Fundamentals of Plasma Physics

Total Page:16

File Type:pdf, Size:1020Kb

Fundamentals of Plasma Physics Prof. Dr. Wolfhard Möller Fundamentals of Plasma Physics Resume of a lecture held at the University of Technology Dresden Issue: Summer 2006 Prof. Dr. Wolfhard Möller Tel. 0351-260-2245 Forschungszentrum Rossendorf [email protected] 01314 Dresden Postfach 510119 http://www.fz-rossendorf.de/FWI Intention It is the purpose of these notes to present a short display of the physical issues and the main results presented in the lecture "Fundamentals of Plasma Physics". It is not meant to replace a textbook. For details, extended discussions and mathematical derivations, the reader is referred to the literature. Literature 1. F.F. Chen, Introduction to Plasma Physics (Plenum Press, New York 1974) 2. R.J. Goldston and P.H. Rutherford, Introduction to Plasma Physics (Institute of Physics Publ., Bristol 1995) 3. C.K. Birdsall and A.B. Langdon, Plasma Physics Via Computer Simulation (Institute of Physics Publ., Bristol 1991) 4. M.A. Lieberman and A.J. Lichtenberg, Principles of Plasma Discharges and Materials Processing (John Wiley & Sons Inc., New York 1994) 5. R. Hippler, S. Pfau, M. Schmidt and K.H. Schoenbach (Eds.), Low Temperature Plasma Physics (Wiley-VCH, Berlin 2001) 6. B.N. Chapman, Glow Discharge Processes – Sputtering and Plasma Etching (John Wiley & Sons, New York 1980) 7. D.E. Post and R. Behrisch (Eds.), Physics of Plasma Wall Interactions in Controlled Fusion (NATO ASI Series B, Vol. 131, Plenum Press, New York 1986) 8. S. Glasstone und R.H. Loveberg, Kontrollierte Thermonukleare Reaktionen (Verlag Karl Thiemig KG, München 1964) 9. K. Miramoto, Plasma Physics and Controlled Nuclear Fusion (Springer, Berlin 2005) 10. R.E.H. Clark and D.H. Reiter, Nuclear Fusion Research: Understanding Plasma-Surface Interactions (Springer, Berlin 2005) 2 Contents Literature....................................................................................................................... 2 1. Plasma definition and classification…………………………………………………….. 5 1.1 Definitions.............................................................................................. 6 1.2 Maxwellian temperature distribution...................................................... 6 1.3 Debye length.......................................................................................... 6 1.4 Plasma frequency................................................................................... 7 1.5 Classification of plasmas......................................................................... 8 2. Collisions in plasmas…………………………………………………............................. 10 2.1 General definitions.................................................................................. 10 2.2 Binary elastic collision kinematics.......................................................... 10 2.3 Differential cross section........................................................................ 12 2.4 Momentum transfer................................................................................ 13 2.5 Coulomb collisions................................................................................. 14 2.6 Collisions of neutrals.............................................................................. 16 2.7 Resonant charge transfer....................................................................... 17 2.8 Polarization scattering……………………………………………………… 19 2.9 Electron elastic scattering at neutrals…………………………………….. 20 2.10Electron impact ionization………………………………………………….. 20 2.11Electron impact dissociation……………………………………………….. 22 2.12Electron impact excitation………………………………………………….. 22 2.13Penning ionization………….……………………………………………….. 23 2.14Chemical reactions………………………………………………………….. 25 3. Motion of charged particles………………………………………….......................….... 25 3.1 Equation of motion.................................................................................. 25 3.2 Constant magnetic field………................................................................ 25 3.3 Constant electric and magnetic fields...................................................... 26 3.4 Inhomogeneous magnetic field................................................................ 27 3.5 Gravitation and magnetic field................................................................. 30 3.6 Drifts and instabilities............................................................................... 30 3.7 Time-dependent magnetic field………..................................................... 31 3.8 Time-dependent electric field................................................................... 33 3.9 Adiabatic invariants…...………................................................................. 33 4. Plasma as a fluid…………..………………………………………….......................…… 36 4.1 Distribution function and moments........................................................... 36 4.2 Particle, momentum and energy balance………………………………….. 37 4.3 Drifts in fluid description…………............................................................. 40 5. Transport……….…………..………………………………………….......................…... 42 5.1 Drift and diffusion…………………............................................................ 42 5.2 Transport of neutrals……………………...…………………………………. 44 5.3 Ambipolar diffusion………………............................................................. 47 5.4 Diffusion in a magnetic field……………...…………………………………. 48 5.5 Plasma resistivity ………………............................................................ 50 5.6 Electrical plasma heating…………………………………………………….. 51 6. Plasma Boundary ………..