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Chinese Physics C 2016年第10期 915-915页

作者： C.Patrignani K.Agashe G.Aielli C.Amsler M.Antonelli D.M.Asner H.Baer sw.Banerjee R.M.Barnett T.Basaglia C.W.Bauer J.J.Beatty V.I.Belousov J.Beringer s.Bethke H.Bichsel O.Biebel E.Blucher G.Brooijmans O.Buchmueller V.Burkert M.A.Bychkov R.N.Cahn M.Carena A.Ceccucci A.Cerri D.Chakraborty M.-C.Chen R.s.Chivukula K.Copic G.Cowan O.Dahl G.D'Ambrosio T.Damour D.de Florian A.de Gouvea T.DeGrand P.de Jong G.Dissertori B.A.Dobrescu M.D'Onofrio M.Doser M.Drees H.K.Dreiner D.A.Dwyer P.Eerola s.Eidelman J.Ellis J.Erler V.V.Ezhela W.Fetscher B.D.Fields B.Foster A.Freitas H.Gallagher L.Garren H.-J.Gerber G.Gerbier T.Gershon T.Gherghetta A.A.Godizov M.Goodman C.Grab A.V.Gritsan C.Grojean D.E.Groom M.Grnewald A.Gurtu T.Gutsche H.E.Haber K.Hagiwara C.Hanhart s.Hashimoto Y.Hayato K.G.Hayes A.Hebecker B.Heltsley J.J.Hernandez-Rey K.Hikasa J.Hisano A.Hcker J.Holder A.Holtkamp J.Huston T.Hyodo K.Irwin J.D.Jackson K.F.Johnson M.Kado M.Karliner U.F.Katz s.R.Klein E.Klempt R.V.Kowalewski F.Krauss M.Kreps B.Krusche Yu.V.Kuyanov Y.Kwon O.Lahav J.Laiho P.Langacker A.Liddle Z.Ligeti C.-J.Lin C.Lippmann T.M.Liss L.Littenberg K.s.Lugovsky s.B.Lugovsky A.Lusiani Y.Makida F.Maltoni T.Mannel A.V.Manohar W.J.Marciano A.D.Martin A.Masoni J.Matthews U.-G.Meiβner D.Milstead R.E.Mitchell P.Molaro K.Mnig F.Moortgat M.J.Mortonson H.Murayama K.Nakamura M.Narain P.Nason s.Navas M.Neubert P.Nevski Y.Nir K.A.Olive s.Pagan Griso J.Parsons J.A.Peacock M.Pennington s.T.Petcov V.A.Petrov A.Piepke A.Pomarol A.Quadt s.Raby J.Rademacker G.Raffelt B.N.Ratcliff P.Richardson A.Ringwald s.Roesler s.Rolli A.Romaniouk L.J.Rosenberg J.L.Rosner G.Rybka R.A.Ryutin C.T.sachrajda Y.sakai G.P.salam s.sarkar F.sauli O.schneider K.scholberg A.J.schwartz D.scott V.sharma s.R.sharpe T.shutt M.silari T.sjstrand P.skands T.skwarnicki J.G.smith G.F.smoot s.spanier H.spieler C.spiering A.stahl s.L.stone Y.sumino T.sumiyoshi M.J.syphers F.Takahashi M.Tanabashi K.Terashi J.Terning R.s.Thorne L.Tiator M.Titov N.P.Tkachenko N.A.Trnqvist D.Tovey G.Valencia R.Van de Water N.Varelas G Particle Data Group Universita di Bologna and INFN dip.scienze per la Qualita della Vita University of Maryland Department of Physics College Park Universit degli studi di Roma "Tor Vergata" Albert Einstein Center for Fundamental Physics Universitt Bern stefan Meyer Institute for subatomic Physics Austrian Academy of sciences Lab.Nazionali di Frascati dell'INFN Pacific Northwest National Laboratory Department of Physics and Astronomy University of Oklahoma University of Louisville Physics Division Lawrence Berkeley National Laboratory CERN European Organization for Nuclear Research Department of Physics The Ohio state University COMPAs Group Institute for High Energy Physics Max-Planck-Institute of Physics Department of Physics University of Washington Ludwig-Maximilians-Universitt Fakultt fr Physik Enrico Fermi Institute and Department of Physics University of Chicago Department of Physics Columbia University High Energy Physics Group Blackett Laboratory Imperial College Jefferson Lab Department of Physics University of Virginia Fermi National Accelerator Laboratory Kavli Institute for Cosmological Physics University of Chicago Department of Physics and Astronomy University of sussex Department of Physics Northern Illinois University Department of Physics and Astronomy University of California Michigan state University Dept.of Physics and Astronomy Department of Physics Royal Holloway University of London INFN-sezione di Napoli Complesso Universitario Monte sant'Angelo Institut des Hautes Etudes scientifiques International Center for Advanced studies(ICAs) UNsAM Department of Physics and Astronomy Northwestern University Department of Physics University of Colorado at Boulder Nikhef P.O.Box 41882 1009 DB Amsterdam and University of Amsterdam Institute for Particle Physics ETH Zurich University of Liverpool Department of Physics Oliver Lodge Lab Physikalisches Institut Universitt Bonn Helsinki Institute of Physics University of Helsinki Department of Physics Budker Institute of Nuclear Physics sB RAs Novosib

