Modeling Plasma Via Electron Impact Ionization
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Study of Memory Effect in an Atmospheric Pressure Townsend
THÈSE En vue de l’obtention du DOCTORAT DE L’UNIVERSITÉ DE TOULOUSE Délivré par l'Université Toulouse 3 - Paul Sabatier Présentée et soutenue par Xi LIN Le 22 février 2019 Study of memory effect in an Atmospheric Pressure Townsend Discharge in the mixture N2/O2 using laser induced fluorescence Ecole doctorale : GEET - Génie Electrique Electronique et Télécommunications : du système au nanosystème Spécialité : Ingénierie des Plasmas Unité de recherche : LAPLACE - Laboratoire PLAsma et Conversion d'Énergie - CNRS-UPS-INPT Thèse dirigée par Simon DAP et Nicolas GHERARDI Jury Mme Svetlana Starikovskaia, Rapporteuse M. Ronny Brandenburg, Rapporteur Mme Françoise Massines, Examinateur M. Frédéric Marchal, Examinateur M. Philippe Teulet, Examinateur M. Simon DAP, Directeur de thèse Acknowledgement I would like to express my deepest thanks to my supervisor, Simon Dap. He has devoted so much time on teaching and leading me into the world of plasma physics. I am very appreciated for his patience and encouragement, also thanks to his support and rich discussion on physics, I finally achieve my thesis. I would also like to express my thanks to Nicolas Naudé for the fruitful discussions and suggestions on electrical characteristics of discharge, and for his knowledge on electrode fabrication and on OES spectroscopy. Thanks to Nicolas Gherardi for his confidence and support on me. Thanks to Prof. Svetlana M Starikovskaia and Prof. Ronny Brandenburg, for reviewing my thesis. I would also like to extend my gratitude to three other jury members, Prof. Françoise Massines, Prof. Feédéric Marchal and Prof. Philippe Teulet, for being the examiners of my work. I appreciate the assistance and advice from the technicians and engineers of Laplace, Benoît Schlegel, Fédéric Sidor, Vincent Bley, Céline Combettes, Cédric Trupin, and Stéphane Martin. -
Excitation Temperature, Degree of Ionization of Added Iron Species, and Electron Density in an Exploding Thin Film Plasma
SpectmchimiccrACIO. Vol. MB. No. II. Pp.10814096. 1981. 0584-8547/81/111081-16SIZ.CNI/O Printedin Great Britain. PerpmonPress Ltd. Excitation temperature, degree of ionization of added iron species, and electron density in an exploding thin film plasma S. Y. SUH* and R. D. SACKS Department of Chemistry, University of Michigan, Ann Arbor, Ml 48109, U.S.A. (Received 7 April 1981) Abstract-Time and spatially resolved spectra of a cylindrically symmetric exploding thin film plasma were obtained with a rotating mirror camera and astigmatic imaging. These spectra were deconvoluted to obtain relative spectral emissivity profiles for nine Fe(H) and two Fe(I) lines. The effective (electronic) excitation temperature at various positions in the plasma and at various times during the first current halfcycle was computed from the Fe(H) emissivity values using the Boltzmann graphical method. The Fe(II)/Fe(I) emissivity ratios together with the temperature were used to determine the degree of ionization of Fe. Finally, the electron density was estimated from the Saha equilibrium. Electronic excitation temperatures range from lO,OOO-15,OOOKnear the electrode surface at peak discharge current to 700&10.000K at 6-10 mm above the electrode surface at the first current zero. Corresponding electron densities range from 10’7-10u cm-’ at peak current to 10’~-10’6cm-3 near zero current. Error propagation and criteria for thermodynamic equilibrium are discussed. 1. IN-~R~DU~~ION THE HIGH-TEMPERATURE plasmas produced by the rapid electrical vaporization of Ag thin films recently have been used as atomization cells and excitation sources for the direct determination of selected elements in micro-size powder samples [ 11. -
Measurements and Studies of Secondary Electron Emission of Diamond Amplified Photocathode