………………………………………….......................…... 54 6.1 Electrostatic sheath………………............................................................ 54 6.2 Presheath…………..……………………...…………………………………. 56 6.3 Potential, flux, ion energy………............................................................. 57 6.4 Negatively biased electrode..….………...…………………………………. 58 3 6.5 Collisional sheath ………………............................................................. 62 6.6 Electrostatic probe …………………………………………………………. 65 7. Plasma Surface Interaction………………………………………….............................. 67 7.1 Ion implantation and reemission............................................................. 67 7.2 Collision cascade....……………………...…………………………………. 73 7.3 Radiation damage.……..………............................................................. 74 7.4 Sputtering……………………….………...…………………………………. 74 7.5 Chemical sputtering..……………............................................................ 76 7.6 Surface reactions……………………………………………………………. 77 7.7 Secondary electron emission.…............................................................. 79 8. Particle Waves and Resonances..………………………………….......................…... 82 8.1 Electron oscillations…………….............................................................. 82 8.2 Electron waves…....……………………...…………………………………. 83 8.3 Ion waves………….……..………............................................................ 84 8.4 Electron oscillations in magnetic fields...………………………………….. 84 8.5 Ion waves in magnetic fields...…............................................................ 86 9. Electromagnetic Waves…………..………………………………….......................…... 88 9.1 Non-magnetized plasma……….............................................................. 88 9.2 Magnetized plasma.……………………...…………………………………. 91 10. Plasma Modelling………………..………………………………….......................….... 95 10.1 Global modelling ………...…….............................................................. 95 10.2 Reactive plasmas……………...………...…………………………………. 98 10.3 Fluid modelling... ………...…….............................................................. 100 10.4 Particle-in-cell computer simulation …...…………………………………. 101 11. Low-temperature DC Plasmas..…….…………………………….......................…..... 104 11.1 Breakdown..…… ………...…….............................................................. 104 11.2 Regimes of operation……………………………………………………..... 106 11.3 DC magnetron discharge...…...………...…………………………………. 108 12. Low-temperature RF Plasmas…………………………………………………………... 111 12.1 Capacitively coupled RF discharge........................................................ 111 12.2 Ion energy distribution……………………………………………………… 117 13. Magnetic Confinement Nuclear Fusion Plasma.…………………………………… 120 15.1 Fusion reactions……………………........................................................ 120 15.2 Ignition.…………..….……..………………………………………………… 121 15.3 Machine concepts…………………........................................................ 122 15.4 Transport.………..….……..………………………………………………… 126 4 1. Plasma Definition and Classification 1.1 Definitions A plasma, the so-called 4th physical condition of matter, is defined as a (partly) ionized gas, which is neutral in average ("quasineutral") and exhibits collective properties (the density has to be high enough). Thus, the plasma consists in most cases of neutral atoms or molecules, positive ions and electrons, which interact by collisions. The most efficient mechanism of ionisation is the collision between electrons and neutrals. For this purpose, a fraction of the electrons has to have kinetic energies which exceed the ionization potential, i.e. above a few eV, so that the electrons have to be rather "hot". In a stationary plasma, the rate of ionization has to be compensated by a loss of charged particles to the environment (wall – see Fig. 1.1), if recombination is neglected. This defines a mean residence time (or "confinement time") of the charged particles in the plasma. Fig. 1.1: A quasineutral plasma with
Recommended publications
  • 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.
    [Show full text]
  • 10. Collisions • Use Conservation of Momentum and Energy and The
    10. Collisions • Use conservation of momentum and energy and the center of mass to understand collisions between two objects. • During a collision, two or more objects exert a force on one another for a short time: -F(t) F(t) Before During After • It is not necessary for the objects to touch during a collision, e.g. an asteroid flied by the earth is considered a collision because its path is changed due to the gravitational attraction of the earth. One can still use conservation of momentum and energy to analyze the collision. Impulse: During a collision, the objects exert a force on one another. This force may be complicated and change with time. However, from Newton's 3rd Law, the two objects must exert an equal and opposite force on one another. F(t) t ti tf Dt From Newton'sr 2nd Law: dp r = F (t) dt r r dp = F (t)dt r r r r tf p f - pi = Dp = ò F (t)dt ti The change in the momentum is defined as the impulse of the collision. • Impulse is a vector quantity. Impulse-Linear Momentum Theorem: In a collision, the impulse on an object is equal to the change in momentum: r r J = Dp Conservation of Linear Momentum: In a system of two or more particles that are colliding, the forces that these objects exert on one another are internal forces. These internal forces cannot change the momentum of the system. Only an external force can change the momentum. The linear momentum of a closed isolated system is conserved during a collision of objects within the system.
