Inelastic Scattering
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Impulse and Momentum
Impulse and Momentum All particles with mass experience the effects of impulse and momentum. Momentum and inertia are similar concepts that describe an objects motion, however inertia describes an objects resistance to change in its velocity, and momentum refers to the magnitude and direction of it's motion. Momentum is an important parameter to consider in many situations such as braking in a car or playing a game of billiards. An object can experience both linear momentum and angular momentum. The nature of linear momentum will be explored in this module. This section will discuss momentum and impulse and the interconnection between them. We will explore how energy lost in an impact is accounted for and the relationship of momentum to collisions between two bodies. This section aims to provide a better understanding of the fundamental concept of momentum. Understanding Momentum Any body that is in motion has momentum. A force acting on a body will change its momentum. The momentum of a particle is defined as the product of the mass multiplied by the velocity of the motion. Let the variable represent momentum. ... Eq. (1) The Principle of Momentum Recall Newton's second law of motion. ... Eq. (2) This can be rewritten with accelleration as the derivate of velocity with respect to time. ... Eq. (3) If this is integrated from time to ... Eq. (4) Moving the initial momentum to the other side of the equation yields ... Eq. (5) Here, the integral in the equation is the impulse of the system; it is the force acting on the mass over a period of time to . -
Part B. Radiation Sources Radiation Safety
Part B. Radiation sources Radiation Safety 1. Interaction of electrons-e with the matter −31 me = 9.11×10 kg ; E = m ec2 = 0.511 MeV; qe = -e 2. Interaction of photons-γ with the matter mγ = 0 kg ; E γ = 0 eV; q γ = 0 3. Interaction of neutrons-n with the matter −27 mn = 1.68 × 10 kg ; En = 939.57 MeV; qn = 0 4. Interaction of protons-p with the matter −27 mp = 1.67 × 10 kg ; Ep = 938.27 MeV; qp = +e Note: for any nucleus A: mass number – nucleons number A = Z + N Z: atomic number – proton (charge) number N: neutron number 1 / 35 1. Interaction of electrons with the matter Radiation Safety The physical processes: 1. Ionization losses inelastic collisions with orbital electrons 2. Bremsstrahlung losses inelastic collisions with atomic nuclei 3. Rutherford scattering elastic collisions with atomic nuclei Positrons at nearly rest energy: annihilation emission of two 511 keV photons 2 / 35 1. Interaction of electrons with1.E+02 the matter Radiation Safety ) 1.E+03 -1 Graphite – Z = 6 .g 2 1.E+01 ) Lead – Z = 82 -1 .g 2 1.E+02 1.E+00 1.E+01 1.E-01 1.E+00 collision 1.E-02 radiative collision 1.E-01 stopping pow er (MeV.cm total radiative 1.E-03 stopping pow er (MeV.cm total 1.E-02 1.E-01 1.E+00 1.E+01 1.E+02 1.E+03 1.E-02 energy (MeV) 1.E-02 1.E-01 1.E+00 1.E+01 1.E+02 1.E+03 Electrons – stopping power 1.E+02 energy (MeV) S 1 dE ) === -1 Copper – Z = 29 ρρρ ρρρ dl .g 2 1.E+01 S 1 dE 1 dE === +++ ρρρ ρρρ dl coll ρρρ dl rad 1 dE 1.E+00 : mass stopping power (MeV.cm 2 g. -
AIAA 19Th Fluid Dynamics, Plasma Dynamics and Lasers Conference June 8-10, 1987/Honolulu, Hawaii
AIAA-87 -1407 Electron-Cyclotron-Resonance (ECR) Plasma Acceleration J. C. Sercel Jet Propulsion Laboratory California Institute of Technology Pasadena, California AIAA 19th Fluid Dynamics, Plasma Dynamics and Lasers Conference June 8-10, 1987/Honolulu, Hawaii For permission to copy or republish, contact the American Institute of Aeronautics and Astronautics 1633 Broadway, New York, NY 10019 AIAA-87-1407 ELECTRON-CYCLOTRON-RESONANCE (ECR) PLASMA ACCELERATION Joel C. Sercel* Jet Propulsion Laboratory California Institute of Technology Pasadena, California Abstract P power per unit volume, W/m3 R position vector, m A research effort directed at analytically v velocity, mls and experimentally investigating Electron U energy, J or eV Cyclotron-Resonance (ECR) plasma acceleration V electrostatic potential, volts is outlined. Relevant