Part B. Radiation Sources Radiation Safety

Total Page:16

File Type:pdf, Size:1020Kb

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. −−−1 ) ρρρ dl collision dE −−−1 1.E-01 : linear stopping power (MeV.cm ) radiative dl total stopping pow er (MeV.cm 1.E-02 1.E-02 1.E-01 1.E+00 1.E+01 1.E+02 1.E+03 3 / 35 energy (MeV) 1. Interaction of electrons with the matter Radiation Safety Continuous Slowing Down 1.E+03 Approximation range: 1.E+02 0 1 1.E+01 rCSDA === dE .g) -2 S E0 tot 1.E+00 graphite 1.E+00 copper 1.E-01 lead 1.E-01 1.E-02 CSDA range(cm graphite 1.E-03 1.E-02 copper 1.E-04 lead 1.E-02 1.E-01 1.E+00 1.E+01 1.E+02 1.E+03 radiation yield energy (MeV) 1.E-03 Radiation yield: 1.E-04 1.E-02 1.E-01 1.E+00 1.E+01 1.E+02 1.E+03 Fraction of the initial kinetic energy that energy (MeV) is converted to Bremsstrahlung energy as the electron slows down to rest. 4 / 35 1. Interaction of electrons with the matter Radiation Safety mbarn Differential Bremsstrahlung cross section: 12 10 MeV 1 dσ 100 MeV 10 2 k × 1 GeV Z dk 10 GeV 8 mbarn 6 25 10 MeV 100 MeV 4 20 1 GeV 10 GeV 2 15 lead – Z = 82 0 0 0.2 0.4 0.6 0.8 1 10 k/T k: photon energy T: electron kinetic energy 5 T = m γ c2 - m c 2 = m c 2 / {1 - v2/c 2}1/2 - m c 2 carbon – Z = 6 0 0 0.2 0.4 0.6 0.8 1 k/T 5 / 35 1. Interaction of electrons with the matter Radiation Safety Multiple scattering mean scattering angle 1.E+02 ) 2 -1 graphite .g 2 2 Es X 1.E+01 θθθ === copper .cm βββp X0 2 lead 1.E+00 mass scattering power S sc 1.E-01 1.E-02 2 1 d θθθ S === sc ρρρ dx 1.E-03 1.E-04 mass scattering power (radian Es = 21.2 MeV 1.E-05 1.E+00 1.E+01 1.E+02 1.E+03 X0: radiation length β: v/c energy (MeV) p: momentum 6 / 35 2. Interaction of electrons with the matter Radiation Safety • Particles involved: – Electrons / Positrons – Photons – Neutrons X0 X0: radiation length 7 / 35 2. Interaction of electrons with the matter Radiation Safety 4 Electromagnetic cascade 3 2 1 photon electron 0 cm positron -1 -2 -3 -4 -5 0 5cm 10 15 one 500 MeV electron interacting with lead target 8 / 35 2. Interaction of photons with the matter Radiation10 Safety Electromagnetic cascade 8 6 4 2 photon 0 electron cm -2 positron -4 -6 -8 -10 0 5 10 15 20 cm one 6 GeV electron interacting with lead target 9 / 35 2. Interaction of photons with the matter Radiation Safety The physical processes: 1. Photo-electric effect removal of an orbital electron of the inner shells (K,L,M) 2. Compton scattering inelastic scattering on loosely bound electrons 3. Pair production production of e -/e + pair essentially with nuclei 4. Rayleigh (coherent) scattering elastic scattering not important for radiation physics 10 / 35 2. Interaction of photons with the matter Radiation Safety 1.E+04 Photon cross sections Graphite - Z = 6 1.E+03 ) -1 coherent .g 1.E+02 2 com pton photoelectric 1.E+01 pair production 1.E+00 total 1.E-01 cross section (cm 1.E-02 1.E-03 1.E-03 1.E-02 1.E-01 