    [Show full text]
  • 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.
    [Show full text]
  • 12. Elastic Collisions A) Overview B) Elastic Collisions V
    12. Elastic Collisions A) Overview In this unit, our focus will be on elastic collisions, namely those collisions in which the only forces that act during the collision are conservative forces. In these collisions, the sum of the kinetic energies of the objects is conserved. We will find that the description of these collisions is significantly simplified in the center of mass frame of the colliding objects. In particular, we will discover that, in this frame, the speed of each object after the collision is the same as its speed before the collision. B) Elastic Collisions In the last unit, we discussed the important topic of momentum conservation. In particular, we found that when the sum of the external forces acting on a system of particles is zero, then the total momentum of the system, defined as the vector sum of the individual momenta, will be conserved. We also determined that the kinetic energy of the system, defined to be the sum of the individual kinetic energies, is not necessarily conserved in collisions. Whether or not this energy is conserved is determined by the details of the forces that the components of the system exert on each other. In the last unit, our focus was on inelastic collisions, those collisions in which the kinetic energy of the system was not conserved. In particular non-conservative work was done by the forces that the individual objects exerted on each other during the collision. In this unit, we will look at examples in which the only forces that act during the collision are conservative forces.
    [Show full text]
  • Collisions in Classical Mechanics in Terms of Mass-Momentum “Vectors” with Galilean Transformations
    World Journal of Mechanics, 2020, 10, 154-165 https://www.scirp.org/journal/wjm ISSN Online: 2160-0503 ISSN Print: 2160-049X Collisions in Classical Mechanics in Terms of Mass-Momentum “Vectors” with Galilean Transformations Akihiro Ogura Laboratory of Physics, Nihon University, Matsudo, Japan How to cite this paper: Ogura, A. (2020) Abstract Collisions in Classical Mechanics in Terms of Mass-Momentum “Vectors” with Galilean We present the usefulness of mass-momentum “vectors” to analyze the colli- Transformations. World Journal of Mechan- sion problems in classical mechanics for both one and two dimensions with ics, 10, 154-165. Galilean transformations. The Galilean transformations connect the mass- https://doi.org/10.4236/wjm.2020.1010011 momentum “vectors” in the center-of-mass and the laboratory systems. We Received: August 28, 2020 show that just moving the two systems to and fro, we obtain the final states in Accepted: October 9, 2020 the laboratory systems. This gives a simple way of obtaining them, in contrast Published: October 12, 2020 with the usual way in which we have to solve the simultaneous equations. For Copyright © 2020 by author(s) and one dimensional collision, the coefficient of restitution is introduced in the Scientific Research Publishing Inc. center-of-mass system. This clearly shows the meaning of the coefficient of This work is licensed under the Creative restitution. For two dimensional collisions, we only discuss the elastic colli- Commons Attribution International sion case. We also discuss the case of which the target particle is at rest before License (CC BY 4.0). http://creativecommons.org/licenses/by/4.0/ the collision.
    [Show full text]
  • Definitions and Concepts for AQA Physics a Level
    Definitions and Concepts for AQA Physics A Level Topic 4: Mechanics and Materials Breaking Stress: The maximum stress that an object can withstand before failure ​ occurs. Brittle: A brittle object will show very little strain before reaching its breaking ​ stress. Centre of Mass: The single point through which all the mass of an object can be ​ said to act. Conservation of Energy: Energy cannot be created or destroyed - it can only be ​ transferred into different forms. Conservation of Momentum: The total momentum of a system before an event, ​ must be equal to the total momentum of the system after the event, assuming no external forces act. Couple: Two equal and opposite parallel forces that act on an object through ​ different lines of action. It has the effect of causing a rotation without translation. Density: The mass per unit volume of a material. ​ Efficiency: The ratio of useful output to total input for a given system. ​ Elastic Behaviour: If a material deforms with elastic behaviour, it will return to its ​ original shape when the deforming forces are removed. The object will not be permanently deformed. Elastic Collision: A collision in which the total kinetic energy of the system before ​ the collision is equal to the total kinetic energy of the system after the collision. Elastic Limit: The force beyond which an object will no longer deform elastically, ​ and instead deform plastically. Beyond the elastic limit, when the deforming forces are removed, the object will not return to its original shape. Elastic Strain Energy: The energy stored in an object when it is stretched.