past research is reviewed. T temperature, Kelvin or eV The prospects for application of ECR plasma acceleration to spacecraft propulsion are described. It is shown that previously unexplained losses in converting microwave magnetic dipole moment power to directed kinetic power via ECR plasma reaction cross section, m2 acceleration can be understood in terms of diffusion of energized plasma to the physical time constant, s walls of the accelerator. It is argued that line radiation losses from electron-ion and electron SubscriPts atom inelastic collisions should be less than estimated in past research. Based on this new A acceleration understanding, the expectation now exists that B Bohm efficient ECR plasma accelerators can be e electron designed for application to high specific impulse ex excitation spacecraft propulsion. ionization summation variable refers to lowest energy level Acronyms and Abbreviations p perpendicular r relative D-He3 Deuterium Helium-Three sp space charge induced ECR Electron-Cyclotron-Resonance to t total GE General Electric JPL Jet Propulsion Laboratory LeRC Lewis Research Center I. -
The Basic Interactions Between Photons and Charged Particles With
Outline Chapter 6 The Basic Interactions between • Photon interactions Photons and Charged Particles – Photoelectric effect – Compton scattering with Matter – Pair productions Radiation Dosimetry I – Coherent scattering • Charged particle interactions – Stopping power and range Text: H.E Johns and J.R. Cunningham, The – Bremsstrahlung interaction th physics of radiology, 4 ed. – Bragg peak http://www.utoledo.edu/med/depts/radther Photon interactions Photoelectric effect • Collision between a photon and an • With energy deposition atom results in ejection of a bound – Photoelectric effect electron – Compton scattering • The photon disappears and is replaced by an electron ejected from the atom • No energy deposition in classical Thomson treatment with kinetic energy KE = hν − Eb – Pair production (above the threshold of 1.02 MeV) • Highest probability if the photon – Photo-nuclear interactions for higher energies energy is just above the binding energy (above 10 MeV) of the electron (absorption edge) • Additional energy may be deposited • Without energy deposition locally by Auger electrons and/or – Coherent scattering Photoelectric mass attenuation coefficients fluorescence photons of lead and soft tissue as a function of photon energy. K and L-absorption edges are shown for lead Thomson scattering Photoelectric effect (classical treatment) • Electron tends to be ejected • Elastic scattering of photon (EM wave) on free electron o at 90 for low energy • Electron is accelerated by EM wave and radiates a wave photons, and approaching • No -
Particles and Deep Inelastic Scattering
Heidi Schellman Northwestern Particles and Deep Inelastic Scattering Heidi Schellman Northwestern University HUGS - JLab - June 2010 June 2010 HUGS 1 Heidi Schellman Northwestern k’ k q P P’ A generic scatter of a lepton off of some target. kµ and k0µ are the 4-momenta of the lepton and P µ and P 0µ indicate the target and the final state of the target, which may consist of many particles. qµ = kµ − k0µ is the 4-momentum transfer to the target. June 2010 HUGS 2 Heidi Schellman Northwestern Lorentz invariants k’ k q P P’ 2 2 02 2 2 2 02 2 2 2 The 5 invariant masses k = m` , k = m`0, P = M , P ≡ W , q ≡ −Q are invariants. In addition you can define 3 Mandelstam variables: s = (k + P )2, t = (k − k0)2 and u = (P − k0)2. 2 2 2 2 s + t + u = m` + M + m`0 + W . There are also handy variables ν = (p · q)=M , x = Q2=2Mµ and y = (p · q)=(p · k). June 2010 HUGS 3 Heidi Schellman Northwestern In the lab frame k’ k θ q M P’ The beam k is going in the z direction. Confine the scatter to the x − z plane. µ k = (Ek; 0; 0; k) P µ = (M; 0; 0; 0) 0µ 0 0 0 k = (Ek; k sin θ; 0; k cos θ) qµ = kµ − k0µ June 2010 HUGS 4 Heidi Schellman Northwestern In the lab frame k’ k θ q M P’ 2 2 2 s = ECM = 2EkM + M − m ! 2EkM 2 0 0 2 02 0 t = −Q = −2EkEk + 2kk cos θ + mk + mk ! −2kk (1 − cos θ) 0 ν = (p · q)=M = Ek − Ek energy transfer to target 0 y = (p · q)=(p · k) = (Ek − Ek)=Ek the inelasticity P 02 = W 2 = 2Mν + M 2 − Q2 invariant mass of P 0µ June 2010 HUGS 5 Heidi Schellman Northwestern In the CM frame k’ k q P P’ The beam k is going in the z direction. -
