Investigation of Molecular Assisted Recombination Detachment Physics in Fusion Relevant Hydrogen Plasmas
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Screening of High-Z Grains and Related Phenomena in Colloidal Plasmas
Condensed Matter Physics, 2003, Vol. 6, No. 3(35), pp. 425–445 Screening of high-Z grains and related phenomena in colloidal plasmas O.Bystrenko, T.Bystrenko, A.Zagorodny Bogolyubov Institute for Theoretical Physics, 03143 Kiev, Ukraine Received April 3, 2003 Recent important results are briefly presented concerning the screening of high-Z impurities in colloidal plasmas. The review focuses on the phe- nomenon of nonlinear screening and its effects on the structure of colloidal plasmas, the role of trapped ions in grain screening, and the effects of strong collisions in the plasma background. It is shown that the above ef- fects may strongly modify the properties of the grain screening giving rise to considerable deviations from the conventional Debye-Huc¨ kel theory as dependent on the physical processes in the plasma background. Key words: high-Z impurity, charged colloidal suspension, dusty plasma, nonlinear screening, bound ionic states, strong collisions PACS: 52.25.Vy, 52.27.Lw, 52.65.-y 1. Introduction Screening of charged objects embedded in a plasma background is one of the important problems of plasma physics, which attracted the attention of researchers during decades. Our interest in this issue is connected, first of all, with its im- plications in spatial ordering phenomena in colloidal plasmas (CP) such as dusty plasmas (DP) or charged colloidal suspensions (CCS). CP consist of a large number of highly charged (Z 103 105) colloidal particles of submicron size immersed in a plasma background.'Experimen− ts have revealed a number of collective effects in CP, in particular, the formation of Coulomb liquids or crystals associated with the strong Coulomb coupling in the colloidal subsystem [1{5]. -
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On the Stability of Gold Nanoparticles Synthesized by Laser Ablation In
Journal of Colloid and Interface Science 489 (2017) 47–56 Contents lists available at ScienceDirect Journal of Colloid and Interface Science journal homepage: www.elsevier.com/locate/jcis On the stability of gold nanoparticles synthesized by laser ablation in liquids ⇑ ⇑ Gerardo Palazzo a,c, , Gabriele Valenza a,b, Marcella Dell’Aglio b, Alessandro De Giacomo a,b, a Department of Chemistry, University of Bari, via Orabona 4, 70125 Bari, Italy b CNR-NANOTEC, Istituto di Nanotecnologia, Via amendola 122/d, 70125 Bari, Italy c CSGI (Center for Colloid and Surface Science) c/o Dept. Chemistry, via Orabona 4, 70125 Bari, Italy graphical abstract article info abstract Article history: ‘‘Naked” gold nanoparticles (AuNPs), synthesized in the absence of any capping agents, prepared by Received 5 July 2016 pulsed laser ablation in liquid (PLAL) are stabilized by negative charges. Common explanations for this Revised 2 September 2016 phenomenon involve the presence of gold oxides and/or the anion adsorption. We have found that Accepted 10 September 2016 AuNP ablated in solutions of acids with very different oxidation power, viz. HCl, H SO , HNO share Available online 12 September 2016 2 4 3 the same size and f-potential. Although, gold oxides have pKas 4, the f-potential of AuNPs ablated in solutions with pH 6 4 is always negative. Keywords: These evidences suggest that the gold oxidation and anion adsorptions have only a minor role on building Pulsed laser ablation in liquids the negative surface potential and we hypothesize, for the first time, that excess electrons formed within Colloidal stability Zeta-potential the plasma phase could charge the metallic particles. -
DIELECTRONIC RECOMBINATION DATA for ASTROPHYSICAL APPLICATIONS: PLASMA RATE-COEFFICIENTS for Feq+ (Q = 7–10, 13–22) and Ni25+ IONS from STORAGE-RING EXPERIMENTS
INTERNATIONAL REVIEW OF ATOMIC AND MOLECULAR PHYSICS (IRAMP) Volume 1, No. 2, July-December 2010, pp. 109-121, © International Science Press, ISSN: 2229-3159 REVIEW ARTICLE DIELECTRONIC RECOMBINATION DATA FOR ASTROPHYSICAL APPLICATIONS: PLASMA RATE-COEFFICIENTS FOR Feq+ (q = 7–10, 13–22) AND Ni25+ IONS FROM STORAGE-RING EXPERIMENTS .. S. SCHIPPERS1, M. LESTINSKY2,3, A. MULLER1, D.W. SAVIN3, E.W. SCHMIDT1 AND A. WOLF2 1Institut für Atom- und Molekülphysik, Justus-Liebig-Universität Giessen, Leihgesterner Weg 217, 35392 Giessen, Germany. 2Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany. 3Columbia Astrophysics Laboratory, Columbia University, 550 West 120th, New York, NY 10027, USA. Abstract: This review summarizes the present status of an ongoing experimental effort to provide reliable rate coefficients for dielectronic recombination of highly charged iron ions for the modeling of astrophysical and other plasmas. The experimental work has been carried out over more than a decade at the heavy-ion storage-ring TSR of the Max-Planck- Institute for Nuclear Physics in Heidelberg, Germany. The experimental and data reduction procedures are outlined. The role of previously disregarded processes such as fine-structure core excitations and trielectronic recombination is highlighted. Plasma rate coefficients for dielectronic recombination of Feq+ ions (q = 7–10, 13–22) and Ni25+ are presented graphically and in a simple parameterized form allowing for easy use in plasma modeling codes. It is concluded that storage-ring experiments are presently the only source for reliable low-temperature dielectronic recombination rate-coefficients of complex ions. PACS Numbers: 34.80.Lx, 52.20.Fs. 1. INTRODUCTION for Nuclear Physics in Heidelberg, Germany. -
Wavesurfer 510 Oscilloscopes Operator's Manual
Operator's Manual WaveSurfer 510 Oscilloscopes WaveSurfer 510 Oscilloscope Operator's Manual © 2017 Teledyne LeCroy, Inc. All rights reserved. Unauthorized duplication of Teledyne LeCroy, Inc. documentation materials other than for internal sales and distribution purposes is strictly prohibited. However, clients are encouraged to duplicate and distribute Teledyne LeCroy, Inc. documentation for their own internal educational purposes. WaveSurfer and Teledyne LeCroy, Inc. are trademarks of Teledyne LeCroy, Inc., Inc. Other product or brand names are trademarks or requested trademarks of their respective holders. Information in this publication supersedes all earlier versions. Specifications are subject to change without notice. 928228 Rev B May 2017 Contents Safety 1 Symbols 1 Precautions 1 Operating Environment 2 Cooling 2 Cleaning 2 Power 3 Oscilloscope Overview 5 Front of Oscilloscope 5 Side of Oscilloscope 6 Back of Oscilloscope 7 Front Panel 8 Signal Interfaces 11 Oscilloscope Set Up 13 Powering On/Off 13 Software Activation 13 Connecting to Other Devices/Systems 14 Language Selection 15 Using MAUI 17 Touch Screen 17 OneTouch Help 24 Working With Traces 31 Zooming 34 Print/Screen Capture 36 Acquisition 37 Auto Setup 37 Viewing Status 38 Vertical 38 Digital (Mixed Signal) 42 Timebase 45 Trigger 52 Display 63 Display Set Up 64 Persistence Display 66 i WaveSurfer 510 Oscilloscope Operator's Manual Math and Measure 69 Cursors 69 Measure 72 Math 79 Memory 91 Analysis Tools 93 WaveScan 93 Pass/Fail Testing 97 Saving Data (File Functions) -
Australian Journal of Physics
CSIRO PUBLISHING Australian Journal of Physics Volume 51, 1998 © CSIRO 1998 A journal for the publication of original research in all branches of physics www.publish.csiro.au/journals/ajp All enquiries and manuscripts should be directed to Australian Journal of Physics CSIRO PUBLISHING PO Box 1139 (150 Oxford St) Collingwood Telephone: 61 3 9662 7626 Vic. 3066 Facsimile: 61 3 9662 7611 Australia Email: [email protected] Published by CSIRO PUBLISHING for CSIRO and the Australian Academy of Science Aust. J. Phys., 1998, 51, 763–834. One-dimensional Self-organised Structures in Dusty Plasmas V. N. Tsytovich General Physics Institute, Russian Academy of Science, Vavilova Str. 38, Moscow, 117942, Russia. [email protected], [email protected]. Contents Abstract 764 Part I. Introduction to Elementary Dusty Plasma Physics, Kinetic and Hydrodynamic Description of Dusty Plasmas 764 1. Dusty Plasma as a New State of Matter 764 2. Main Physical Mechanisms of Dust–Dust Interactions, Attraction and Repulsion in Plasmas 767 3. General Theoretical Concepts, Kinetic and Hydrodynamic Descriptions of Dusty Plasmas 771 4. Some Useful Relations in Dusty Plasma Physics 773 5. Some New Computational Results 782 Part II. One-dimensional Structures in Dusty Plasmas 790 6. Introduction to Concept of Dust–Plasma Structures 790 7. 1D Self-organised Dust–Plasma Structures 793 8. Numerical Results for 1D Dust Structures 798 9. Spherical Self-organised Structures 805 10. Some Problems of Dust Structures 808 Part III. Shocks in Dusty Plasmas 809 11. Introduction to Shock Physics in Dusty Plasmas 809 12. General Nonlinear Equations and Conservation of Total Mass, Total Momentum and Total Energy Densities 810 13. -
Pipenightdreams Osgcal-Doc Mumudvb Mpg123-Alsa Tbb
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Table of Contents (Online)