    [Show full text]
  • How the Saha Ionization Equation Was Discovered
    How the Saha Ionization Equation Was Discovered Arnab Rai Choudhuri Department of Physics, Indian Institute of Science, Bangalore – 560012 Introduction Most youngsters aspiring for a career in physics research would be learning the basic research tools under the guidance of a supervisor at the age of 26. It was at this tender age of 26 that Meghnad Saha, who was working at Calcutta University far away from the world’s major centres of physics research and who never had a formal training from any research supervisor, formulated the celebrated Saha ionization equation and revolutionized astrophysics by applying it to solve some long-standing astrophysical problems. The Saha ionization equation is a standard topic in statistical mechanics and is covered in many well-known textbooks of thermodynamics and statistical mechanics [1–3]. Professional physicists are expected to be familiar with it and to know how it can be derived from the fundamental principles of statistical mechanics. But most professional physicists probably would not know the exact nature of Saha’s contributions in the field. Was he the first person who derived and arrived at this equation? It may come as a surprise to many to know that Saha did not derive the equation named after him! He was not even the first person to write down this equation! The equation now called the Saha ionization equation appeared in at least two papers (by J. Eggert [4] and by F.A. Lindemann [5]) published before the first paper by Saha on this subject. The story of how the theory of thermal ionization came into being is full of many dramatic twists and turns.
    [Show full text]
  • Bibliography of Low Energy Electron
    Bibliography of Low Energy Electron Collision Cross Section Data United States Department of Commerce National Bureau of Standards Miscellaneous Publication 289 — THE NATIONAL BUREAU OF STANDARDS The National Bureau of Standards 1 provides measurement and technical information services essential to the efficiency and effectiveness of the work of the Nation's scientists and engineers. The Bureau serves also as a focal point in the Federal Government for assuring maximum application of the physical and engineering sciences to the advancement of technology in industry and commerce. To accomplish this mission, the Bureau is organized into three institutes covering broad program areas of research and services: THE INSTITUTE FOR BASIC STANDARDS . provides the central basis within the United States for a complete and consistent system of physical measurements, coordinates that system with the measurement systems of other nations, and furnishes essential services leading to accurate and uniform physical measurements throughout the Nation's scientific community, industry, and commerce. This Institute comprises a series of divisions, each serving a classical subject matter area: —Applied Mathematics—Electricity—Metrology—Mechanics—Heat—Atomic Physics—Physical Chemistry—Radiation Physics—Laboratory Astrophysics 2—Radio Standards Laboratory, 2 which includes Radio Standards Physics and Radio Standards Engineering—Office of Standard Refer- ence Data. THE INSTITUTE FOR MATERIALS RESEARCH . conducts materials research and provides associated materials services including mainly reference materials and data on the properties of ma- terials. Beyond its direct interest to the Nation's scientists and engineers, this Institute yields services which are essential to the advancement of technology in industry and commerce. This Institute is or- ganized primarily by technical fields: —Analytical Chemistry—Metallurgy—Reactor Radiations—Polymers—Inorganic Materials—Cry- ogenics 2—Materials Evaluation Laboratory-— Office of Standard Reference Materials.
    [Show full text]
  • The Effects of Elastic Scattering in Neutral Atom Transport D
    The effects of elastic scattering in neutral atom transport D. N. Ruzic Citation: Phys. Fluids B 5, 3140 (1993); doi: 10.1063/1.860651 View online: http://dx.doi.org/10.1063/1.860651 View Table of Contents: http://pop.aip.org/resource/1/PFBPEI/v5/i9 Published by the American Institute of Physics. Related Articles Dissociation mechanisms of excited CH3X (X = Cl, Br, and I) formed via high-energy electron transfer using alkali metal targets J. Chem. Phys. 137, 184308 (2012) Efficient method for quantum calculations of molecule-molecule scattering properties in a magnetic field J. Chem. Phys. 137, 024103 (2012) Scattering resonances in slow NH3–He collisions J. Chem. Phys. 136, 074301 (2012) Accurate time dependent wave packet calculations for the N + OH reaction J. Chem. Phys. 135, 104307 (2011) The k-j-j′ vector correlation in inelastic and reactive scattering J. Chem. Phys. 135, 084305 (2011) Additional information on Phys. Fluids B Journal Homepage: http://pop.aip.org/ Journal Information: http://pop.aip.org/about/about_the_journal Top downloads: http://pop.aip.org/features/most_downloaded Information for Authors: http://pop.aip.org/authors Downloaded 23 Dec 2012 to 192.17.144.173. Redistribution subject to AIP license or copyright; see http://pop.aip.org/about/rights_and_permissions The effects of elastic scattering in neutral atom transport D. N. Ruzic University of Illinois, 103South Goodwin Avenue, Urbana Illinois 61801 (Received 14 December 1992; accepted21 May 1993) Neutral atom elastic collisions are one of the dominant interactions in the edge of a high recycling diverted plasma. Starting from the quantum interatomic potentials, the scattering functions are derived for H on H ‘, H on Hz, and He on Hz in the energy range of 0.