Analysis of Thruster Requirements and Capabilities for Local Satellite Clusters
I I ANALYSIS OF THRUSTER REQUIREMENTS AND CAPABILITIES FOR LOCAL SATELLITE CLUSTERS G. I. Yashkot, D.E. Hastingstt I Massachusetts Institute of Technology Cambridge, Massachusetts I Abstract This paper examines the propulsive requirements necessary to maintain the relative positions of satellites orbiting in a local cluster. Formation of these large baseline arrays could allow high resolution imaging of terrestrial or I astronomical targets using techniques similar to those used for decades in radio interferometry. A key factor in the image quality is the relative positions of the individual apertures in the sparse array. The relative positions of satellites in a cluster are altered by "tidal" accelerations which are a function of the cluster baseline and orbit altitude. These accelerations must be counteracted by continuous thrusting to maintain the relative positions of the satellites. I Analysis of propulsive system requirements, limited by spacecraft power, volume, and mass constraints, indicates that specific impulses and efficiencies typical of ion engines or Hall thrusters (SPT's) are necessary to maintain large cluster baselines. In addition, required thrust to spacecraft mass ratios for reasonable size clusters are approximately I 15J..LNlkg. Finally, the ability of a proposed linear ion microthruster to meet these requirements is examined. A variation of Brophy's method is used to show that primary electron containment lengths on the order of 10 mm are I necessary to achieve those thruster characteristics. Preliminary sizing -
Chemical Applications of Inelastic X-Ray Scattering
BNL- 68406 CHEMICAL APPLICATIONS OF INELASTIC X-RAY SCATTERING H. Hayashi and Y. Udagawa Research Institute for Scientific Measurements Tohoku University Sendai, 980-8577, Japan J.-M. Gillet Structures, Proprietes et Modelisation des Solides UMR8580 Ecole Centrale Paris, Grande Voie des Vignes, 92295 Chatenay-Malabry Cedex, France W.A. Caliebe and C.-C. Kao National Synchrotron Light Source Brookhaven National Laboratory Upton, New York, 11973-5000, USA August 2001 National Synchrotron Light Source Brookhaven National Laboratory Operated by Brookhaven Science Associates Upton, NY 11973 Under Contract with the United States Department of Energy Contract Number DE-AC02-98CH10886 DISCLAIMER This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, nor any of their contractors, subcontractors or their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy; completeness, or any third party’s use or the results of such use of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof or its contractors or subcontractors. Th.e views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof. CHEMICAL APPLICATIONS OF INELASTIC X-RAY SCATTERING H. -
Relative Merits and Limiting Factors for X-Ray and Electron Microscopy of Thick, Hydrated Organic Materials (2020 Revised Version)
Relative merits and limiting factors for x-ray and electron microscopy of thick, hydrated organic materials (2020 revised version) Ming Du1, and Chris Jacobsen2;3;4;∗ 1Department of Materials Science and Engineering, Northwestern University, 2145 Sheridan Road, Evanston IL 60208, USA 2Advanced Photon Source, Argonne National Laboratory, 9700 South Cass Avenue, Argonne IL 60439, USA 3Department of Physics & Astronomy, Northwestern University, 2145 Sheridan Road, Evanston IL 60208, USA 4Chemistry of Life Processes Institute, Northwestern University, 2170 Campus Drive, Evanston IL 60208, USA ∗Corresponding author; Email: [email protected] Abstract Electron and x-ray microscopes allow one to image the entire, unlabeled structure of hydrated mate- rials at a resolution well beyond what visible light microscopes can achieve. However, both approaches involve ionizing radiation, so that radiation damage must be considered as one of the limits to