Total probability for reaction Yield
|
|
- Gloria Mathews
- 5 years ago
- Views:
Transcription
1 Total probability for reaction Yield If target has thickness d, and target material has # nuclei/volume: n 0 [part./cm 3 ] Y=σ n 0 d The yield gives the intensity of the characteristic signal from the reaction process per incoming particle with the cross section σ! It also gives the number of reaction products per incoming particle! N # incident particles/time [part/s] Y tot =σ n 0 d N gives total yield per unit time
2 Another Example Estimate the number of 14 C atoms produced in the mummy of Ramses II by 3290 years of cosmic ray bombardment! Cosmic ray flux at ground level of ~ particles/m 2 s. Adopt a cross section of σ = 0.1 barn for 14 N(n,p) 14 C. The living Ramses contained N particles and C particles.
3 Estimate of 14 C production & 14 C content Production: use standard production equation! Y( C) = σ [ barn] N( N) I [ particles m s] t Y( C) = [ cm ] [ particles m s] 3290[ y] Y( C) = [ cm ] [ particles cm s] [ s] Y( C) = cosmic particles are produced in the mummy. Content: use standard decay equation! N ( t ) = N N are (3290 (3290 N 0 y ) y ) e contained λ t = = in the e 15 ln y 14 mummy! C y particles
4 Absorption and Transmission I 0 I(d) Absorption and transmission of the initial beam with intensity I 0 depends on the target thickness d and total interaction cross section σ tot = σ i for all possible reactions between projectiles and target material of cross section σ i: d Id ( ) = I e 0 µ = n σ 0 i µ d i
5 Cosmic Ray Absorption in Atmosphere µ Id ( ) = I e d ; µ = n σ 0 0 i How many of the /cm 2 neutrons produced at 12 km height will reach the surface of the earth assuming an average nitrogen density of part/cm 3 and an interaction cross section of 0.1 barn? i 2 I ( 12km) = [n / cm s] e I n n 2 ( 12km) = 53. [n / cm s] [ N/ cm ] [ cm ] [ cm]
6 Interaction processes between projectile and target material atomic excitation processes X-ray-visible light (Coulomb Interaction between projectile and atomic electrons): elastic scattering processes (mechanical momentum without energy transfer): σ i [kbarn] char. particle energies inelastic scattering processes char. γ-radiation (mechanical momentum and energy transfer): radiative capture reactions char. γ-radiation (Coulomb Interaction between projectile and atomic nucleus): nuclear reaction processes (Strong Interaction between projectile and atomic nucleus): σ i [barn] σ i [barn] σ i [µbarn] char. particle radiation σ i [mbarn]
7 Radiation Detectors Radiation detectors are based on material which shows a high probability (cross section) for interacting with a particular kind of radiation (in a particular energy range)! The interaction process initiates an excitation or ionisation event in the material (e.g. atomic excitation, or solid state excitation) which results in light or particle emission which in turn can be used for generating an electrical pulse for analyzing and interpreting the event in the data acquisition electronics. There are three kind of detector materials: Scintillator Solid State Detector Ionisation Chamber X-ray, γ-ray, and neutron radiation particle- and γ-ray radiation particle radiation
8 Example: NaI scintillator Photons in the visible light range are created by excitation of NaI material with radiation photons are absorbed on photo cathode and generate free electrons by photo-effect electrons are multiplied in photo multiplier and converted to an electrical signal
9 Ionization chamber and semiconductor detectors Detectors are based on the principle of ionization along the track of energetic charged particle, production of ionelectron pairs, which are accelerated by attached electrical fields to anode or cathode pole of detector, charge pulse is converted in electrical pulse, pulse height corresponds to energy loss of initial energetic particle.
10 Summary Tools are needed to instigate the characteristic excitation processes by energy transfer The determination of the energy transfer in the excitation process requires the knowledge of the interaction probability cross section Tools are needed to analyze the characteristic light or radiation signatures High detection efficiency requires high absorption probability of radiation in detector high interaction cross section!
1.4 The Tools of the Trade!
1.4 The Tools of the Trade! Two things are required for material analysis: excitation mechanism for originating characteristic signature (radiation) radiation detection and identification system (spectroscopy)
More information1.5. The Tools of the Trade!