BNL-81607-2008-IR C-A/APl#328 October 2008 Measurements and Studies of Secondary Electron Emission of Diamond Amplified Photocathode Qiong Wu Collider-Accelerator Department Brookhaven National Laboratory Upton, NY 11973 Notice: This document bas been authorized by employees of Brookhaven Science Associates, LLC under Contract No. DE-AC02-98CH10886 with the US.Department of Energy. Tbe United States Government retains a non- exclusive, paid-up, irrevocable, world-wide license to publish or reproduce the published form ofthis document, or allow others to do so, for United States Government purposes. MEASUREMENTSAND STUDIES OF SECONDARY ELECTRONEMISSION OF DIAMONDAMPLIFIED PHOTOCATHODE Qiong Wu September, 2008 CONTENTS 1 Introduction .......................................................................................................... 1 1.1 The Diamond Amplified Photocathode (DAF') hoject .................................... 1 1.2 Advantages of diamond for amplified photocathodes ...................................... 4 1.2.1 Wide Band Gq ..... ....................................... 5 1.2.2 Best Rigidiiy ..................... ............ 6 1.2.3 Highest Thermal Conducfivity ................................................................................................ 7 1.2.4 Very high Mobility and Sahrralion Velocity............ ....................... ....8 2 DAP Design ........................................................................................................ 10 2.1 vacuum .......................................................................................................... -
The Moedal Experiment at the LHC. Searching Beyond the Standard
126 EPJ Web of Conferences , 02024 (2016) DOI: 10.1051/epjconf/201612602024 ICNFP 2015 The MoEDAL experiment at the LHC Searching beyond the standard model James L. Pinfold (for the MoEDAL Collaboration)1,a 1 University of Alberta, Physics Department, Edmonton, Alberta T6G 0V1, Canada Abstract. MoEDAL is a pioneering experiment designed to search for highly ionizing avatars of new physics such as magnetic monopoles or massive (pseudo-)stable charged particles. Its groundbreaking physics program defines a number of scenarios that yield potentially revolutionary insights into such foundational questions as: are there extra dimensions or new symmetries; what is the mechanism for the generation of mass; does magnetic charge exist; what is the nature of dark matter; and, how did the big-bang develop. MoEDAL’s purpose is to meet such far-reaching challenges at the frontier of the field. The innovative MoEDAL detector employs unconventional methodologies tuned to the prospect of discovery physics. The largely passive MoEDAL detector, deployed at Point 8 on the LHC ring, has a dual nature. First, it acts like a giant camera, comprised of nuclear track detectors - analyzed offline by ultra fast scanning microscopes - sensitive only to new physics. Second, it is uniquely able to trap the particle messengers of physics beyond the Standard Model for further study. MoEDAL’s radiation environment is monitored by a state-of-the-art real-time TimePix pixel detector array. A new MoEDAL sub-detector to extend MoEDAL’s reach to millicharged, minimally ionizing, particles (MMIPs) is under study Finally we shall describe the next step for MoEDAL called Cosmic MoEDAL, where we define a very large high altitude array to take the search for highly ionizing avatars of new physics to higher masses that are available from the cosmos. -
Experiments and Simulations of an Atmospheric Pressure Lossy Dielectric Barrier Townsend Discharge
Journal of Physics D: Applied Physics PAPER Related content - Atmospheric pressure glow discharge Experiments and simulations of an atmospheric plasma A A Garamoon and D M El-zeer pressure lossy dielectric barrier Townsend - Diffuse barrier discharges discharge Z Navrátil, R Brandenburg, D Trunec et al. - Nonlinear phenomena in dielectric barrier discharges: pattern, striation and chaos To cite this article: S Im et al 2014 J. Phys. D: Appl. Phys. 47 085202 Jiting OUYANG, Ben LI, Feng HE et al. Recent citations View the article online for updates and enhancements. - Radial structures of atmospheric-pressure glow discharges with multiple current pulses in helium Zhanguo Bai et al This content was downloaded from IP address 128.12.245.233 on 22/09/2020 at 18:06 Journal of Physics D: Applied Physics J. Phys. D: Appl. Phys. 47 (2014) 085202 (10pp) doi:10.1088/0022-3727/47/8/085202 Experiments and simulations of an atmospheric pressure lossy dielectric barrier Townsend discharge S Im, M S Bak1, N Hwang2 and M A Cappelli Mechanical Engineering Department, Stanford University, Stanford, California 94305-3032, USA E-mail: [email protected] Received 25 September 2013, revised 7 January 2014 Accepted for publication 9 January 2014 Published 7 February 2014 Abstract A diffuse discharge is produced in atmospheric pressure air between porous alumina dielectric barriers using low-frequency (60 Hz) alternating current. To study its formation mechanism, both the discharge current and voltage are measured while varying the dielectric barrier porosity (0%, 48% or 85%) and composition (99% Al2O3 ,99% SiO2 or 75% Al2O3 + 16% SiO2 + 9% other oxides). -