imaging. Drawing upon earlier work, we describe here a unified approach to estimating the image contrast (and thus the required exposure and corresponding radiation dose) in both x-ray and electron microscopy. This approach accounts for factors such as plural and inelastic scattering, and (in electron microscopy) the use of energy filters to obtain so-called \zero loss" images. As expected, it shows that electron microscopy offers lower dose for specimens thinner than about 1 µm (such as for studies of macromolecules, viruses, bacteria and archaebacteria, and thin sectioned material), while x-ray microscopy offers superior charac- teristics for imaging thicker specimen such as whole eukaryotic cells, thick-sectioned tissues, and organs. The required radiation dose scales strongly as a function of the desired spatial resolution, allowing one to understand the limits of live and frozen hydrated specimen imaging. -
Phenomenological Review on Quark–Gluon Plasma: Concepts Vs
Review Phenomenological Review on Quark–Gluon Plasma: Concepts vs. Observations Roman Pasechnik 1,* and Michal Šumbera 2 1 Department of Astronomy and Theoretical Physics, Lund University, SE-223 62 Lund, Sweden 2 Nuclear Physics Institute ASCR 250 68 Rez/Prague,ˇ Czech Republic; [email protected] * Correspondence: [email protected] Abstract: In this review, we present an up-to-date phenomenological summary of research developments in the physics of the Quark–Gluon Plasma (QGP). A short historical perspective and theoretical motivation for this rapidly developing field of contemporary particle physics is provided. In addition, we introduce and discuss the role of the quantum chromodynamics (QCD) ground state, non-perturbative and lattice QCD results on the QGP properties, as well as the transport models used to make a connection between theory and experiment. The experimental part presents the selected results on bulk observables, hard and penetrating probes obtained in the ultra-relativistic heavy-ion experiments carried out at the Brookhaven National Laboratory Relativistic Heavy Ion Collider (BNL RHIC) and CERN Super Proton Synchrotron (SPS) and Large Hadron Collider (LHC) accelerators. We also give a brief overview of new developments related to the ongoing searches of the QCD critical point and to the collectivity in small (p + p and p + A) systems. Keywords: extreme states of matter; heavy ion collisions; QCD critical point; quark–gluon plasma; saturation phenomena; QCD vacuum PACS: 25.75.-q, 12.38.Mh, 25.75.Nq, 21.65.Qr 1. Introduction Quark–gluon plasma (QGP) is a new state of nuclear matter existing at extremely high temperatures and densities when composite states called hadrons (protons, neutrons, pions, etc.) lose their identity and dissolve into a soup of their constituents—quarks and gluons. -
Digitalcommons@University of Nebraska - Lincoln
University of Nebraska - Lincoln DigitalCommons@University of Nebraska - Lincoln Instructional Materials in Physics and Calculus-Based General Physics Astronomy 1975 COLLISIONS Follow this and additional works at: https://digitalcommons.unl.edu/calculusbasedphysics Part of the Other Physics Commons "COLLISIONS" (1975). Calculus-Based General Physics. 6. https://digitalcommons.unl.edu/calculusbasedphysics/6 This Article is brought to you for free and open access by the Instructional Materials in Physics and Astronomy at DigitalCommons@University of Nebraska - Lincoln. It has been accepted for inclusion in Calculus-Based General Physics by an authorized administrator of DigitalCommons@University of Nebraska - Lincoln. Module -- STUDY GUIDE COLLISIONS INTRODUCTION If you have ever watched or played pool, football, baseball, soccer, hockey, or been involved in an automobile accident you have some idea about the results of a collision. We are interested in studying collisions for a variety of reasons. For example, you can determine the speed of a bullet by making use of the physics of the collision process. You can also estimate the speed of an automobile before the accident by knowing the physics of the collision process and a few other physical principles. Physicists use collisions to determine the properties of atomic and subatomic particles. Essentially, a particle accelerator is a device that provides a controlled collision process between subatomic particles so that, among other things, some of the properties of the target particle can be studied. In addition the study of collisions is an example of the use of a fundamental physical tool, i.e., a conservation law. A conservation law implies that something remains the same, i.e., is conserved, as you have seen in a previous module, Conservation of Energy. -