1.5. The Tools of the Trade! Two things are required for material analysis: excitation mechanism for originating characteristic signature (radiation) radiation detection and identification system (spectroscopy)
More informationNuclear Physics and Astrophysics
Nuclear Physics and Astrophysics PHY-30 Dr. E. Rizvi Lecture 4 - Detectors Binding Energy Nuclear mass MN less than sum of nucleon masses Shows nucleus is a bound (lower energy) state for this configuration
More informationThe interaction of radiation with matter
Basic Detection Techniques 2009-2010 http://www.astro.rug.nl/~peletier/detectiontechniques.html Detection of energetic particles and gamma rays The interaction of radiation with matter Peter Dendooven
More informationEEE4106Z Radiation Interactions & Detection
EEE4106Z Radiation Interactions & Detection 2. Radiation Detection Dr. Steve Peterson 5.14 RW James Department of Physics University of Cape Town steve.peterson@uct.ac.za May 06, 2015 EEE4106Z :: Radiation
More informationPhysics 736. Experimental Methods in Nuclear-, Particle-, and Astrophysics. Lecture 3
Physics 736 Experimental Methods in Nuclear-, Particle-, and Astrophysics Lecture 3 Karsten Heeger heeger@wisc.edu Review of Last Lecture a colleague shows you this data... what type of reaction is this?
More informationNeutron Interactions Part I. Rebecca M. Howell, Ph.D. Radiation Physics Y2.5321
Neutron Interactions Part I Rebecca M. Howell, Ph.D. Radiation Physics rhowell@mdanderson.org Y2.5321 Why do we as Medical Physicists care about neutrons? Neutrons in Radiation Therapy Neutron Therapy
More informationRadiation (Particle) Detection and Measurement
Radiation (Particle) Detection and Measurement Radiation detection implies that the radiation interacts (e.g. leaves at least part of its energy) in the material. A specific material is chosen, because
More informationParticle Energy Loss in Matter
Particle Energy Loss in Matter Charged particles loose energy when passing through material via atomic excitation and ionization These are protons, pions, muons, The energy loss can be described for moderately
More informationApplied Nuclear Physics (Fall 2006) Lecture 21 (11/29/06) Detection of Nuclear Radiation: Pulse Height Spectra
22.101 Applied Nuclear Physics (Fall 2006) Lecture 21 (11/29/06) Detection of Nuclear Radiation: Pulse Height Spectra References: W. E. Meyerhof, Elements of Nuclear Physics (McGraw-Hill, New York, 1967),
More informationToday, I will present the first of two lectures on neutron interactions.
Today, I will present the first of two lectures on neutron interactions. I first need to acknowledge that these two lectures were based on lectures presented previously in Med Phys I by Dr Howell. 1 Before
More informationCopyright 2008, University of Chicago, Department of Physics. Experiment VI. Gamma Ray Spectroscopy
Experiment VI Gamma Ray Spectroscopy 1. GAMMA RAY INTERACTIONS WITH MATTER In order for gammas to be detected, they must lose energy in the detector. Since gammas are electromagnetic radiation, we must
More informationScintillation Detector
Scintillation Detector Introduction The detection of ionizing radiation by the scintillation light produced in certain materials is one of the oldest techniques on record. In Geiger and Marsden s famous
More informationDetecting high energy photons. Interactions of photons with matter Properties of detectors (with examples)
Detecting high energy photons Interactions of photons with matter Properties of detectors (with examples) Interactions of high energy photons with matter Cross section/attenution length/optical depth Photoelectric
More informationAPPLIED RADIATION PHYSICS
A PRIMER IN APPLIED RADIATION PHYSICS F A SMITH Queen Mary & Westfield College, London fe World Scientific m Singapore * New Jersey London Hong Kong CONTENTS CHAPTER 1 : SOURCES of RADIATION 1.1 Introduction
More informationRadioactivity. Lecture 6 Detectors and Instrumentation
Radioactivity Lecture 6 Detectors and Instrumentation The human organs Neither humans nor animals have an organ for detecting radiation from radioactive decay! We can not hear it, smell it, feel it or
More informationhν' Φ e - Gamma spectroscopy - Prelab questions 1. What characteristics distinguish x-rays from gamma rays? Is either more intrinsically dangerous?