Verification of Gyrokinetic Codes: Theoretical Background & Numerical Implementations
N.Tronko 1, T.Goerler 2 , A.Bottino 2 , B.D.Scott 2, E.Sonnendrücker 1 Verification of Gyrokinetic codes: Theoretical background & Numerical implementations NumKin 2016, IRMA, Strasbourg, France 1 NMPP, Max Planck Institute für Plasmaphysik 2 TOK, Max Planck Institute für Plasmaphysik VeriGyro Project Participants Enabling Research Project on Verification of Gyrokinetic codes • Germany! Max Planck Insitute for Plasma Physics (Garching and Greifswald) • Switzerland SPC-EPFL, Lausanne • Finland! Aalto Univeristy • Great Britain University of Warwick • France CEA Cadarache, Université Paris IV, Rennes, Toulouse, Lorraine, Bretagne IRMA, Maison de la Simulation (Saclay) • USA Saint Michel’s College, VT NumKin 2016 VeriGyro Project @ IPP Garching Interdisciplinary Project in IPP Max Planck (Garching) NMPP Division (Numerical Methods for Plasma Physics) • Development and implementation of new algorithms for fusion and astrophysical plasma modeling • Development of libraries (i.e. Selalib) • Verification of existing codes • Participants: N. Tronko, E. Sonnendrücker Enabling Research Project VeriGyro TOK (Tokamak Theory) • Development of major codes • Plasma modeling and comparison with experimental results (ASDEX Upgrade) • Participants: T. Görler, A. Bottino, B. D. Scott NumKin 2016 VeriGyro Project: Motivation • Verification of Global (Electromagnetic) Gyrokinetic codes: Why? • Most popular tools for magnetised plasmas simulations: • Significant Development since last 10 years • Electrostatic gyrokinetic implementations : well established ! [Dimits -
Abstract an Introduction to the Physics and Applications Of
Abstract An Introduction To The Physics And Applications Of Electron Sources Kevin L. Jensen Naval Research Laboratory Models of thermal, field, photo, and secondary emission, as well as space charge limited current flow, have existed since the 1920’s. With the realization that such sources were crucial to Radar and communications, research in harnessing their capabilities greatly accelerated, and now they are key components of cutting edge applications such as High Power Microwave generation and x-ray Free Electron Lasers. Although the processes behind the emission mechanisms (namely, heat, electric field, photoemission effect, and ejection of secondaries due to a high energy primary beam) appear distinct, they can all be understood collectively using simple models from quantum mechanics, condensed matter physics, and electrostatics. A description of the theoretical models and some history behind each mechanism, examples of the kinds of emitters that employ those mechanisms, and the challenges to utilizing the beams generated by various electron source candidates (particularly with respect to beam parameters such as current density, space charge, emittance, and brightness) will be covered. A full description of the canonical emission equations of thermal (Richardson), field (Fowler-Nordheim), photo (Fowler-DuBridge), and secondary (Young) equations is given – but even more interestingly, a demonstration of how the equations are fundamentally related is explored. Processes that affect emission, such as electrostatic shielding, coatings, space charge (Child-Langmuir), and complications due to material properties (metal versus semiconductor) shall be described. Biographical Summary Kevin L. Jensen is a theoretical physicist whose research concerns emission properties of electron sources, particularly cold cathodes and photocathodes, but also thermal and secondary sources, for vacuum nanoelectronics, space-based applications, high power microwave generation, and particle accelerators and Free Electron Lasers. -
Physical Mechanism of Superconductivity
