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Quadratic convective flow of radiated nano-j.ffrey liquid subj.ct to multiple convective conditions and Cattaneo-Christov double diffusion

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Applied Mathematics and Mechanics(English Edition) 2018年第9期39卷 1311-1326页

作者： p.B.SAMpATH KUMAR B.MAHANTHESH B.j.GIREESHA S.A.SHEHZAD Department of Studies and Research in Mathematics Kuvempu University Department of Mathematics Christ University Department of Mathematics COMSATS Institute of Information Technology

A nonlinear flow of j.ffrey liquid with Cattaneo-Christov heat flux is investigated in the presence of nanoparticles. The features of thermophoretic and Brownian movement are retained. The effects of nonlinear radiation, magnetohydrodynamic(MHD), and convective conditions are accounted. The conversion of governing equations into ordinary differential equations is prepared via stretching transformations. The consequent equations are solved using the Runge-Kutta-Fehlberg(RKF) method. Impacts of physical constraints on the liquid velocity, the temperature, and the nanoparticle volume fraction are analyzed through graphical illustrations. It is established that the velocity of the liquid and its associated boundary layer width increase with the mixed convection parameter and the Deborah number.

关键词： nonlinear convection j.ffrey liquid nanoliquid convective condition thermophoretic Brownian motion

Hypertension：健康人的血压是由酶nNOS调节的

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现代生物医学进展 2017年第11期17卷 I0003-I0004页

作者： Husain Shabeeh Sitara Khan Benyu j.ang Sally Brett Narbeh Melikian Barbara Casadei phil.p j. chowienczyk Aj.y M. Shah From the King’s College London British Heart Foundation Centre Cardiovascular Division United Kingdom (H.S. S.K. B.J. S.B. N.M. P.J.C. A.M.S.) and Department of Cardiovascular Medicine University of Oxford United Kingdom (B.C.). From the King’s College London British Heart Foundation Centre Cardiovascular Division United Kingdom (H.S. S.K. B.J. S.B. N.M. P.J.C. A.M.S.) and Department of Cardiovascular Medicine University of Oxford United Kingdom (B.C.). From the King’s College London British Heart Foundation Centre Cardiovascular Division United Kingdom (H.S. S.K. B.J. S.B. N.M. P.J.C. A.M.S.) and Department of Cardiovascular Medicine University of Oxford United Kingdom (B.C.). From the King’s College London British Heart Foundation Centre Cardiovascular Division United Kingdom (H.S. S.K. B.J. S.B. N.M. P.J.C. A.M.S.) and Department of Cardiovascular Medicine University of Oxford United Kingdom (B.C.). From the King’s College London British Heart Foundation Centre Cardiovascular Division United Kingdom (H.S. S.K. B.J. S.B. N.M. P.J.C. A.M.S.) and Department of Cardiovascular Medicine University of Oxford United Kingdom (B.C.). From the King’s College London British Heart Foundation Centre Cardiovascular Division United Kingdom (H.S. S.K. B.J. S.B. N.M. P.J.C. A.M.S.) and Department of Cardiovascular Medicine University of Oxford United Kingdom (B.C.). From the King’s College London British Heart Foundation Centre Cardiovascular Division United Kingdom (H.S. S.K. B.J. S.B. N.M. P.J.C. A.M.S.) and Department of Cardiovascular Medicine University of Oxford United Kingdom (B.C.). From the King’s College London British Heart Foundation Centre Cardiovascular Division United Kingdom (H.S. S.K. B.J. S.B. N.M. P.J.C. A.M.S.) and Department of Cardiovascular Medicine University of Oxford United Kingdom (B.C.).

