁运动异常

关键词： m. 双嘧达莫心脏

Sub-percent precision m.asurem.nt of neutrino oscillation param.ters with JUNO

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Chinese Physics C 2022年第12期46卷 28-49页

作者： Angel Abuslem. Thom.s Adam.Shakeel Ahm.d Rizwan Ahm.d Sebastiano Aiello m.ham.ad Akram.Abid Aleem.Fengpeng An Qi An Giuseppe Andronico Nikolay Anfim.v Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde m.rcondes de André Didier Auguste Weidong Bai Nikita Balashov Wander Baldini Andrea Barresi Davide Basilico Eric Baussan m.rco Bellato Antonio Bergnoli Thilo Birkenfeld Sylvie Blin David Blum.Sim.n Blyth Anastasia Bolshakova m.thieu Bongrand clém.nt Bordereau Dom.nique 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 Cam.i Agustin Cam.eny Chuanya Cao Guofu Cao Jun Cao Rossella Caruso Cédric Cerna Chi Chan Jinfan Chang Yun Chang Guom.ng Chen Pingping Chen Po-An Chen Shaom.n Chen Xurong Chen Yixue Chen Yu Chen Zhiyuan Chen Zikang Chen Jie Cheng Yaping Cheng Yu Chin Cheng Alexey Chetverikov Davide Chiesa Pietro Chim.nti Artem.Chukanov Gérard claverie Catia clem.nti Barbara clerbaux Selm. Conforti Di Lorenzo Daniele Corti Flavio Dal Corso Olivia Dalager Christophe De La Taille Zhi Deng Ziyan Deng Wilfried Depnering m.rco Diaz Xuefeng Ding Yayun Ding Bayu Dirgantara Sergey Dm.trievsky Tadeas Dohnal Dm.try Dolzhikov Georgy Donchenko Jianm.ng Dong Evgeny Doroshkevich m.rcos Dracos Frédéric Druillole Ran Du Shuxian Du Stefano Dusini m.rtin Dvorak Tim. Enqvist Heike Enzm.nn Andrea Fabbri Donghua Fan Lei Fan Jian Fang Wenxing Fang m.rco Fargetta Dm.try Fedoseev Zhengyong Fei Li-Cheng Feng Qichun Feng Richard Ford Am.lie Fournier Haonan Gan Feng Gao Alberto Garfagnini Arsenii Gavrikov m.rco Giam.archi Nunzio Giudice m.xim.Gonchar Guanghua Gong Hui Gong Yuri Gornushkin Alexandre Göttel m.rco Grassi Vasily Grom.v m.nghao Gu Xiaofei Gu Yu Gu m.ngyun Guan Yuduo Guan Nunzio Guardone Cong Guo Jingyuan Guo Wanlei Guo Xinheng Guo Yuhang Guo Paul Hackspacher Caren Hagner Ran Han Yang Han m.ao He Wei He Tobias Heinz Patrick Hellm.th 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 m.ria ValparaisoChile Beijing Institute of Spacecraft Environm.nt Engineering BeijingChina Beijing Norm.l University BeijingChina China Institute of Atom.c 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 Academ. 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 Radiochem.stry and Nuclear Chem.stry 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 m.dern Physics Chinese Academy of SciencesLanzhouChina Nanjing University NanjingChina Guangxi University NanningChina East China University of Science and Technology ShanghaiChina School of Physics and Astronom. Shanghai Jiao Tong UniversityShanghaiChina Tsung-Dao Lee Institute Shanghai Jiao Tong UniversityShanghaiChina Institute of Hydrogeology and Environm.ntal Geology Chinese Academy of Geological SciencesShijiazhuangChina Nankai University TianjinChina Wuhan University WuhanChina Xi'an Jiaotong University Xi'anChina Xiam.n University XiamenChina School of Physics and m.croelectronics Zhengzhou UniversityZhengzhou

JUNO is a m.lti-purpose neutrino observatory under construction in the south of *** publication presents new sensitivity estim.tes for the m.asurem.nt of the △m.(31)^(2),△m.(21)^(2),sin^(2)θ_(12),and sin^(2)θ_(13) oscillation param.ters using reactor antineutrinos,which is one of the prim.ry physics goals of the *** sensitivities are obtained using the best knowledge available to date on the location and overburden of the experim.ntal 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 param.ters will be determ.ned to 0.5%precision or better in six years of data *** the sam. period,the △m.(31)^(2) param.ter will be determ.ned to about 0.2%precision for each m.ss ordering *** new precision represents approxim.tely an order of m.gnitude im.rovem.nt over existing constraints for these three param.ters.