Physical Mechanism of Superconductivity Part 1 – High Tc Superconductors Xue-Shu Zhao, Yu-Ru Ge, Xin Zhao, Hong Zhao ABSTRACT The physical mechanism of superconductivity is proposed on the basis of carrier-induced dynamic strain effect. By this new model, superconducting state consists of the dynamic bound state of superconducting electrons, which is formed by the high-energy nonbonding electrons through dynamic interaction with their surrounding lattice to trap themselves into the three - dimensional potential wells lying in energy at above the Fermi level of the material. The binding energy of superconducting electrons dominates the superconducting transition temperature in the corresponding material. Under an electric field, superconducting electrons move coherently with lattice distortion wave and periodically exchange their excitation energy with chain lattice, that is, the superconducting electrons transfer periodically between their dynamic bound state and conducting state, so the superconducting electrons cannot be scattered by the chain lattice, and supercurrent persists in time. Thus, the intrinsic feature of superconductivity is to generate an oscillating current under a dc voltage. The wave length of an oscillating current equals the coherence length of superconducting electrons. The coherence lengths in cuprates must have the value equal to an even number times the lattice constant. A superconducting material must simultaneously satisfy the following three criteria required by superconductivity. First, the superconducting materials must possess high – energy nonbonding electrons with the certain concentrations required by their coherence lengths. Second, there must exist three – dimensional potential wells lying in energy at above the Fermi level of the material. Finally, the band structure of a superconducting material should have a widely dispersive antibonding band, which crosses the Fermi level and runs over the height of the potential wells to ensure the normal state of the material being metallic. -
CHAPTER 12: the Atomic Nucleus
CHAPTER 12 The Atomic Nucleus ◼ 12.1 Discovery of the Neutron ◼ 12.2 Nuclear Properties ◼ 12.3 The Deuteron ◼ 12.4 Nuclear Forces ◼ 12.5 Nuclear Stability ◼ 12.6 Radioactive Decay ◼ 12.7 Alpha, Beta, and Gamma Decay ◼ 12.8 Radioactive Nuclides Structure of matter Dark matter and dark energy are the yin and yang of the cosmos. Dark matter produces an attractive force (gravity), while dark energy produces a repulsive force (antigravity). ... Astronomers know dark matter exists because visible matter doesn't have enough gravitational muster to hold galaxies together. Hierarchy of forces ◼ Sta Standard Model tries to unify the forces into one force Ernest Rutherford “Father of the Nucleus” Story so far: Unification Faraday Glashow,Weinberg,Salam Georgi,Glashow Green,Schwarz Witten 1831 1967 1974 1984 1995 Electricity } } } Electromagnetic force } } } Magnetism} } Electro-weak force } } } Weak nuclear force} } Grand unified force } } } 5 Different } Strong nuclear force} } D=10 String } M-theory ? } Theories } Gravitational force} +branes in D=11 Page 6 © Imperial College London Discovery of the Neutron 3) Nuclear magnetic moment: The magnetic moment of an electron is over 1000 times larger than that of a proton. The measured nuclear magnetic moments are on the same order of magnitude as the proton’s, so an electron is not a part of the nucleus. ◼ In 1930 the German physicists Bothe and Becker used a radioactive polonium source that emitted α particles. When these α particles bombarded beryllium, the radiation penetrated several centimeters of lead. The neutrons collide elastically with the protons of the paraffin thereby producing the5.7 MeV protons Discovery of the Neutron ◼ Photons are called gamma rays when they originate from the nucleus. -
1 the Derivation of Particle Monte Carlo Methods for Plasma Modeling
The derivation of Particle Monte Carlo methods for plasma modeling from transport equations. Savino Longo Dipartimento di Chimica dell'Università and CNR/IMIP, Via Orabona 4, 70126 Bari, Italy. e-mail: [email protected] Abstract: We analyze here in some detail, the derivation of the Particle and Monte Carlo methods of plasma simulation, such as Particle in Cell (PIC), Monte Carlo (MC) and Particle in Cell / Monte Carlo (PIC/MC) from formal manipulation of transport equations. Keywords: Charged Particle Transport, Boltzmann Equation, Monte Carlo Methods, Particle-in-Cell, Vlasov/Boltzmann equation 1 1.Introduction An accurate calculation of the velocity distribution of charged particles in non equilibrium plasmas is necessary in order to evaluate