    [Show full text]
  • 1 Introduction
    i i Karl-Heinz Spatschek: High Temperature Plasmas — Chap. spatscheck0415c01 — 2011/9/1 — page 1 — le-tex i i 1 1 Introduction A plasma is a many body system consisting of a huge number of interacting (charged and neutral) particles. More precisely, one defines a plasma as a quasineu- tral gas of charged and neutral particles which exhibits collective behavior. In many cases, one considers quasineutral gases consisting of charged particles, namely electrons and positively charged ions of one species. Plasmas may contain neutral atoms. In this case, the plasma is called partially or incompletely ionized. Other- wise the plasma is said to be completely or fully ionized. The term plasma is not limited to the most common electron–ion case. One may have electron–positron plasmas, quark-gluon plasmas, and so on. Semiconductors contain plasma con- sisting of electrons and holes. Most of the matter in the universe occurs in the plasma state. It is often said that 99% of the matter in the universe is in the plasma state. However, this estimate may not be very accurate. Remember the discussion on dark matter. Nevertheless, the plasma state is certainly dominating the universe. Modern plasma physics emerged in 1950s, when the idea of thermonuclear re- actor was introduced. Fortunately, modern plasma physics completely dissociated from weapons development. The progression of modern plasma physics can be retraced from many monographs, for example, [1–15]. In simple terms, plasmas can be characterized by two parameters, namely, charged particle density n and temperature T. The density varies over roughly 28 6 34 3 orders of magnitude, for example, from 10 to 10 m .
    [Show full text]
  • Energy Considerations in Collisions How It Works
    L-8 (M-7) I. Collisions II. Work and Energy • Momentum: an object of mass m, moving with velocity v has a momentum p = m v. • Momentum is an important and useful concept that is used to analyze collisions – The colliding objects exert strong forces on each other over relatively short time intervals – Details of the forces are usually not known, but the forces acting on the objects are equal in magnitude and opposite in direction (3rd law) – The law of conservation of momentum which follows from Newton’s 2nd and 3rd laws, allows us to predict what happens in collisions 1 2 I. Physics of collisions: Law of Conservation of Momentum conservation of momentum • A consequence of Newton’s Newton’s Cradle 3rd law is that if we add the • The concept of momentum is very useful momentum of both objects when discussing how 2 objects interact. before a collision, it is the same as the momentum of • Suppose two objects are on a collision the two objects immediately course. AB after the collision. • We know their masses and speeds before • The law of conservation of momentum and the law of they collide conservation of energy are During the short time of • The momentum concept helps us to two of the fundamental laws of nature. the collision, the effect of predict what will happen after they collide. gravity is not important. 3 4 Momentum conservation in a two-body collision, Energy considerations in collisions How it works. v • Objects that are in motion have kinetic energy: v B, before A, before KE = ½ m v2 (Note that KE does not depend on before B collision A the direction of the object’s motion) more on this .
    [Show full text]
  • Lecture 8: Statistical Equilibria, Saha Equation
    Statistical Equilibria: Saha Equation We are now going to consider the statistics of equilibrium. Specifically, suppose we let a system stand still for an extremely long time, so that all processes can come into balance. We then measure the fraction of particles that are in each of several states (e.g., if we have a pure hydrogen gas, we might want to know the ionization fraction). How can we compute this fraction? We’ll take a look at this in several different ways. We will then step back and ask ourselves when these equilibrium formulae do not apply. This is important! To paraphrase Clint Eastwood, “An equation’s got to know its limitations”. In virtually all astronomical problems we deal with approximations, so we always need a sense of when those approximations fail. This serves a double purpose: it keeps us from making errors, but it also keeps us from applying too complex an approach to a simple problem. Let’s start out with a simple case. We consider a column of isothermal gas (temperature T ) in a constant gravitational acceleration g. Each molecule has mass m. If we can treat this like an ideal gas, Ask class: how do we figure out how the pressure vary with height h? An ideal gas has pressure P = nkT , where n is the number density. In equilibrium the pressure gradient balances the weight of the gas, so dP/dh = −ρg. Using ρ = nm = P m/kT and the constancy of T , we have dP/dh = −(mg/kT )P , so P = P0 exp(−mgh/kT ), where P0 is defined as the pressure at h = 0.
    [Show full text]