在一项新的研究中。来自英国伦敦国王学院的研究人员发现调节血压的一氧化氮（NO）是在神经组织中而不是在血管壁中形成的。这一发现可能导致人们开发出更加有效地治疗高血压的方法。

关键词：高血压 nNOS 健康人神经组织一氧化氮研究人员酶血管壁

复发性口疮患者静止期与溃疡期T抑制细胞功能比较研究

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口腔医学纵横 2001年第1期17卷 57-59页

作者：胡雁 Neil W Savage phil B Sugerman Greg j.Sey mour 广东省口腔医院广东广州510280 昆士兰大学牙学院

目的 :本研究旨在比较RAU患者溃疡期和静止期外周血淋巴细胞抑制活性 ,探索T抑制细胞在RAU发病学中的作用。方法 :应用刀豆碱 (ConA)激活产生的淋巴细胞抑制检测方法探测了 12位RAU患者溃疡期和静止期外周血淋巴细胞抑制活性。结果 :溃... 详细信息

目的 :本研究旨在比较RAU患者溃疡期和静止期外周血淋巴细胞抑制活性 ,探索T抑制细胞在RAU发病学中的作用。方法 :应用刀豆碱 (ConA)激活产生的淋巴细胞抑制检测方法探测了 12位RAU患者溃疡期和静止期外周血淋巴细胞抑制活性。结果 :溃疡期患者的T淋巴细胞抑制率明显低于正常组 (p p >0 .0 5 )。结论 :RAU患者外周血T抑制细胞功能在溃疡期降低。

关键词：复发性口疮 T淋巴细胞亚群抑制性静止期溃疡期比较研究

Accretion in strong field gravity with eXTp

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Science China(physics,Mechanics & Astronomy) 2019年第2期62卷 45-73页

作者： Alessandra De Rosa phil Uttley Lij.n Gou Yuan Liu Cosimo Bambi Didier Barret Tomaso Belloni Emanuele Berti Stefano Bianchi Ilaria Caiazzo piergiorgio Casella Marco Feroci Valeria Ferrari Leonardo Gualtieri j.remy Heyl Adam Ingram Vladimir Karas Fangj.n Lu Bin Luo Giorgio Matt Sara Motta j.seph Neilsen paolo pani Andrea Santangelo XinWen Shu j.nFeng Wang j.an-Min Wang YongQuan Xue Yupeng Xu WeiMin Yuan YeFei Yuan Shuang-Nan Zhang Shu Zhang Ivan Agudo Lorenzo Amati Nils Andersson Cristina Baglio pavel Bakala Altan Baykal Sudip Bhattacharyya Ignazio Bombaci NiccolóBucciantini Fiamma Capitanio Riccardo Ciolfi Wei K.Cui Filippo D'Ammando Thomas Dauser Melania Del Santo Barbara De Marco Tiziana Di Salvo Chris Done Michal Dovciak Andrew C.Fabian Maurizio Falanga Angelo Francesco Gambino Bruce Gendre Victoria Grinberg Alexander Heger j.roen Homan Rosario Iaria j.aChen j.ang ChiChuan j.n Elmar Koerding Manu Linares Zhu Liu Thomas j.Maccarone j.lien Malzac Antonios Manousakis Frédéric Marin Andea Marinucci Missagh Mehdipour Mariano Méndez Simone Migliari Cole Miller Giovanni Miniutti Emanuele Nardini paul T.O'Brien j.lian p.Osborne pierre Olivier petrucci Andrea possenti Alessandro Riggio j.rome Rodriguez Andrea Sanna Lij.ng Shao Malgosia Sobolewska Eva Sramkova Abigail L.Stevens Holger Stiele Giulia Stratta Zdenek Stuchlik j.ri Svoboda Fabrizio Tamburini Thomas M.Tauris Francesco Tombesi Gabriel Torok Martin Urbanec Frederic Vincent QingWen Wu Feng Yuan j.an j.M.in't Zand Andrzej.A.Zdziarski XinLin Zhou INAF-Istituto di Astrofisica e planetologie Spaziali Via Fosso del Cavaliere Anton pannekoek Institute for Astronomy University of Amsterdam National Astronomical Observatories Chinese Academy of Science Institute of High Energy physics Chinese Academy of Science Center for Field Theory and particle physics and Department of physics Fudan University IRAp Universitéde ToulouseCNRSUPSCNES INAF-Osservatorio Astronomico di Brera Department of physics and Astronomy The University of MississippiUniversity Dipartimento di Matematica e Fisica Universitàdegli studi Roma Tre University of British Columbia INAF-Osservatorio Astronomico di Roma INFN-Roma 2 c/o Dipartimento di Fisica II Universit?di Roma"Tor Vergata" Dipartimento di Fisica Universitàdegli Studi di Roma"La Sapienza"&Sezione INFN Roma1 Department of physics University of OxfordClarendon Laboratory Astronomical Institute Academy of Sciences School of Astronomy and Space Science Nanjing University MIT Kavli Institute for Astrophysics and Space Research Institut für Astronomie und Astrophysik Eberhard Karls Universität Department of physics Anhui Normal University Department of Astronomy and Institute of Theoretical physics and Astrophysics Xiamen University CAS Key Laboratory for Research in Galaxies and Cosmology Department of AstronomyUniversity of Science and Technology of China Instituto de Astrofísica de Andalucia(CSIC) Glorieta de la Astronomía s/n INAF-Istituto di Astrofisica Spaziale e Fisica cosmica di Bologna Mathematical Sciences and STAG Research Centre University of Southampton New York University Abu Dhabi Institute of physics and Research Centre for Computational physics and Data processing Faculty of Philosophy&ScienceSilesian University in OpavaíBezru?ovo nám. Department of physics Middle East Technical University Department of Astronomy and Astrophysics Tata Institute of Fundamental Research Dipartimento di Fisica Universit?di Pisa&INFN INAF-Osservatorio Astrofisico di Arcetri INAF-Osservatorio Astronomico di padova INFN-TIFpA Trento Ins