1.E+00 1.E+01 1.E+02 1.E+03 1.E+04 1.E+05 energy (MeV) 11 / 35 2. Interaction of photons with the matter Radiation Safety 1.E+04 Photon cross sections Lead - Z = 82 1.E+03 ) -1 coherent .g 1.E+02 2 com pton photoelectric 1.E+01 pair production 1.E+00 total 1.E-01 cross section (cm 1.E-02 1.E-03 1.E-03 1.E-02 1.E-01 1.E+00 1.E+01 1.E+02 1.E+03 1.E+04 1.E+05 energy (MeV) 12 / 35 2. Interaction of photons with the matter 1.E+04 1.E+03 Radiation Safety ) -1 coherent .g 1.E+02 2 com pton photoelectric 1.E+01 pair production Photo-electric effect: 1.E+00 total 1.E-01 photo-electron cross section (cm 1.E-02 ΔE = E 0 –E1 = K a 1.E-03 ΔE = E – E 1.E-03 1.E-02 1.E-01 1.E+00 1.E+01 1.E+02 1.E+03 1.E+04 1.E+05 0 energy (MeV) ΔE = E 0 –E2 = K b E2 E E E0 1 0 E KLMN KLMN incoming X-ray The K lines Auger electron ΔE = E 1 –E2 = L a E1 Auger-electron E1 ΔE = E 1 –E2 –E3 E2 E2 ΔE = E –E 1 3 KLMN KLMN = L b E3 E3 The L lines 13 / 35 2. Interaction of photons with the matter 1.E+04 1.E+03 Radiation Safety ) -1 coherent .g 1.E+02 2 com pton photoelectric Compton scattering: 1.E+01 scattered photon pair production 1.E+00 total energy E c 1.E-01 θ cross section (cm E0 1.E-02 Ec === 1.E-03 E0 1.E-03 1.E-02 1.E-01 1.E+00 1.E+01 1.E+02 1.E+03 1.E+04 1.E+05 primary photon Compton electron 1 +++ ((()(1 −−− cos θθθ))) energy (MeV) m c 2 energy = E -E 0 energy E 0 0 c 2 2 dσ/dW (r e x cm / electron) E (MeV) 1.E+02 c 1.E+00 50 keV 100 keV 500 keV 1.E+01 1 MeV 1.E-01 10 MeV 50 keV 100 MeV 100 keV 500 keV 1.E+00 1 MeV 1.E-02 10 MeV 100 MeV 1.E-01 1.E-03 0 30 60 90 120 150 180 θθθ (degrees) 1.E-02 0 30 60 90 120 150 180 θθθ (degrees) 14 / 35 2. Interaction of photons with the matter 1.E+04 Radiation Safety 1.E+03 ) -1 coherent .g 1.E+02 2 com pton photoelectric 1.E+01 Pair production: pair production 1.E+00 total 1.E-01 cross section (cm 1.E-02 1.E-03 1.E-03 1.E-02 1.E-01 1.E+00 1.E+01 1.E+02 1.E+03 1.E+04 1.E+05 2 energy (MeV) σnucleus ∝ Z threshold: 1.022 MeV 1 σ ∝ Z 0.9 electron 0.8 threshold: 2.044 MeV 0.7 0.6 0.5 0.4 0.3 relative probability 0.2 0.1 0 0 0.2 0.4 0.6 0.8 1 E/k 15 / 35 2. Interaction of photons with the matter Radiation Safety Interaction of photons with matter Macroscopic description - Attenuation factors The mass attenuation coefficient μ/ρ: 1 −µ d (cm ) 0 .9 N = N 0 × e µ 1 dN 0 .8 µµ N µ === − d ( g⋅cm −2 ) ρρρ ρρρN dl 0 .7 ρ 0 .6 N = N 0 × e units: cm 2.g -1 0 .5 The linear attenuation coefficient μ: 0 .4 1 dN 0 .3 µµµ === 0 .2 N dl 0 .1 0 units: cm -1 0 1 2 3 4 5 6 7 8 9 1 0 d (cm) d (g.cm -2) The conversion factor from σ (barns.atom -1) to μ/r (cm 2.g -1): µµµ N === 10 −−−24 A σσσ ρρρ A 16 / 35 2.
Recommended publications
  • 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
    [Show full text]
  • 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.
    [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]
  • 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.