Gamma spectroscopy - Prelab questions 1. What characteristics distinguish x-rays from gamma rays? Is either more intrinsically dangerous? 2. Briefly discuss dead time in a detector. What factors are important
More informationParticle Energy Loss in Matter
Particle Energy Loss in Matter Charged particles, except electrons, loose energy when passing through material via atomic excitation and ionization These are protons, pions, muons, The energy loss can
More informationParticle Interactions in Detectors
Particle Interactions in Detectors Dr Peter R Hobson C.Phys M.Inst.P. Department of Electronic and Computer Engineering Brunel University, Uxbridge Peter.Hobson@brunel.ac.uk http://www.brunel.ac.uk/~eestprh/
More informationNeutron interactions and dosimetry. Eirik Malinen Einar Waldeland
Neutron interactions and dosimetry Eirik Malinen Einar Waldeland Topics 1. Neutron interactions 1. Scattering 2. Absorption 2. Neutron dosimetry 3. Applications The neutron Uncharged particle, mass close
More informationChapter V: Interactions of neutrons with matter
Chapter V: Interactions of neutrons with matter 1 Content of the chapter Introduction Interaction processes Interaction cross sections Moderation and neutrons path For more details see «Physique des Réacteurs
More informationRad T 290 Worksheet 2
Class: Date: Rad T 290 Worksheet 2 1. Projectile electrons travel from a. anode to cathode. c. target to patient. b. cathode to anode. d. inner shell to outer shell. 2. At the target, the projectile electrons
More informationIntroduction to Radiological Sciences Neutron Detectors. Theory of operation. Types of detectors Source calibration Survey for Dose
Introduction to Radiological Sciences Neutron Detectors Neutron counting Theory of operation Slow neutrons Fast neutrons Types of detectors Source calibration Survey for Dose 2 Neutrons, what are they?
More informationIII. Energy Deposition in the Detector and Spectrum Formation
1 III. Energy Deposition in the Detector and Spectrum Formation a) charged particles Bethe-Bloch formula de 4πq 4 z2 e 2m v = NZ ( ) dx m v ln ln 1 0 2 β β I 0 2 2 2 z, v: atomic number and velocity of
More informationGeneral Physics (PHY 2140)
General Physics (PHY 2140) Lecture 19 Modern Physics Nuclear Physics Nuclear Reactions Medical Applications Radiation Detectors Chapter 29 http://www.physics.wayne.edu/~alan/2140website/main.htm 1 Lightning
More informationGeneral Physics (PHY 2140)
General Physics (PHY 2140) Lightning Review Lecture 19 Modern Physics Nuclear Physics Nuclear Reactions Medical Applications Radiation Detectors Chapter 29 http://www.physics.wayne.edu/~alan/2140website/main.htm
More informationInteraction of Ionizing Radiation with Matter
Type of radiation charged particles photonen neutronen Uncharged particles Charged particles electrons (β - ) He 2+ (α), H + (p) D + (d) Recoil nuclides Fission fragments Interaction of ionizing radiation
More informationActivation Analysis. Characteristic decay mechanisms, α, β, γ Activity A reveals the abundance N:
2.5. Isotope analysis and neutron activation techniques The previously discussed techniques of material analysis are mainly based on the characteristic atomic structure of the elements and the associated
More informationPHYS 3446 Lecture #12
PHYS 3446 Lecture #12 Wednesday, Oct. 18, 2006 Dr. 1. Particle Detection Ionization Detectors MWPC Scintillation Counters Time of Flight 1 Announcements Next LPCC Workshop Preparation work Each group to
More informationEmphasis on what happens to emitted particle (if no nuclear reaction and MEDIUM (i.e., atomic effects)
LECTURE 5: INTERACTION OF RADIATION WITH MATTER All radiation is detected through its interaction with matter! INTRODUCTION: What happens when radiation passes through matter? Emphasis on what happens
More informationSOURCES of RADIOACTIVITY
Section 9: SOURCES of RADIOACTIVITY This section briefly describes various sources of radioactive nuclei, both naturally occurring and those produced artificially (man-made) in, for example, reactors or