The Review summarizes much of particle physics and *** data from previous editions,plus 3,062 new measurements from 721 papers,we list,evaluate,and average measured properties of gauge bosons and the recently discovered Higgs boson,leptons,quarks,mesons,and *** summarize searches for hypothetical particles such as supersymmetric particles,heavy bosons,axions,dark photons,*** the particle properties and search limits are listed in summary *** also give numerous tables,figures,formulae,and reviews of topics such as Higgs Boson Physics,supersymmetry,Grand Unified Theories,Neutrino Mixing,Dark Energy,Dark Matter,Cosmology,Particle Detectors,Colliders,Probability and *** the 117 reviews are many that are new or heavily revised,including new reviews on Pentaquarks and Inflation.

关键词： CA Organization Chinese Physics C UsA DEsY CERN

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Latest results from GRAAL collaboration

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Chinese Physics C 2009年第12期33卷 1249-1253页

作者： V. Vegna V. Bellini J.P. Bouquet L. Casano A. D'Angelo J.P. Didelez R. Di salvo A. Fantini D. Franco G. Gervino F. Ghio G. Giardina B. Girolami A. Giusa M. Guidal E. Hourany A.s. Ignatov R. Kunnel A. Lapik A. Lleres P. Levi sandri F. Mammoliti G. Mandaglio M. Manganaro M. Moricciani A.N. Mushkarenkov V.G. Nedorezov C. Randieri D. Rebreyend N.V. Rudnev G. Russo C. schaerf M.L. sperduto M.C. sutera A.Turinge dip. di Fisica Università degli Studi di Roma 'Tor Vergata' via della Ricerca Scientifica 1 I-00133 Roma Italy INFN - sezione di Roma 'Tor Vergata' via della Ricerca Scientifica 1 I-00133 Roma Italy dip. di Fisica e Astronomia Università di Catania via Santa Sofia 44 I-95123 Catania Italy INFN - sezione di Catania via Santa Sofia 44 I-95123 Catania Italy LPsC Universit Joseph Fourier Grenoble 1 CNRS/IN2P3 Institut National Polytechnique de Grenoble 53 Avenue des Martyres 38026 Grenoble France IPNO Universit de Paris-Sud 11 CNRS/IN2P3 15 rue Georges Clemenceau 91406 Orsay France dip. di Fisica sperimentale Università di Torino via P.Giuria I-00125 Torino Italy INFN - sezione di Torino via P.Giuria I-00125 Torino Italy Istituto superiore di sanità viale Regina Elena 299 I-00161 Roma Italy INFN - sezione di Roma piazzale Aldo Moro 2 I-00185 Roma Italy dip. di Fisica Universitàdi Messina salita Sperone 31 I-98166 Messina Italy Institute for Nuclear Research RAS 117312 Moscow Russia INFN - Laboratori Nazionali di Frascati via E.Fermi 40 I-00044 Frascati Italy INFN - sezione di Catania via Santa Sofia 44 I-95123 Catania Italy

The GRAAL experimental set-up consists of a polarized and tagged photon beam that covers an energy range from a minimum of 600 MeV up to a maximum of 1500 MeV, of a liquid Hydrogen or Deuterium target and of the 4π Lagrange detector optimized for photon detection. It allows the study of pseudo-scalar and vector meson photoproduCtion on the nucleon in the energy range corresponding to the second and the third resonance regions. In the following, the ∑ beam asymmetries in η and π0 photoproduction on quasi-free nucleon are shown. Also single and double polarization observables in K＋A photoproduction on free proton are shown; they are important to confirm the role of new or poorly known resonances in the 1900 MeV mass region.