Basic Elements of Neutron Inelastic Scattering
2012 NCNR Summer School on Fundamentals of Neutron Scattering Basic Elements of Neutron Inelastic Scattering Peter M. Gehring National Institute of Standards and Technology NIST Center for Neutron Research Gaithersburg, MD USA Φs hω Outline 1. Introduction - Motivation - Types of Scattering 2. The Neutron - Production and Moderation - Wave/Particle Duality 3. Basic Elements of Neutron Scattering - The Scattering Length, b - Scattering Cross Sections - Pair Correlation Functions - Coherent and Incoherent Scattering - Neutron Scattering Methods (( )) (( )) (( )) (( )) 4. Summary of Scattering Cross Sections ω0 ≠ 0 (( )) (( )) (( )) (( )) - Elastic (Bragg versus Diffuse) (( )) (( )) (( )) (( )) - Quasielastic (Diffusion) - Inelastic (Phonons) ω (( )) (( )) (( )) (( )) Motivation Structure and Dynamics The most important property of any material is its underlying atomic / molecular structure (structure dictates function). Bi2Sr2CaCu2O8+δ In addition the motions of the constituent atoms (dynamics) are extremely important because they provide information about the interatomic potentials. An ideal method of characterization would be one that can provide detailed information about both structure and dynamics. Types of Scattering How do we “see”? Thus scattering We see something when light scatters from it. conveys information! Light is composed of electromagnetic waves. λ ~ 4000 A – 7000 A However, the details of what we see are ultimately limited by the wavelength. Types of Scattering The tracks of a compact disk act as a diffraction grating, producing a separation of the colors of white light. From this one can determine the nominal distance between tracks on a CD, which is 1.6 x 10-6 meters = 16,000 Angstroms. To characterize materials we must determine the underlying structure. We do this by using d the material as a diffraction grating. -
The Franck-Hertz Experiment
Experiment A1 THE FRANCK-HERTZ EXPERIMENT References Weidner and Sells, Elementary Physics, p. 256. Harnwell and Livengood, Experimental Atomic Physics, pp. 314-323. Eisberg, Fundamentals of Modern Physics, pp. 124-128 The Taylor Manual, pp. 410-415. Object: To observe energy level quantization in mercury atoms. The method uses a measurement of the energy loss in inelastic collisions between electrons and atomic mercury in a gaseous state through which they pass. This classic experiment was important when the quantum theory was still under challenge. It showed that the same energy level difference observed when the atom lost energy through photon emission can account for the energy lost by electrons in the beam when the atom absorbed energy. Background: The first excited state of a mercury atom is about 5 volts above the ground state. When an electron collides with one of these atoms, but has less than 5 eV of kinetic energy, the only option available is an elastic collision. Because there is an enormous difference between the rest mass of the electron and the rest mass of the mercury atom, very little kinetic energy will be transferred from the electron to the mercury atom. Once the electron has a kinetic energy greater than 5 eV, it is possible for the electron to undergo an inelastic collision. In this case the electron will loose the energy of excitation plus the same small energy transferred as in the elastic collisions. In both the elastic and inelastic collisions momentum must be conserved as well as energy. This explains the small kinetic energy of the mercury atom after the collision in both cases.