More informationATOMIC WORLD P.1. ejected photoelectrons. current amplifier. photomultiplier tube (PMT)
ATOMIC WORLD P. HKAL PAPER I 0 8 The metal Caesium has a work function of.08 ev. Given: Planck constant h = 6.63 0 34 J s, charge of an electron e =.60 0 9 C (a) (i) Calculate the longest wavelength of
More informationOutline. Radiation Interactions. Spurs, Blobs and Short Tracks. Introduction. Radiation Interactions 1
Outline Radiation Interactions Introduction Interaction of Heavy Charged Particles Interaction of Fast Electrons Interaction of Gamma Rays Interactions of Neutrons Radiation Exposure & Dose Sources of
More informationChapter 3: Neutron Activation and Isotope Analysis
Chapter 3: Neutron Activation and Isotope Analysis 3.1. Neutron Activation Techniques 3.2. Neutron Activation of Paintings 3.3. From Qumran to Napoleon 3.4. Neutron Activation with Accelerators 3.5. Isotope
More informationRadiation Detection for the Beta- Delayed Alpha and Gamma Decay of 20 Na. Ellen Simmons
Radiation Detection for the Beta- Delayed Alpha and Gamma Decay of 20 Na Ellen Simmons 1 Contents Introduction Review of the Types of Radiation Charged Particle Radiation Detection Review of Semiconductor
More information6 Neutrons and Neutron Interactions
6 Neutrons and Neutron Interactions A nuclear reactor will not operate without neutrons. Neutrons induce the fission reaction, which produces the heat in CANDU reactors, and fission creates more neutrons.
More informationLecture 4. Detectors for Ionizing Particles
Lecture 4 Detectors for Ionizing Particles Introduction Overview of detector systems Sources of radiation Radioactive decay Cosmic Radiation Accelerators Content Interaction of Radiation with Matter General
More informationShell Atomic Model and Energy Levels
Shell Atomic Model and Energy Levels (higher energy, deeper excitation) - Radio waves: Not absorbed and pass through tissue un-attenuated - Microwaves : Energies of Photos enough to cause molecular rotation
More informationScience of Nuclear Energy and Radiation a Comprehensive Course for Science Teachers June 22-25, 1998 McMaster University
Science of Nuclear Energy and Radiation a Comprehensive Course for Science Teachers June 22-25, 1998 McMaster University Notes to accompany Lab demonstrations by Barry Diacon, Technician, Department of
More informationContents. Charged Particles. Coulomb Interactions Elastic Scattering. Coulomb Interactions - Inelastic Scattering. Bremsstrahlung
Contents Marcel MiGLiERiNi Nuclear Medicine, Radiology and Their Metrological Aspects. Radiation in Medicine. Dosimetry 4. Diagnostics & Therapy 5. Accelerators in Medicine 6. Therapy Planning 7. Nuclear
More informationCHAPTER 12 TEST REVIEW
IB PHYSICS Name: Period: Date: # Marks: 76 Raw Score: IB Curve: DEVIL PHYSICS BADDEST CLASS ON CAMPUS CHAPTER 12 TEST REVIEW 1. An alpha particle is accelerated through a potential difference of 10 kv.
More informationChemistry 311: Instrumentation Analysis Topic 2: Atomic Spectroscopy. Chemistry 311: Instrumentation Analysis Topic 2: Atomic Spectroscopy
Topic 2b: X-ray Fluorescence Spectrometry Text: Chapter 12 Rouessac (1 week) 4.0 X-ray Fluorescence Download, read and understand EPA method 6010C ICP-OES Winter 2009 Page 1 Atomic X-ray Spectrometry Fundamental
More informationPhotons: Interactions
Photons: Interactions Photons appear in detector systems as primary photons, created in Bremsstrahlung and de-excitations Photons are also used for medical applications, both imaging and radiation treatment.
More informationB. Rouben McMaster University Course EP 4D03/6D03 Nuclear Reactor Analysis (Reactor Physics) 2015 Sept.-Dec.
2: Fission and Other Neutron Reactions B. Rouben McMaster University Course EP 4D03/6D03 Nuclear Reactor Analysis (Reactor Physics) 2015 Sept.-Dec. 2015 September 1 Contents Concepts: Fission and other
More informationLecture 14 Krane Enge Cohen Williams Nuclear Reactions Ch 11 Ch 13 Ch /2 7.5 Reaction dynamics /4 Reaction cross sections 11.