PERIODICALS PHYSICAL REVIEW B Postmaster send address changes to: For editorial and subscription correspondence, APS Subscription Services please see inside front cover Suite 1NO1 „ISSN: 1098-0121… 2 Huntington Quadrangle Melville, NY 11747-4502 THIRD SERIES, VOLUME 73, NUMBER 3 CONTENTS JANUARY 2006-15(I) Physical Review B Editorial Policies and Practices ................................................... iii Physical Review B Information for Contributors ..................................................... vii Subject Matter Categories for Physical Review B .................................................... x BRIEF REPORTS Electronic structure: wide-band, narrow-band, and strongly correlated systems Thermodynamic and transport properties of YTe3, LaTe3, and CeTe3 (4 pages) ......................... 033101 N. Ru and I. R. Fisher X-ray anomalous scattering investigation of BaVS3 (4 pages) ........................................ 033102 Sébastien Fagot, Pascale Foury-Leylekian, Sylvain Ravy, Jean-Paul Pouget, Émilio Lorenzo, Yves Joly, Martha Greenblatt, Maxim V. Lobanov, and Guerman Popov Interaction of polarized light with three-dimensional opal-based photonic crystals (4 pages) ............... 033103 A. V. Baryshev, A. B. Khanikaev, H. Uchida, M. Inoue, and M. F. Limonov Low-threshold and high-efficiency optical parametric oscillator using a one-dimensional single-defect photonic crystal with quadratic nonlinearity (4 pages) ...................................................... 033104 Fang-Fang Ren, Rui Li, Chen Cheng, Jing Chen, -
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Ultrashort Optical Pulse Propagators
Ultrashort Optical Pulse Propagators Jerome V Moloney Arizona Center for Mathematical Sciences University of Arizona, Tucson Lecture I. From Maxwell to Nonlinear Schrödinger Lecture II. A Unidirectional Maxwell Propagator Lecture III. Relation to other Propagators and Applications An Artists Rendering - New Scientist, February 19, 2000 From Linear to Extreme NLO Light string propagation in air. Maxwell Equations I Maxwell’s Equations G GG∂B ∇×ED=− ; ∇• = ρ ∂t G GG∂D G ∇×Hj= + ;0∇•B= ∂t Constitutive Relations G GGGG B = µε00HD; =+EP G G Polarization P () rt , couples light to matter. Maxwell Equations II Vector Wave Equation G G GG22 2 11∂ EP∂ ∇−EE22−∇()∇• = 22 ct∂ ε0c∂t Note: Most pulse propagationG models derived from Maxwell assume that ∇∇ () • E = 0 . Coupling between field components can only occur via nonlinear polarization i.e. nonlinear birefringence. GGG GGG P(rt,,) =+PLN(rt) PL(rt,) Maxwell Equations III Linear and Nonlinear Polarization Models GGGG+∞ GGGGGG Pr,,t=−ε χτ()1 rt Er,τdτ⇔Pr,ω=εχr,ωEr,ω L () 00∫ ()() ()()() −∞ GGGG GGGGG Pr,,t=−ε χτ(3) rt ,t−τ,t−τEr,τEr,τEr,τdτdτdτ NL () 01∫∫∫ ( 23) ( 1) ( 2) ( 3) 123 8 3 GGGGGGG G G χω()()rE,,ω,ω()r,ωE(r,ω)E()r,ω Pr,ωε= 123 1 2 3 NL ()0 ∫∫∫ δω()12++ω ω3−ωddω1ω2dω3 Practically, the linear polarization response is treated at some approximate level – nonlinear polarization is assumed to be instantaneous (Kerr) with a possible delayed (Raman) term. For ultra wide bandwidth pulses even linear dispersion is nontrivial to describe! Maxwell Equations III Some nonlinear polarization models: -
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A&A 557, A2 (2013) Astronomy DOI: 10.1051/0004-6361/201220628 & c ESO 2013 Astrophysics Experimental rate coefficients of F5+ recombining into F4+ S. Ali1,3,I.Orban1,S.Mahmood1,S.D.Loch2, and R. Schuch1 1 Department of Physics, Stockholm University, AlbaNova 10691 Stockholm, Sweden e-mail: [email protected] 2 Department of Physics, Auburn University, Auburn, AL 36849, USA 3 Department of Physics, University of Gujrat, 50700 Gujrat, Pakistan Received 25 October 2012 / Accepted 19 May 2013 ABSTRACT Recombination spectra of F5+ producing F4+ have been investigated with high-energy resolution, using the CRYRING heavy-ion stor- age ring. The absolute recombination rate coefficients are derived in the centre-of-mass energy range of 0−25 eV. The experimental results are compared with intermediate-coupling AUTOSTRUCTURE calculations for 2s−2p (n = 0) core excitation and show very good agreement in the resonance energy positions and intensities. Trielectronic recombination with 2s2−2p2 transitions are clearly identified in the spectrum. Contributions from F5+ ions in an initial metastable state are also considered. The energy-dependent re- combination spectra are convoluted with Maxwell-Boltzmann energy distribution in the 103−106 K temperature range. The resulting temperature-dependent rate coefficients are compared with theoretical results from the literature. In the 103−104 K range, the calcu- lated data significantly underestimates the plasma recombination rate coefficients. Above 8 × 104 K, our AUTOSTRUCTURE results and plasma rate coefficients from elsewhere show agreement that is better than 25% with the experimental results. Key words. atomic data – atomic processes – plasmas 1. Introduction called trielectronic recombination (TR) is possible in Be-like ions. -
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