关键词： polarized photon meson photoproduction polarization observables

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Hydrocarbon Play Assessment of “Oswil” Field, Onshore Niger Delta Region

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Journal of Geological Research 2021年第1期3卷 11-21页

作者： Osisanya,W.O. Alile,O.M. Eze,s.U. Ibitoye,T.A. Oyanameh,O.E. Department of Physics University of BeninBenin CityEdo stateNigeria Department of Marine Geology Nigeria Maritime UniversityOkerenkokoDelta State Department of Petroleum Engineering and Geosciences Petroleum Training InstituteEffurunNigeria Department of Earth science Anchor UniversityLagosNigeria

Hydrocarbon play assessment of any field involves the evaluation of the production capacity of hydrocarbon reservoir unit in the *** involves detail study of the reservoir petrophysical properties and geological interpretation of structures suitable for hydrocarbon accumulation in the field as observed from seismic reflection *** study details the assessment of hydrocarbon play in OsWIL field onshore in Niger Delta,with the intent of appraising its productivity using a combination of seismic,well logs,petrophysical parameters and volumetric estimation using proven techniques which involves an integrated *** reservoir windows“R1”and“R2”were defined from five wells OsWIL-02,04,06,07 and *** top and base of each reservoir window was delineated from the *** interpretation for inline 6975 revealed two horizons(X and Y)and eight faults labelled(F1,F2,F6,F8,F10,F16,F17 and F18).Five faults(F1,F6,F10,F17 and F18)were identified as synthetic faults and dip basin wards while three faults(F2,F8 and F16)were identified as antithetic faults and dips ***-depth structural map at top of reservoirs R1 and R2 revealed structural highs and *** observations are characteristics of growth structures(faults)which depicts the tectonic style of the Niger *** of petrophysical evaluation for reservoirs“R1”and“R2”across the five wells were *** reservoir“R1”effective porosity values of 27%,26%,23%,20%and 22%were obtained for wells OsWIL-04,12,07,06 and 02 respectively with an average of 23.6%,while for reservoir“R2”effective porosity values of 26%,22%,21%,24%and 23%for wells OsWIL-04,12,07,06 and 02 were obtained respectively with an average of 23.2%.This porosity values correspond with the already established porosity range of 28-32%within the Agbada formation of the Niger *** index of the order(K>100mD)were obtained for both reservoirs across the five wells and is rated very *** sat

关键词： seismic Well logs Petrophysical parameters Hydrocarbon play structural interpretation Niger Delta

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Weak measurements and quantum-to-classical transitions in free electron-photon interactions

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Light(science & Applications) 2023年第11期12卷 2519-2529页

作者： Yiming Pan Eliahu Cohen Ebrahim Karimi Avraham Gover Norbert schönenberger TomášChlouba Kangpeng Wang saar Nehemia Peter Hommelhoff Ido Kaminer Yakir Aharonov school of Physical science and Technology and Center for Transformative science ShanghaiTech UniversityShanghai 200031China Department of Electrical Engineering TechnionHaifa 3200003Israel Department of Physics of Complex systems Weizmann Institute of ScienceRehovot 7610001Israel Faculty of Engineering and the Institute of Nanotechnology and Advanced Materials Bar Ilan UniversityRamat Gan 5290002Israel Department of Physics University of OttawaOttawaOntario K1N 6N5Canada Department of Electrical Engineering Physical Electronics Center for Laser-Matter Interaction(LMI)Tel Aviv UniversityRamat Aviv 6997801Israel Department of Physics Friedrich-Alexander Universität Erlangen-Nürnberg(FAU)Staudtstraße 191058 ErlangenGermany school of Physics and Astronomy Tel Aviv UniversityRamat Aviv 6997801Israel Institute for Quantum studies Chapman UniversityOrangeCA 92866USA

