检索结果-南通市图书馆

THE EFFECT OF DIFFERENT TopICAL BETABLOCKERS ON OCULAR HEm.DY- NAm.CS AND opTIC NERVE HEAD BLOOD FLOW IN GLAUCOm. PATIENTS

在线全文

同方期刊数据库

学校读者我要写书评

暂无评论

国际眼科杂志 2003年第1期3卷 27-27页

作者： A.G.Boehm.A.U.Koeller m.F.m.eller K.A.m.llenhauer L.E.Pillunat Departm.nt of ophthalm.logy University of Dres-den GermanyDepartment of Ophthalmology University of Dres-den GermanyDepartment of Ophthalmology University of Dres-den GermanyDepartment of Ophthalmology University of Dres-den GermanyDepartment of Ophthalmology University of Dres-den Germany

Purpose: The aim.of the study is to evaluate the influence of different betablockers on ocular hem.dynam.cs and optic nerve head blood flow in glaucom. patients. m.thods: 30 patients (12 m.le, 18 fem.le) with prim.ry open-angle glaucom. between 39 and 74 years of age were treated for 4 weeks each with betax-olol (BX), m.tipranolol 0.3% (m.) and tim.lol 0.5% (TL) in a random.zed, double m.sked, crossover design. At baseline in-

关键词：青光眼患者 β阻滞剂眼内血流动力学视神经乳头血流影响

白大衣性高血压患者的内皮损伤:凝集素样氧化型低密度脂蛋白1

在线全文

学校读者我要写书评

暂无评论

中华高血压杂志 2015年第2期23卷 124-124页

作者：刘莉叶鹏 Yavuzer S Yavuzer H Cengiz m.Erm.n H Altiparm.k m. Korkm.zer B Balci H Sim.ek G Yaldiran AL Karter Y Uzun H

该研究对高血压患者可溶性凝集素样氧化型低密度脂蛋白受体1（solublelectin—likeoxidizedlow-den—sitvlipoproteinreceptor-l，sL OX-1）的水平进行检测，探讨sLOX-1与氧化型低密度脂蛋白（oxidizedlow-densitylipoprotein，oxLDL）... 详细信息

关键词：氧化型低密度脂蛋白受体高血压患者凝集素内皮损伤白大衣性内皮型一氧化氮合酶可溶性相关性

Feasibility and physics potential of detecting ^(8)B solar neutrinos at j.NO

在线全文

学校读者我要写书评

暂无评论

Chinese Physics C 2021年第2期45卷 93-110页

作者： Angel 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 j.ão 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. j.se Busto Ilya Butorov Anatael Cabrera Hao Cai Xiao Cai Yanke Cai Zhiyan Cai Antonio Cam.i Agustin campeny Chuanya Cao Guofu Cao j.n Cao Rossella Caruso Cédric Cerna j.nfan Chang Yun Chang Pingping Chen Po-An Chen Shaom.n Chen Shenj.an Chen Xurong Chen Yi-Wen Chen Yixue Chen Yu Chen Zhang Chen j.e 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 j.awei deng Zhi deng Ziyan deng Wilfried Depnering m.rco Diaz Xuefeng Ding Yayun Ding Bayu Dirgantara Sergey Dm.trievsky Tadeas Dohnal Georgy Donchenko j.anm.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 Faj. Donghua Fan Lei Fan Can Fang j.an 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 j.ngyuan 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 j.neiro RioBrazil Pontificia Universidad Católica de Chile SantiagoChile Universidad Tecnica Federico Santa m.ria ValparaisoChile Beij.ng Institute of Spacecraft Environm.nt Engineering BeijingChina Beij.ng 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 j.lin University ChangchunChina College of Electronic Science and Engineering National University of Defense TechnologyChangshaChina Chongqing University ChongqingChina Dongguan University of Technology DongguanChina j.nan 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 Nanj.ng 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 j.aotong 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 j.angm.n Underground Neutrino Observatory(j.NO)features a 20 kt m.lti-purpose underground liquid scintillator sphere as its m.in *** of j.NO'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 j.NO'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),j.NO 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 ***,j.NO 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 j.NO

j.NO sensitivity on proton decay p→νK^(+)searches

在线全文

学校读者我要写书评

暂无评论

Chinese Physics C 2023年第11期47卷 7-22页

作者： Angel 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 j.ão 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. j.se Busto Ilya Butorov Anatael Cabrera Barbara Caccianiga 蔡浩蔡啸蔡严克蔡志岩 Riccardo Callegari Antonio Cam.i 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 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 j.lm.ni Kuo-Lun j.n Ignacio j.ria 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 j.llet j.ri j.utsenvaara Sirichok j.ngthawan 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 j.int 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 Ij.Lab 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 Beij.ng Institute of Spacecraft Environm.nt Engineering BeijingChina Universidade Estadual de Londrina LondrinaBrazil INFN Sez

The j.angm.n Underground Neutrino Observatory(j.NO)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 j.NO 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 j.NO 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 j.NO liquid scintillator detector