Lecture 14 Krane Enge Cohen Williams Nuclear Reactions Ch 11 Ch 13 Ch 13 7.1/2 7.5 Reaction dynamics 11.2 13.2 7.3/4 Reaction cross sections 11.4 2.10 Reaction theories compound nucleus 11.10 13.7 13.1-3
More informationAtoms, Radiation, and Radiation Protection
James E. Turner Atoms, Radiation, and Radiation Protection Third, Completely Revised and Enlarged Edition BICENTENNIAL J 0 1 8 0 Q 71 z m z CAVILEY 2007 1 ;Z z ü ; m r B10ENTENNIAL WILEY-VCH Verlag GmbH
More informationenergy loss Ionization + excitation of atomic energy levels Mean energy loss rate de /dx proportional to (electric charge) 2 of incident particle
Lecture 4 Particle physics processes - particles are small, light, energetic à processes described by quantum mechanics and relativity à processes are probabilistic, i.e., we cannot know the outcome of
More informationNeutrino Helicity Measurement
PHYS 851 Introductory Nuclear Physics Instructor: Chary Rangacharyulu University of Saskatchewan Neutrino Helicity Measurement Stefan A. Gärtner stefan.gaertner@gmx.de December 9 th, 2005 2 1 Introduction
More informationRadiation Quantities and Units
Radiation Quantities and Units George Starkschall, Ph.D. Lecture Objectives Define and identify units for the following: Exposure Kerma Absorbed dose Dose equivalent Relative biological effectiveness Activity
More informationParticle Detectors. How to See the Invisible
Particle Detectors How to See the Invisible Which Subatomic Particles are Seen? Which particles live long enough to be visible in a detector? 2 Which Subatomic Particles are Seen? Protons Which particles
More informationElastic scattering. Elastic scattering
Elastic scattering Now we have worked out how much energy is lost when a neutron is scattered through an angle, θ We would like to know how much energy, on average, is lost per collision In order to do
More informationCHARGED PARTICLE INTERACTIONS
CHARGED PARTICLE INTERACTIONS Background Charged Particles Heavy charged particles Charged particles with Mass > m e α, proton, deuteron, heavy ion (e.g., C +, Fe + ), fission fragment, muon, etc. α is
More informationDR KAZI SAZZAD MANIR
DR KAZI SAZZAD MANIR PHOTON BEAM MATTER ENERGY TRANSFER IONISATION EXCITATION ATTENUATION removal of photons from the beam by the matter. ABSORPTION SCATTERING TRANSMISSION Taking up the energy from the
More informationChemistry Instrumental Analysis Lecture 19 Chapter 12. Chem 4631
Chemistry 4631 Instrumental Analysis Lecture 19 Chapter 12 There are three major techniques used for elemental analysis: Optical spectrometry Mass spectrometry X-ray spectrometry X-ray Techniques include:
More informationJohn Ellison University of California, Riverside. Quarknet 2008 at UCR
Cosmic Rays John Ellison University of California, Riverside Quarknet 2008 at UCR 1 What are Cosmic Rays? Particles accelerated in astrophysical sources incident on Earth s atmosphere Possible sources
More informationDetectors for High Energy Physics
Detectors for High Energy Physics Ingrid-Maria Gregor, DESY DESY Summer Student Program 2017 Hamburg July 26th/27th Disclaimer Particle Detectors are very complex, a lot of physics is behind the detection
More informationCross-Sections for Neutron Reactions
22.05 Reactor Physics Part Four Cross-Sections for Neutron Reactions 1. Interactions: Cross-sections deal with the measurement of interactions between moving particles and the material through which they
More informationA Comparison between Channel Selections in Heavy Ion Reactions
Brazilian Journal of Physics, vol. 39, no. 1, March, 2009 55 A Comparison between Channel Selections in Heavy Ion Reactions S. Mohammadi Physics Department, Payame Noor University, Mashad 91735, IRAN (Received
More informationNuclear Reactions A Z. Radioactivity, Spontaneous Decay: Nuclear Reaction, Induced Process: x + X Y + y + Q Q > 0. Exothermic Endothermic