How does the quantum-to-classical transition of measurement occur?This question is vital for both foundations and applications of quantum ***,we develop a new measurement-based framework for characterizing the classical and quantum free electron-photon interactions and then experimentally test *** first analyze the transition from projective to weak measurement in generic light-matter interactions and show that any classical electron-laserbeam interaction can be represented as an outcome of weak *** particular,the appearance of classical point-particle acceleration is an example of an amplified weak value resulting from weak measurement.A universal factor,exp(-Γ^(2)=2),quantifies the measurement regimes and their transition from quantum to classical,whereΓcorresponds to the ratio between the electron wavepacket size and the optical *** measurement-based formulation is experimentally verified in both limits of photon-induced near-field electron microscopy and the classical acceleration regime using a *** results shed new light on the transition from quantum to classical electrodynamics,enabling us to employ the essence of the wave-particle duality of both light and electrons in quantum measurement for exploring and applying many quantum and classical light-matter interactions.

关键词： quantum photon acceleration

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Prevalence of Circadian Blood Pressure Patterns and Factors Associated with Non-dipping among Black Patients with Untreated and Treated Hypertension: A Cross-sectional study

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World Journal of Cardiovascular Diseases 2017年第11期7卷 399-412页

作者： T. s. Mvunzi Y. Lubenga F. B. Lepira J. R. Makulo A. Nkodila D. K. Kuntonda Y. samafundu Y. M. Nlandu Y. M. Engole B. P. Kianu F. Kintoki D. Mupepe N. Buila R. M. Kongo E. V. Kintoki Division of Cardiology University of Kinshasa Hospital Kinshasa Congo Division of nephrology Department of Internal Medicine University of Kinshasa Hospital Kinshasa Congo Centre medical cite des aveugles University of Kinshasa Hospital Kinshasa Congo Clinique ngaliema University of Kinshasa Hospital Kinshasa Congo

Objective: To determine the prevalence of circadian BP patterns and to assess factors associated with the non-dipping pattern in untreated and treated hypertensive patients, studied separately. Methods: Clinical data and ABPM were obtained from 52 untreated and 168 treated hypertensive patients referred for ABPM to Monkole Hospital in Kinshasa. Twenty-four ABPM was performed using an oscillometric device. Non-dipping pattern encompasses non-dipping (nocturnal systolic BP dip less than 10% of daytime systolic BP) and reverse dipping (mean night sBP higher than the day sBP). Results: the prevalence of non-dipping pattern was 75% (63.5% non-dipping and 11.5% reverse dipping) and 70% (60.1% non-dipping and 10.1% reverse dipping) in untreated and treated hypertensive patients, respectively. Advanced age (adjusted OR 1.80;95%CI 1.96 - 3.38;p = 0.015), female sex (adjusted OR 2.28;95%CI 1.19 - 4.36;p = 0.013), diabetes (adjusted OR 5.06;95%CI 1.38 - 6.95;p = 0.014), reduced kidney function (adjusted OR 3.10;95%CI 1.50 - 6.43;p = 0.018), inflammation (adjusted OR 2.65;95%CI 1.76 - 6.48;p = 0.031), LVH (adjusted OR 4.45;95%CI 1.78 - 7.67;p = 0.024) and antihypertensive therapy (adjusted OR 0.19;95%CI 0.12 - 0.64;p = 0.018) emerged as the main independent factors significantly associated with the non-dipping pattern in the study population. Conclusion: the non-dipping pattern was a common finding in studied patients and associated with traditional and emerging risk factors suggesting that this abnormal pattern could be a marker of high cardiovascular risk.

关键词： Non-dipping Prevalence Risk Factors Hypertension Black Africans

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日珥磁场结构的Rayleigh-Tayler不稳定性和无黑子双带耀斑

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天文学报 1982年第3期 203-210页

作者：曹天君许敖敖成中杰中国科学院紫金山天文台南京大学天文系美国海军实验室

本文根据无黑子双带耀斑发生前暗条周围色球纤维形态的观测特征,讨论了这类耀斑的储能过程。文中还讨论了这类日珥磁场结构的不稳定性问题。当宁静日珥中磁场梯度和顶部磁力线曲率超过一定的阈值时,会引起日珥磁场结构中的Rayleigh-Tay... 详细信息