    [Show full text]
  • Elastic Scattering, Fusion, and Breakup of Light Exotic Nuclei
    Eur. Phys. J. A (2016) 52: 123 THE EUROPEAN DOI 10.1140/epja/i2016-16123-1 PHYSICAL JOURNAL A Review Elastic scattering, fusion, and breakup of light exotic nuclei J.J. Kolata1,a, V. Guimar˜aes2, and E.F. Aguilera3 1 Physics Department, University of Notre Dame, Notre Dame, IN, 46556-5670, USA 2 Instituto de F`ısica,Universidade de S˜aoPaulo, Rua do Mat˜ao,1371, 05508-090, S˜aoPaulo, SP, Brazil 3 Departamento de Aceleradores, Instituto Nacional de Investigaciones Nucleares, Apartado Postal 18-1027, C´odigoPostal 11801, M´exico, Distrito Federal, Mexico Received: 18 February 2016 Published online: 10 May 2016 c The Author(s) 2016. This article is published with open access at Springerlink.com Communicated by N. Alamanos Abstract. The present status of fusion reactions involving light (A<20) radioactive projectiles at energies around the Coulomb barrier (E<10 MeV per nucleon) is reviewed, emphasizing measurements made within the last decade. Data on elastic scattering (providing total reaction cross section information) and breakup channels for the involved systems, demonstrating the relationship between these and the fusion channel, are also reviewed. Similarities and differences in the behavior of fusion and total reaction cross section data concerning halo nuclei, weakly-bound but less exotic projectiles, and strongly-bound systems are discussed. One difference in the behavior of fusion excitation functions near the Coulomb barrier seems to emerge between neutron-halo and proton-halo systems. The role of charge has been investigated by comparing the fusion excitation functions, properly scaled, for different neutron- and proton-rich systems. Possible physical explanations for the observed differences are also reviewed.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • Status of Electron Transport Cross Sections
    A11102 mob2fl NBS PUBLICATIONS AlllOb MOflOAb NBSIR 82-2572 Status of Electron Transport Cross Sections U.S. DEPARTMENT OF COMMERCE National Bureau of Standards Washington, DC 20234 September 1 982 Prepared for: Office of Naval Research Arlington, Virginia 22217 Space Science Data Center NASA Goddard Space Flight Center Greenbelt, Maryland 20771 Office of Health and Environmental Research Department of Energy jyj Washington, DC 20545 c.2 '»AT10*AL. BURKAU OF »TAMTARJ»a LIBRARY SEP 2 0 1982 NBSIR 82-2572 STATUS OF ELECTRON TRANSPORT CROSS SECTIONS S. M. Seltzer and M. J. Berger U S. DEPARTMENT OF COMMERCE National Bureau of Standards Washington, DC 20234 September 1 982 Prepared for: Office of Naval Research Arlington, Virginia 22217 Space Science Data Center NASA Goddard Space Flight Center Greenbelt, Maryland 20771 Office of Health and Environmental Research Department of Energy Washington, DC 20545 (A Q * U.S. DEPARTMENT OF COMMERCE, Malcolm Baldrige, Secretary NATIONAL BUREAU OF STANDARDS, Ernest Ambler, Director u r ju ' ^ l. .• .. w > - H *+ Status of Electron Transport Cross Sections Stephen M. Seltzer and Martin J. Berger National Bureau of Standards Washington, D.C. 20234 This report describes recent developments and improvements pertaining to cross sections for electron-photon transport calculations. The topics discussed include: (1) electron stopping power (mean excitation energies, density-effect correction); (2) bremsstrahlung production by electrons (radiative stopping power, spectrum of emitted photons); (3) elastic scattering of electrons by atoms; (4) electron-impact ionization of atoms. Key words: bremsstrahlung; cross sections; elastic scattering; electron- impact ionization; electrons; photons; stopping power; transport. Summary of a paper presented at the Annual Meeting of the American Nuclear Society, June 7-11, 1982, Los Angeles, California.
    [Show full text]
  • Part Fourteen Kinematics of Elastic Neutron Scattering
    22.05 Reactor Physics - Part Fourteen Kinematics of Elastic Neutron Scattering 1. Multi-Group Theory: The next method that we will study for reactor analysis and design is multi-group theory. This approach entails dividing the range of possible neutron energies into small regions, ΔEi and then defining a group cross-section that is averaged over each energy group i. Neutrons enter each group as the result of either fission (recall the distribution function for fission neutrons) or scattering. Accordingly, we need a thorough understanding of the scattering process before proceeding. 2. Types of Scattering: Fission neutrons are born at high energies (>1 MeV). However, the fission reaction is best sustained by neutrons that are at thermal energies with “thermal” defined as 0.025 eV. It is only at these low energies that the cross-section of U-235 is appreciable. So, a major challenge in reactor design is to moderate or slow down the fission neutrons. This can be achieved via either elastic or inelastic scattering: a) Elastic Scatter: Kinetic energy is conserved. This mechanism works well for neutrons with energies 10 MeV or below. Light nuclei, ones with low mass number, are best because the lighter the nucleus, the larger the fraction of energy lost per collision. b) Inelastic Scatter: The neutron forms an excited state with the target nucleus. This requires energy and the process is only effective for neutron energies above 0.1 MeV. Collisions with iron nuclei are the preferred approach. Neutron scattering is important in two aspects of nuclear engineering. One is the aforementioned neutron moderation.