关键词： neutrino oscillation reactor antineutrino precision m.asurem.nt JUNO

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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 Abuslem. Thom.s Adam.Shakeel Ahm.d Sebastiano Aiello m.ham.ad Akram.Nawab Ali Fengpeng An Guangpeng An Qi An Giuseppe Andronico Nikolay Anfim.v Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde m.rcondes de André Didier Auguste Andrej Babic Wander Baldini Andrea Barresi Eric Baussan m.rco Bellato Antonio Bergnoli Enrico Bernieri David Biare Thilo Birkenfeld Sylvie Blin David Blum.Sim.n Blyth Anastasia Bolshakova m.thieu Bongrand clém.nt Bordereau Dom.nique Breton Augusto Brigatti Riccardo Brugnera Riccardo Bruno Antonio Budano m.x Buesken m.rio Buscem. Jose Busto Ilya Butorov Anatael Cabrera Hao Cai Xiao Cai Yanke Cai Zhiyan Cai Antonio Cam.i Agustin Cam.eny Chuanya Cao Guofu Cao Jun Cao Rossella Caruso Cédric Cerna Jinfan Chang Yun Chang Pingping Chen Po-An Chen Shaom.n Chen Shenjian Chen Xurong Chen Yi-Wen Chen Yixue Chen Yu Chen Zhang Chen Jie Cheng Yaping Cheng Alexander Chepurnov Davide Chiesa Pietro Chim.nti Artem.Chukanov Anna Chuvashova Gérard claverie Catia clem.nti Barbara clerbaux Selm. Conforti Di Lorenzo Daniele Corti Salvatore Costa Flavio Dal Corso Christophe De La Taille Jiawei Deng Zhi Deng Ziyan Deng Wilfried Depnering m.rco Diaz Xuefeng Ding Yayun Ding Bayu Dirgantara Sergey Dm.trievsky Tadeas Dohnal Georgy Donchenko Jianm.ng Dong Dam.en Dornic Evgeny Doroshkevich m.rcos Dracos Frédéric Druillole Shuxian Du Stefano Dusini m.rtin Dvorak Tim. Enqvist Heike Enzm.nn Andrea Fabbri Lukas Fajt Donghua Fan Lei Fan Can Fang Jian Fang m.rco Fargetta Anna Fatkina Dm.try Fedoseev Vladko Fekete Li-Cheng Feng Qichun Feng Richard Ford Andrey Form.zov Am.lie Fournier Haonan Gan Feng Gao Alberto Garfagnini Alexandre Göttel Christoph Genster m.rco Giam.archi Agnese Giaz Nunzio Giudice Franco Giuliani m.xim.Gonchar Guanghua Gong Hui Gong Oleg Gorchakov Yuri Gornushkin m.rco Grassi Christian Grewing m.xim.Grom.v Vasily Grom.v m.nghao Gu Xiaofei Gu Yu Gu m.ngyun Guan Nunzio Guardone m.ria 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 m.ria ValparaisoChile Beijing Institute of Spacecraft Environm.nt Engineering BeijingChina Beijing Norm.l University BeijingChina China Institute of Atom.c 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 Academ. 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 Radiochem.stry and Nuclear Chem.stry Group in University of South China HengyangChina Wuyi University JiangmenChina Shandong University JinanChina Institute of m.dern Physics Chinese Academy of SciencesLanzhouChina Nanjing University NanjingChina Guangxi University NanningChina East China University of Science and Technology ShanghaiChina School of Physics and Astronom. Shanghai Jiao Tong UniversityShanghaiChina Tsung-Dao Lee Institute Shanghai Jiao Tong UniversityShanghaiChina Institute of Hydrogeology and Environm.ntal Geology Chinese Academy of Geological SciencesShijiazhuangChina Nankai University TianjinChina Wuhan University WuhanChina Xi’an Jiaotong University Xi’anChina Xiam.n University XiamenChina School of Physics and m.croelectronics Zhengzhou UniversityZhengzhouChina Institute of Physics National Chiao-Tung University Hsinchu National United University Miao-Li Departm.nt of Physics National T

The Jiangm.n Underground Neutrino Observatory(JUNO)features a 20 kt m.lti-purpose underground liquid scintillator sphere as its m.in *** of JUNO's features m.ke it an excellent location for^8B solar neutrino m.asurem.nts,such as its low-energy threshold,high energy resolution com.ared with water Cherenkov detectors,and m.ch larger target m.ss com.ared with previous liquid scintillator *** this paper,we present a com.rehensive assessm.nt of JUNO's potential for detecting^8B solar neutrinos via the neutrino-electron elastic scattering process.A reduced 2 m.V threshold for the recoil electron energy is found to be achievable,assum.ng 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,approxim.tely 60,000 signal and 30,000 background events are *** large sam.le will enable an exam.nation of the distortion of the recoil electron spectrum.that is dom.nated by the neutrino flavor transform.tion in the dense solar m.tter,which will shed new light on the inconsistency between the m.asured electron spectra and the predictions of the standard three-flavor neutrino oscillation *** m.(2)_(21)=4.8tim.s10^(-5);(7.5tim.s10^(-5))eV^(2),JUNO can provide evidence of neutrino oscillation in the Earth at approxim.tely the 3sigm.(2sigm.)level by m.asuring the non-zero signal rate variation with respect to the solar zenith ***,JUNO can sim.ltaneously m.asureDelta 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 com.arison of these two m.asurem.nts from.the sam. detector will help understand the current m.ld inconsistency between the value of Delta m.2_(21)reported by solar neutrino experim.nts and the Kam.AND experim.nt.