本文根据无黑子双带耀斑发生前暗条周围色球纤维形态的观测特征,讨论了这类耀斑的储能过程。文中还讨论了这类日珥磁场结构的不稳定性问题。当宁静日珥中磁场梯度和顶部磁力线曲率超过一定的阈值时,会引起日珥磁场结构中的Rayleigh-Tayler不稳定性的发生,导致暗条突然消失,发生这种不稳定性时,日珥支撑磁场中会产生中性电流片,并能引起两边的磁流向中心部分集中。磁力线的快速重连导致双带耀斑的产生。

关键词：双带耀斑暗条活动区磁场电流片 Rayleigh-Tayler 不稳定性

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药物诱导帕金森病患者的心肌123I-MIBG闪烁扫描检查

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世界核心医学期刊文摘(神经病学分册) 2006年第8期 61-61页

作者： Lee P.H. Kim J.s. shin D.H 樊慧婷 Department of Neurology College of Medicine Ajou University Woncheon- dong san 5 suwon Kyungki- do 442- 749 south Korea Dr.

Cardiac sympathetic dysfunction was investigated using 123Imetaiodobenzylguanidine (MIBG) myocardial scintigraphy in 20 patients with drug induced parkinsonism (dip). The mean heart to mediastinum ratio was significantly greater in patients with dip than in those with Parkinson’s disease (mean (sD): 2.07 (0.39) v 1.28 (0.15), p s not different between the dip patients and controls. Two dip patients whose MIBG uptake was significantly reduced showed persistent parkinsonism and responded dramatically to levodopa.

关键词：帕金森病药物诱导 I-MIBG 患者心肌

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Anchor钉重建伸肌腱止点治疗锤状指

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临床和实验医学杂志 2006年第12期5卷 1939-1940页

作者：陆大明陆振良徐雪平张振文昆山市第一人民医院骨科江苏昆山215300

目的探讨治疗锤状指的手术方法。方法对12例锤状指的患者采用Anchor钉重建伸肌腱止点的手术方法治疗。结果术后随访2-12个月，11例患者于术后6周左右复查X线片均未见骨锚松动、脱落；术后8周远侧指间关节活动自如。结论使用Anchor钉... 详细信息

目的探讨治疗锤状指的手术方法。方法对12例锤状指的患者采用Anchor钉重建伸肌腱止点的手术方法治疗。结果术后随访2-12个月，11例患者于术后6周左右复查X线片均未见骨锚松动、脱落；术后8周远侧指间关节活动自如。结论使用Anchor钉重建伸肌腱止点治疗锤状指，具有操作简单、肌腱修复可靠、术后并发症少的优点，是一种值得推广的手术方法。

关键词： Anchor钉锤状指手术治疗

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Observatory science with eXTP

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science China(Physics,Mechanics & Astronomy) 2019年第2期62卷 97-138页