    [Show full text]
  • ELEMENTARY PARTICLES in PHYSICS 1 Elementary Particles in Physics S
    ELEMENTARY PARTICLES IN PHYSICS 1 Elementary Particles in Physics S. Gasiorowicz and P. Langacker Elementary-particle physics deals with the fundamental constituents of mat- ter and their interactions. In the past several decades an enormous amount of experimental information has been accumulated, and many patterns and sys- tematic features have been observed. Highly successful mathematical theories of the electromagnetic, weak, and strong interactions have been devised and tested. These theories, which are collectively known as the standard model, are almost certainly the correct description of Nature, to first approximation, down to a distance scale 1/1000th the size of the atomic nucleus. There are also spec- ulative but encouraging developments in the attempt to unify these interactions into a simple underlying framework, and even to incorporate quantum gravity in a parameter-free “theory of everything.” In this article we shall attempt to highlight the ways in which information has been organized, and to sketch the outlines of the standard model and its possible extensions. Classification of Particles The particles that have been identified in high-energy experiments fall into dis- tinct classes. There are the leptons (see Electron, Leptons, Neutrino, Muonium), 1 all of which have spin 2 . They may be charged or neutral. The charged lep- tons have electromagnetic as well as weak interactions; the neutral ones only interact weakly. There are three well-defined lepton pairs, the electron (e−) and − the electron neutrino (νe), the muon (µ ) and the muon neutrino (νµ), and the (much heavier) charged lepton, the tau (τ), and its tau neutrino (ντ ). These particles all have antiparticles, in accordance with the predictions of relativistic quantum mechanics (see CPT Theorem).
    [Show full text]
  • Theory of Inelastic Lepton-Nucleus Scattering Granddon D
    Iowa State University Capstones, Theses and Retrospective Theses and Dissertations Dissertations 1988 Theory of inelastic lepton-nucleus scattering Granddon D. Yen Iowa State University Follow this and additional works at: https://lib.dr.iastate.edu/rtd Part of the Nuclear Commons Recommended Citation Yen, Granddon D., "Theory of inelastic lepton-nucleus scattering " (1988). Retrospective Theses and Dissertations. 9746. https://lib.dr.iastate.edu/rtd/9746 This Dissertation is brought to you for free and open access by the Iowa State University Capstones, Theses and Dissertations at Iowa State University Digital Repository. It has been accepted for inclusion in Retrospective Theses and Dissertations by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. INFORMATION TO USERS The most advanced technology has been used to photo­ graph and reproduce this manuscript from the microfilm master. UMI films the original text directly from the copy submitted. Thus, some dissertation copies are in typewriter face, while others may be from a computer printer. In the unlikely event that the author did not send UMI a complete manuscript and there are missing pages, these will be noted. Also, if unauthorized copyrighted material had to be removed, a note will indicate the deletion. Oversize materials (e.g., maps, drawings, charts) are re­ produced by sectioning the original, beginning at the upper left-hand comer and continuing from left to right in equal sections with small overlaps. Each oversize page is available as one exposure on a standard 35 mm slide or as a IT x 23" black and white photographic print for an additional charge.
    [Show full text]
  • Cross Sections for Neutron Inelastic Scattering and (N, 2N) Processes
    AE-88 00 Cross Sections for Neutron Inelastic 00 w < Scattering and (n, 2n) Processes. A Review of Available Experimental and Theoretical Data. M. Leimdörfer, E. Bock and L Arkeryd AKTIEBOLAGET ATOMENERGI STOCKHOLM SWEDEN 1962 AE-88 CROSS SECTIONS FOR NEUTRON INELASTIC SCATTERING AND ( n, 2n ) PROCESSES A Review of Available Experimental and Theoretical Data by M. Leimdörfer, E. Bock and L. Arkeryd Summary: A survey of the present state of knowledge on (n, n') and (n, 2n) reactions has been performed. The result is presented in the form of a main index to references on all elements and several special indices to different theoretical ways of approach, such as the direct-interaction concept, the continuum model (including level density theories), the discrete-level statistical model (Hauser-Feshbach), with a subsection on the optical model, 486 references accompanied with abstracts giving essential information pertaining to the field are supplied in the report. It is intended to keep this review up to date by regular issue of supplements. The abstracts have been arranged alphabetically according to the name of the first author. Printed and distributed in October 1962. Contents: Foreword page I Introduction I - V Main Coordinate Index Arranged According to Elements and Publishing Year VI - XXIV Subject Indices XXV - XXVI Author Index XXVII - XXXV Abstracts 1 - 486 A first edition of this report was issued as VDIT-50 (RFA-74) in Fehruary 1962. In the present, revised, edition such publica- tions as have appeared since the issue of the former report have been included, simultaneously as the.organization has been improved and, we hope, most of the inevitable printing errors have been removed.
    [Show full text]