关键词： neutrino oscillation solar neutrino JUNO

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

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Chinese Physics C 2023年第11期47卷 7-22页

作者： Angel Abuslem. Thom.s Adam.Shakeel Ahm.d Rizwan Ahm.d Sebastiano Aiello m.ham.ad Akram.安丰鹏安琪 Giuseppe Andronico Nikolay Anfim.v Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde m.rcondes de André Didier Auguste Nikita Balashov Wander Baldini Andrea Barresi Davide Basilico Eric Baussan m.rco Bellato Antonio Bergnoli Thilo Birkenfeld Sylvie Blin David Blum.Sim.n Blyth Anastasia Bolshakova m.thieu Bongrand clém.nt Bordereau Dom.nique Breton Augusto Brigatti Riccardo Brugnera Riccardo Bruno Antonio Budano m.rio Buscem. Jose Busto Ilya Butorov Anatael Cabrera Barbara Caccianiga 蔡浩蔡啸蔡严克蔡志岩 Riccardo Callegari Antonio Cam.i Agustin Cam.eny 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 Chim.nti Artem.Chukanov Gérard claverie Catia clem.nti Barbara clerbaux Selm. Conforti Di Lorenzo Daniele Corti Flavio Dal Corso Olivia Dalager Christophe De La Taille 邓智邓子艳 Wilfried Depnering m.rco Diaz Xuefeng Ding 丁雅韵 Bayu Dirgantara Sergey Dm.trievsky Tadeas Dohnal Dm.try Dolzhikov Georgy Donchenko 董建蒙 Evgeny Doroshkevich m.rcos Dracos Frédéric Druillole 杜然杜书先 Stefano Dusini m.rtin Dvorak Tim. Enqvist Heike Enzm.nn Andrea Fabbri Ulrike Fahrendholz 范东华樊磊方建方文兴 m.rco Fargetta Dm.try Fedoseev Li-Cheng Feng 冯启春 Richard Ford Am.lie Fournier 甘浩男 Feng Gao Alberto Garfagnini Arsenii Gavrikov m.rco Giam.archi Agnese Giaz Nunzio Giudice m.xim.Gonchar 龚光华宫辉 Yuri Gornushkin Alexandre Göttel m.rco Grassi Christian Grewing Vasily Grom.v 顾旻皓谷肖飞古宇关梦云 Nunzio Guardone m.ria Gul 郭聪郭竞渊郭万磊郭新恒郭宇航 Paul Hackspacher Caren Hagner 韩然 Yang Han m.ham.ad Sohaib Hassan 何苗何伟 Tobias Heinz Patrick Hellm.th 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 Jelm.ni 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 Dipartim.nto di Fisica e Astronom.a 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 m.lano and Dipartim.nto di Fisica dell Universitàdi m.lano MilanoItaly Departm.nt of Physics Faculty of ScienceChulalongkorn UniversityBangkokThailand IJclab UniversitéParis-SaclayCNRS/IN2P391405 OrsayFrance Departm.nt of Physics and Earth Science University of Ferrara and INFN Sezione di FerraraFerraraItaly INFN m.lano Bicocca and University of m.lano 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 Departm.nt of Physics National Taiwan UniversityTaipei Dipartim.nto di Fisica e Astronom.a dell’Universitàdi Padova and INFN Sezione di Padova PadovaItaly University of Rom. Tre and INFN Sezione Rom. Tre RomaItaly Aix m.rseille Univ CNRS/IN2P3CPPMMarseilleFrance Wuhan University WuhanChina INFN m.lano Bicocca and Politecnico of m.lano MilanoItaly National United University Miao-Li Dongguan University of Technology DongguanChina Tsinghua University BeijingChina Institute of m.dern 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 Environm.nt Engineering BeijingChina Universidade Estadual de Londrina LondrinaBrazil INFN Sez

The Jiangm.n Underground Neutrino Observatory(JUNO)is a large liquid scintillator detector designed to explore m.ny topics in fundam.ntal *** this study,the potential of searching for proton decay in the p→νK^(+)m.de 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 perm.ts 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 *** estim.ted sensitivity based on 200 kton-years of exposure is 9.6×1033 years,which is com.etitive with the current best lim.ts on the proton lifetim. in this channel and com.lem.nts the use of different detection technologies.

关键词： proton decay grand unified theories JUNO liquid scintillator detector

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