Radioactivity, Spontaneous Decay: Nuclear Reactions A Z 4 P D+ He + Q A 4 Z 2 Q > 0 Nuclear Reaction, Induced Process: x + X Y + y + Q Q = ( m + m m m ) c 2 x X Y y Q > 0 Q < 0 Exothermic Endothermic 2
More informationPhysics 736. Experimental Methods in Nuclear-, Particle-, and Astrophysics. Lecture 4
Physics 736 Experimental Methods in Nuclear-, Particle-, and Astrophysics Lecture 4 Karsten Heeger heeger@wisc.edu Homework Homework is posted on course website http://neutrino.physics.wisc.edu/teaching/phys736/
More informationQuality Assurance. Purity control. Polycrystalline Ingots
Quality Assurance Purity control Polycrystalline Ingots 1 Gamma Spectrometry Nuclide Identification Detection of Impurity Traces 1.1 Nuclides Notation: Atomic Mass Atomic Number Element Neutron Atomic
More informationLECTURE 4 PRINCIPLE OF IMAGE FORMATION KAMARUL AMIN BIN ABDULLAH
LECTURE 4 PRINCIPLE OF IMAGE FORMATION KAMARUL AMIN BIN ABDULLAH Lesson Objectives At the end of the lesson, student should able to: Define attenuation Explain interactions between x-rays and matter in
More information2 Give the compound nucleus resulting from 6-MeV protons bombarding a target of. my notes in the part 3 reading room or on the WEB.
Lecture 15 Krane Enge Cohen Williams Reaction theories compound nucleus 11.10 13.7 13.1-3 direct reactions 11.11 13.11/12 ch 14 Admixed Wave functions residual interaction 5.1-4 Admixed Wave functions
More informationPHYS 5012 Radiation Physics and Dosimetry
Radiative PHYS 5012 Radiation Physics and Dosimetry Mean Tuesday 24 March 2009 Radiative Mean Radiative Mean Collisions between two particles involve a projectile and a target. Types of targets: whole
More informationDecays and Scattering. Decay Rates Cross Sections Calculating Decays Scattering Lifetime of Particles
Decays and Scattering Decay Rates Cross Sections Calculating Decays Scattering Lifetime of Particles 1 Decay Rates There are THREE experimental probes of Elementary Particle Interactions - bound states
More informationNuclear Physics. (PHY-231) Dr C. M. Cormack. Nuclear Physics This Lecture
Nuclear Physics (PHY-31) Dr C. M. Cormack 11 Nuclear Physics This Lecture This Lecture We will discuss an important effect in nuclear spectroscopy The Mössbauer Effect and its applications in technology
More information(i) Show that the energy of a single photon is about 3 x J.
1(a) A helium-neon laser emits red light of wavelength 6.3 x 10 7 m. (i) Show that the energy of a single photon is about 3 x 10 19 J. [2] The power of the laser beam is 1.0 mw. Show that about 3 x 10
More informationO WILEY- MODERN NUCLEAR CHEMISTRY. WALTER D. LOVELAND Oregon State University. DAVID J. MORRISSEY Michigan State University
MODERN NUCLEAR CHEMISTRY WALTER D. LOVELAND Oregon State University DAVID J. MORRISSEY Michigan State University GLENN T. SEABORG University of California, Berkeley O WILEY- INTERSCIENCE A JOHN WILEY &
More informationPARTICLES REVELATION THROUGH SCINTILLATION COUNTER
14-25 JUNE 2004 SUMMER STAGE PARTICLES REVELATION THROUGH SCINTILLATION COUNTER by Flavio Cavalli and Marcello De Vitis Liceo Scientifico Statale Farnesina Tutor: Marco Mirazita 1) COSMIC RAYS - The Muons
More informationLECTURE 6: INTERACTION OF RADIATION WITH MATTER
LCTUR 6: INTRACTION OF RADIATION WITH MATTR All radiation is detected through its interaction with matter! INTRODUCTION: What happens when radiation passes through matter? Interlude The concept of cross-section
More informationChapter 2 Radiation-Matter Interactions
Chapter 2 Radiation-Matter Interactions The behavior of radiation and matter as a function of energy governs the degradation of astrophysical information along the path and the characteristics of the detectors.