作者： Jean J.M.in 't Zand Enrico Bozzo JinLu Qu Xiang-Dong Li Lorenzo Amati Yang Chen Immacolata Donnarumma Victor Doroshenko stephen A.Drake Margarita Hernanz Peter A.Jenke Thomas J.Maccarone simin Mahmoodifar Domitilla de Martino Alessandra De Rosa Elena M.Rossi Antonia Rowlinson Gloria sala Giulia stratta Thomas M.Tauris Joern Wilms XueFeng Wu Ping Zhou Iván Agudo Diego Altamirano Jean-Luc Atteia Nils A.andersson M.Cristina Baglio David R.Ballantyne Altan Baykal Ehud Behar Tomaso Belloni s.dip bh.ttach.ryya stefano Bianchi Anna Bilous Pere Blay Joao Braga sφren Brandt Edward F.Brown Niccolo Bucciantini Luciano Burderi Edward M.Cackett Riccardo Campana sergio Campana Piergiorgio Casella Yuri Cavecchi Frank Chambers Liang Chen Yu-Peng Chen Jér?me Chenevez Maria Chernyakova ChiChuan Jin Riccardo Ciolfi Elisa Costantini Andrew Cumming Antonino D'Aì Zi-Gao Dai Filippo D'Ammando Massimiliano De Pasquale Nathalie Degenaar Melania Del santo Valerio D'Elia Tiziana Di salvo Gerry Doyle Maurizio Falanga XiLong Fan Robert D.Ferdman Marco Feroci Federico Fraschetti Duncan K.Galloway Angelo F.Gambino Poshak Gandhi MingYu Ge Bruce Gendre Ramandeep Gill Diego G?tz Christian Gouiffès Paola Grandi Jonathan Granot Manuel Güdel Alexander Heger Craig O.Heinke Jeroen Homan Rosario Iaria Kazushi Iwasawa Luca Izzo Long Ji Peter G.Jonker Jordi José Jelle s.Kaastra Emrah Kalemci Oleg Kargaltsev Nobuyuki Kawai Laurens Keek stefanie Komossa Ingo Kreykenbohm Lucien Kuiper Devaky Kunneriath Gang Li En-Wei Liang Manuel Linares Francesco Longo FangJun Lu Alexander A.Lutovinov Denys Malyshev Julien Malzac Antonios Manousakis Ian McHardy Missagh Mehdipour YunPeng Men Mariano Méndez Roberto P.Mignani Romana Mikusincova M.Coleman Miller Giovanni Miniutti Christian Motch Joonas Nättilä Emanuele Nardini Torsten Neubert Paul T.O'Brien Mauro Orlandini Julian P.Osborne Luigi Pacciani stéphane Paltani Maurizio Paolillo Iossif E.Papadakis Biswajit Paul Alberto Pellizzoni Uria Peretz Miguel A.Pérez Torres Emanuele Perinati Chanda Prescod-Weinstein Pablo Reig sRON Netherlands Institute for space Research Department of Astronomy University of Geneva Key Laboratory for Particle Astrophysics Institute of High Energy PhysicsChinese Academy of Sciences school of Astronomy and space science Nanjing University INAF-IAsF Bologna AsI Via del Politecnico snc INAF-Istituto di Astrofisica e Planetologie spaziali Institut für Astronomie und Astrophysik Tübingen Universit?t Tübingen NAsA Goddard space Flight Center ICREA&Institute of space sciences(IEEC-CsIC) Campus UABCarrer de Can Magrans CsPAR SPA University of Alabama in Huntsville Department of Physics Texas Tech University INAF Osservatorio Astronomico di Capodimonte Leiden Observatory Leiden University Anton Pannekoek Institute University of Amsterdam AsTRON Netherlands Institute for Radio Astronomy Universitat Politecnica de Catalunya(UPC-IEEC) Universitádegli studi di Urbino‘Carlo Bo’ Max-Planck-Institut für Radioastronomie Dr.Karl-Remeis-sternwarte and Erlangen Centre for Astroparticle Physics(ECAP) Friedrich Alexander Universit?t Erlangen-Nurnberg Purple Mountain Observatory Chinese Academy of Sciences Instituto de Astrofysíca de Andalucia-CsIC Department of Physics and Astronomy University of Southampton IRAP Universitéde ToulouseCNRSUPSCNES Mathematical sciences and sTAG Research Centre University of Southampton New York University Abu Dhabi Center for Relativistic Astrophysics School of PhysicsGeorgia Institute of Technology Physics Department Middle East Technical University Department of Physics Technion-Israel Institute of Technology INAF Osservatorio Astronomico di Brera Tata Institute of Fundamental Research dipartimento di Matematica e Fisica Universitàdegli Studi Roma Tre Instituto de Astrofísica de Canarias Instituto Nacional de Pesquisas Espaciais-INPE National space Institute Technical University of Denmark(DTU Space) Department of Physics and Astronomy Michigan State University INAF Osservatorio Astrofisico di Arcetri dipartimento di Fisica Universitádegli Studi di Cagliari Department of Physics and A

In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry(eXTP) mission for studies related to Observatory science targets. These include flaring stars, supernova remnants, accreting white dwarfs, low and high mass X-ray binaries, radio quiet and radio loud active galactic nuclei, tidal disruption events, and gamma-ray bursts. eXTP will be excellently suited to study one common aspect of these objects: their often transient nature. Developed by an international Consortium led by the Institute of High Energy Physics of the Chinese Academy of science, the eXTP mission is expected to be launched in the mid 2020s.

关键词： space research in struments nuclear astrophysics flare stars accretion and accretion disks mass loss and stellar winds cataclysmic binaries X-ray binaries supernova remnants active galactic nuclei X-ray bursts gamma-ray bursts gravitational waves

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