the rate at which collisional elementary processes take place in these media as well as their transport properties [1]. In doing so, one has to take into account the effect of inertia, scattering, externally applied and self-coherent fields, all affecting the particle transport. To this aim, different particle simulation techniques have been used extensively, as an alternative to the grid-based solution of transport equations [1] by finite differences or finite element techniques. To these belong the very well-know Test Particle Monte Carlo (TPMC, or simply Monte Carlo, MC [1]), the Particle in Cell (PIC [2,3]) and Particle in Cell / Monte Carlo methods (PIC/MC [4]). No explicit description of the methods will be given here because of their widespread application within the plasma modelling community, and we assume in the following that they are already known to the reader. -
Non-Collider Searches for Stable Massive Particles
Non-collider searches for stable massive particles S. Burdina, M. Fairbairnb, P. Mermodc,, D. Milsteadd, J. Pinfolde, T. Sloanf, W. Taylorg aDepartment of Physics, University of Liverpool, Liverpool L69 7ZE, UK bDepartment of Physics, King's College London, London WC2R 2LS, UK cParticle Physics department, University of Geneva, 1211 Geneva 4, Switzerland dDepartment of Physics, Stockholm University, 106 91 Stockholm, Sweden ePhysics Department, University of Alberta, Edmonton, Alberta, Canada T6G 0V1 fDepartment of Physics, Lancaster University, Lancaster LA1 4YB, UK gDepartment of Physics and Astronomy, York University, Toronto, ON, Canada M3J 1P3 Abstract The theoretical motivation for exotic stable massive particles (SMPs) and the results of SMP searches at non-collider facilities are reviewed. SMPs are defined such that they would be suffi- ciently long-lived so as to still exist in the cosmos either as Big Bang relics or secondary collision products, and sufficiently massive such that they are typically beyond the reach of any conceiv- able accelerator-based experiment. The discovery of SMPs would address a number of important questions in modern physics, such as the origin and composition of dark matter and the unifi- cation of the fundamental forces. This review outlines the scenarios predicting SMPs and the techniques used at non-collider experiments to look for SMPs in cosmic rays and bound in mat- ter. The limits so far obtained on the fluxes and matter densities of SMPs which possess various detection-relevant properties such as electric and magnetic charge are given. Contents 1 Introduction 4 2 Theory and cosmology of various kinds of SMPs 4 2.1 New particle states (elementary or composite) . -
Ionization Balance in EBIT and Tokamak Plasmas N
Ionization balance in EBIT and tokamak plasmas N. J. Peacock, R. Barnsley, M. G. O’Mullane, M. R. Tarbutt, D. Crosby et al. Citation: Rev. Sci. Instrum. 72, 1250 (2001); doi: 10.1063/1.1324755 View online: http://dx.doi.org/10.1063/1.1324755 View Table of Contents: http://rsi.aip.org/resource/1/RSINAK/v72/i1 Published by the American Institute of Physics. Related Articles Bragg x-ray survey spectrometer for ITER Rev. Sci. Instrum. 83, 10E126 (2012) Novel energy resolving x-ray pinhole camera on Alcator C-Mod Rev. Sci. Instrum. 83, 10E526 (2012) Measurement of electron temperature of imploded capsules at the National Ignition Facility Rev. Sci. Instrum. 83, 10E121 (2012) South pole bang-time diagnostic on the National Ignition Facility (invited) Rev. Sci. Instrum. 83, 10E119 (2012) Temperature diagnostics of ECR plasma by measurement of electron bremsstrahlung Rev. Sci. Instrum. 83, 073111 (2012) Additional information on Rev. Sci. Instrum. Journal Homepage: http://rsi.aip.org Journal Information: http://rsi.aip.org/about/about_the_journal Top downloads: http://rsi.aip.org/features/most_downloaded Information for Authors: http://rsi.aip.org/authors Downloaded 08 Aug 2012 to 194.81.223.66. Redistribution subject to AIP license or copyright; see http://rsi.aip.org/about/rights_and_permissions REVIEW OF SCIENTIFIC INSTRUMENTS VOLUME 72, NUMBER 1 JANUARY 2001 Ionization balance in EBIT and tokamak plasmas N. J. Peacock,a) R. Barnsley,b) and M. G. O’Mullane Euratom/UKAEA Fusion Association, Culham Science Centre, Abingdon, Oxon OX14 3DB, United Kingdom M. R. Tarbutt, D. Crosby, and J. D. Silver The Clarendon Laboratory, University of Oxford, Parks Road, Oxford OX1 3PU, United Kingdom J.