In this paper we describe the potential of the enhanced X-ray Timing and polarimetry(eXTp) mission for studies related to accretion flows in the strong field gravity regime around both stellar-mass and supermassive black-holes. eXTp has the unique capability of using advanced "spectral-timing-polarimetry" techniques to analyze the rapid variations with three orthogonal diagnostics of the flow and its geometry, yielding unprecedented insight into the inner accreting regions, the effects of strong field gravity on the material within them and the powerful outflows which are driven by the accretion process.

关键词： X-ray black holes physics accretion

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两种宫内节育器避孕效果比较

中国卫生产业 2015年第13期12卷 189-191页

作者：祖美娟三门峡市灵宝市计划生育服务站河南三门峡472500

目的比较安舒环和爱母环两种宫内节育器的临床避孕效果。方法对该站2012年1月—2014年1月收治400例自愿要求避孕的育龄妇女,按照自愿的原则,分为观察组和对照组,随访12个月,观察使用效果及不良反应。结果观察组200例,因症取出1例,占0.5%... 详细信息

目的比较安舒环和爱母环两种宫内节育器的临床避孕效果。方法对该站2012年1月—2014年1月收治400例自愿要求避孕的育龄妇女,按照自愿的原则,分为观察组和对照组,随访12个月,观察使用效果及不良反应。结果观察组200例,因症取出1例,占0.5%,脱落1例,占0.5%,续用195例,占97%;对照组200例,因症取出10例,占5%,脱落20例,占5.5%,续用170例,占85%,观察组因症取出率、脱落率低于对照组,续用率高于对照组,两组比较有统计学意义(pp>0.05);观察组术后1个月、3个月、6个月不良反应发生率分别为4.00%、3.50%、2.0%低于对照组16.00%、16.00%、7.00%,差异具有统计学意义(p<0.05)。结论安舒环避孕效果更好,不良反应发生率更低,且有助于降低远期妇科疾病发病风险。

关键词：安舒环爱母环宫内节育器