More informationLAB 4: Gamma-ray coincidence spectrometry (2018)
LAB 4: Gamma-ray coincidence spectrometry (2018) As you have seen, in several of the radioactive sources we encountered so far, they typically emit more than one gamma photon per decay or even more than
More informationBa (Z = 56) W (Z = 74) preferred target Mo (Z = 42) Pb (Z = 82) Pd (Z = 64)
Produced by accelerating electrons with high voltage and allowing them to collide with metal target (anode), e.g, Tungsten. Three Events (Two types of x-ray) a) Heat X-Ray Tube b) bremsstrahlung (braking
More informationLecture 32 April
Lecture 32 April 08. 2016. Hydrogen Discharge Tube and Emission of Discrete Wavelengths Description of the discrete Hydrogen Emission Spectrum by the Balmer (1884) Rydberg Ritz formula (1908) Cathode Ray
More informationLast Lecture 1) Silicon tracking detectors 2) Reconstructing track momenta
Last Lecture 1) Silicon tracking detectors 2) Reconstructing track momenta Today s Lecture: 1) Electromagnetic and hadronic showers 2) Calorimeter design Absorber Incident particle Detector Reconstructing
More informationNeutron Detection. n interactions with matter n detection High/low energy n detectors
Neutron Detection Example of n detection: Well logging Reservoir/Formation Evaluation Brief introduction to neutron generation Continuous sources Large accelerators Pulsed neutron generators n interactions
More informationINTERACTIONS OF RADIATION WITH MATTER
INTERACTIONS OF RADIATION WITH MATTER Renée Dickinson, MS, DABR Medical Physicist University of Washington Medical Center Department of Radiology Diagnostic Physics Section Outline Describe the various
More informationUniversity of Oslo. Department of Physics. Interaction Between Ionizing Radiation And Matter, Part 2 Charged-Particles.
Interaction Between Ionizing Radiation And Matter, Part Charged-Particles Audun Sanderud Excitation / ionization Incoming charged particle interact with atom/molecule: Ionization Excitation Ion pair created
More informationGeneral Physics (PHY 2140)
General Physics (PHY 2140) Lecture 37 Modern Physics Nuclear Physics Radioactivity Nuclear reactions http://www.physics.wayne.edu/~apetrov/phy2140/ Chapter 29 1 Lightning Review Last lecture: 1. Nuclear
More informationEEE4101F / EEE4103F Radiation Interactions & Detection
EEE4101F / EEE4103F Radiation Interactions & Detection 1. Interaction of Radiation with Matter Dr. Steve Peterson 5.14 RW James Department of Physics University of Cape Town steve.peterson@uct.ac.za March
More informationInteraction of Radiation with Matter
Bose Institute Interaction of Radiation with Matter Dhruba Gupta Department of Physics Bose Institute, Kolkata Winter School on Astroparticle Physics (WAPP 011) December 0-9, 9, 011 at Mayapuri,, Darjeeling
More informationChapter Four (Interaction of Radiation with Matter)
Al-Mustansiriyah University College of Science Physics Department Fourth Grade Nuclear Physics Dr. Ali A. Ridha Chapter Four (Interaction of Radiation with Matter) Different types of radiation interact
More informationX-ray Energy Spectroscopy (XES).
X-ray Energy Spectroscopy (XES). X-ray fluorescence as an analytical tool for element analysis is based on 3 fundamental parameters: A. Specificity: In determining an x-ray emission energy E certainty
More informationSCINTILLATION DETECTORS AND PM TUBES
SCINTILLATION DETECTORS AND PM TUBES General Characteristics Introduction Luminescence Light emission without heat generation Scintillation Luminescence by radiation Scintillation detector Radiation detector
More informationneutrons in the few kev to several MeV Neutrons are generated over a wide range of energies by a variety of different processes.
Neutrons 1932: Chadwick discovers the neutron 1935: Goldhaber discovers 10 B(n,α) 7 Li reaction 1936: Locher proposes boron neutron capture as a cancer therapy 1939: Nuclear fission in 235 U induced by
More informationDedicated Arrays: MEDEA GDR studies (E γ = MeV) Highly excited CN E*~ MeV, 4 T 8 MeV
Dedicated Arrays: MEDEA GDR studies (E γ = 10-25 MeV) Highly excited CN E*~ 250-350 MeV, 4 T 8 MeV γ-ray spectrum intermediate energy region 10 MeV/A E beam 100 MeV/A - large variety of emitted particles
More informationIntroduction to Nuclear Engineering
2016/9/27 Introduction to Nuclear Engineering Kenichi Ishikawa ( ) http://ishiken.free.fr/english/lecture.html ishiken@n.t.u-tokyo.ac.jp 1 References Nuclear Physics basic properties of nuclei nuclear
More informationBasic physics Questions
Chapter1 Basic physics Questions S. Ilyas 1. Which of the following statements regarding protons are correct? a. They have a negative charge b. They are equal to the number of electrons in a non-ionized
More informationPlanetary Atmospheres Part 2
Planetary Atmospheres Part 2 Atmospheric Layers: The temperature gradient (whether it increases or decreases with altitude) is set by the type of absorption that occurs. We can affect this! Photo- disassocia,on
More informationPrinciples and Applications of Neutron Based Inspection Techniques. Tsahi Gozani Rapiscan Laboratories 520Almanor Ave, Sunnyvale, CA
Principles and Applications of Neutron Based Inspection Techniques Tsahi Gozani Rapiscan Laboratories 520Almanor Ave, Sunnyvale, CA Presentation to the International Topical meeting on Nuclear Research
More informationPhysics 3204 UNIT 3 Test Matter Energy Interface
Physics 3204 UNIT 3 Test Matter Energy Interface 2005 2006 Time: 60 minutes Total Value: 33 Marks Formulae and Constants v = f λ E = hf h f = E k + W 0 E = m c 2 p = h λ 1 A= A T 0 2 t 1 2 E k = ½ mv 2
More information2. Passage of Radiation Through Matter
2. Passage of Radiation Through Matter Passage of Radiation Through Matter: Contents Energy Loss of Heavy Charged Particles by Atomic Collision (addendum) Cherenkov Radiation Energy loss of Electrons and
More informationAppendix A2. Particle Accelerators and Detectors The Large Hadron Collider (LHC) in Geneva, Switzerland on the Border of France.
Appendix A. Particle Accelerators and Detectors The Large Hadron Collider (LHC) in Geneva, Switzerland on the Border of France. Prepared by: Arash Akbari-Sharbaf Why Build Accelerators? Probe deeper From
More informationPrinciples of neutron TOF cross section measurements
Principles of neutron TOF cross section measurements J. Heyse, C. Paradela, P. Schillebeeckx EC JRC IRMM Standards for Nuclear Safety, Security and Safeguards (SN3S) H.I. Kim Korea Atomic Energy Research
More informationRadioactivity. The Nobel Prize in Physics 1903 for their work on radioactivity. Henri Becquerel Pierre Curie Marie Curie
Radioactivity Toward the end of the 19 th century, minerals were found that would darken a photographic plate even in the absence of light. This phenomenon is now called radioactivity. Marie and Pierre
More informationAPEX CARE INSTITUTE FOR PG - TRB, SLET AND NET IN PHYSICS
Page 1 1. Within the nucleus, the charge distribution A) Is constant, but falls to zero sharply at the nuclear radius B) Increases linearly from the centre, but falls off exponentially at the surface C)
More informationLecture 3 - Compton Scattering
Lecture 3 - Compton Scattering E. Daw March 0, 01 1 Review of Lecture Last time we recalled that in special relativity, as in pre-relativistic dynamics, the total energy in an interaction or collision
More informationInteraction of Particles and Matter
MORE CHAPTER 11, #7 Interaction of Particles and Matter In this More section we will discuss briefly the main interactions of charged particles, neutrons, and photons with matter. Understanding these interactions
More informationWithin the vast field of atomic physics, collisions of heavy ions with atoms define
Chapter 1 Introduction Within the vast field of atomic physics, collisions of heavy ions with atoms define one of the most active areas of research. In the last decades, the design and construction of
More informationIntroduction to Electromagnetic Radiation and Radiative Transfer
Introduction to Electromagnetic Radiation and Radiative Transfer Temperature Dice Results Visible light, infrared (IR), ultraviolet (UV), X-rays, γ-rays, microwaves, and radio are all forms of electromagnetic
More information