Introduction to Nuclear Science

Similar documents
Introduction to Nuclear Science

Alpha Decay. Decay alpha particles are monoenergetic. Nuclides with A>150 are unstable against alpha decay. E α = Q (1-4/A)

Chapter Three (Nuclear Radiation)

Basic science. Atomic structure. Electrons. The Rutherford-Bohr model of an atom. Electron shells. Types of Electrons. Describing an Atom

Nuclear Physics. Chapter 43. PowerPoint Lectures for University Physics, Thirteenth Edition Hugh D. Young and Roger A. Freedman

Chapter 44. Nuclear Structure

There are 82 protons in a lead nucleus. Why doesn t the lead nucleus burst apart?

2007 Fall Nuc Med Physics Lectures

Physics of Radioactive Decay. Purpose. Return to our patient

Basic Nuclear Theory. Lecture 1 The Atom and Nuclear Stability

Introduction to Nuclear Physics and Nuclear Decay

Chapter 30 Nuclear Physics and Radioactivity

Chapter Four (Interaction of Radiation with Matter)

Some nuclei are unstable Become stable by ejecting excess energy and often a particle in the process Types of radiation particle - particle

Chem 481 Lecture Material 1/30/09

4 Nuclear Stability And Instability

Thursday, April 23, 15. Nuclear Physics

Lecture 33 Chapter 22, Sections 1-2 Nuclear Stability and Decay. Energy Barriers Types of Decay Nuclear Decay Kinetics

Fundamental Forces. Range Carrier Observed? Strength. Gravity Infinite Graviton No. Weak 10-6 Nuclear W+ W- Z Yes (1983)

General Physics (PHY 2140)

ZX or X-A where X is chemical symbol of element. common unit: [unified mass unit = u] also known as [atomic mass unit = amu] or [Dalton = Da]


Chapter 22 - Nuclear Chemistry

Chapter 37. Nuclear Chemistry. Copyright (c) 2011 by Michael A. Janusa, PhD. All rights reserved.

Lecture 1. Introduction to Nuclear Science

Units and Definition

Chapter VIII: Nuclear fission

Class XII Chapter 13 - Nuclei Physics

Types of radiation resulting from radioactive decay can be summarized in a simple chart. Only X-rays, Auger electrons and internal conversion

Nuclear Physics Fundamentals and Application Prof. H.C. Verma Department of Physics Indian Institute of Technology, Kanpur

Physics 3204 UNIT 3 Test Matter Energy Interface

Atomic and nuclear physics

Phys102 Lecture 29, 30, 31 Nuclear Physics and Radioactivity

NOTES: 25.2 Nuclear Stability and Radioactive Decay

α particles, β particles, and γ rays. Measurements of the energy of the nuclear

Physics 1C. Lecture 29A. "Nuclear powered vacuum cleaners will probably be a reality within 10 years. " --Alex Lewyt, 1955


Lesson 1. Introduction to Nuclear Science


General Physics (PHY 2140)

Nuclear Physics and Nuclear Reactions

Chemistry 132 NT. Nuclear Chemistry. Not everything that can be counted counts, and not everything that counts can be counted.

α particles, β particles, and γ rays. Measurements of the energy of the nuclear

LECTURE 23 NUCLEI. Instructor: Kazumi Tolich

Nuclear Physics Part 2A: Radioactive Decays

Atomic and Nuclear Radii

Chemistry 201: General Chemistry II - Lecture

Section 10: Natural Transmutation Writing Equations for Decay

Chapter 18: Radioactivity And Nuclear Transformation. Presented by Mingxiong Huang, Ph.D.,

6 Neutrons and Neutron Interactions

From Last Time. Stronger than coulomb force, But much shorter range than coulomb force.

Chapter 29. Nuclear Physics

Nuclear Reactions A Z. Radioactivity, Spontaneous Decay: Nuclear Reaction, Induced Process: x + X Y + y + Q Q > 0. Exothermic Endothermic

Nuclear Spectroscopy: Radioactivity and Half Life

Physics 107: Ideas of Modern Physics

Physics 107: Ideas of Modern Physics

Decay Mechanisms. The laws of conservation of charge and of nucleons require that for alpha decay, He + Q 3.1

16.5 Coulomb s Law Types of Forces in Nature. 6.1 Newton s Law of Gravitation Coulomb s Law

Sources of Radiation

Slide 1 / 57. Nuclear Physics & Nuclear Reactions Practice Problems

Chemistry 1000 Lecture 3: Nuclear stability. Marc R. Roussel

Nice Try. Introduction: Development of Nuclear Physics 20/08/2010. Nuclear Binding, Radioactivity. SPH4UI Physics

Instead, the probability to find an electron is given by a 3D standing wave.

Physics 107: Ideas of Modern Physics

FACTS WHY? C. Alpha Decay Probability 1. Energetics: Q α positive for all A>140 nuclei

CHAPTER 7 TEST REVIEW

Chapter 22. Preview. Objectives Properties of the Nucleus Nuclear Stability Binding Energy Sample Problem. Section 1 The Nucleus

Alpha decay, ssion, and nuclear reactions

Nuclear Fission Fission discovered by Otto Hahn and Fritz Strassman, Lisa Meitner in 1938

NUCLEI, RADIOACTIVITY AND NUCLEAR REACTIONS

H 1. Nuclear Physics. Nuclear Physics. 1. Parts of Atom. A. Nuclear Structure. 2b. Nomenclature. 2. Isotopes. AstroPhysics Notes

Multiple Choice Questions

Radioactivity. Radioactivity

CHEMISTRY Topic #1: Atomic Structure and Nuclear Chemistry Fall 2017 Dr. Susan Findlay See Exercises 2.3 to 2.6

RADIOACTIVITY. An atom consists of protons, neutrons and electrons.

Chapter 19 - Nuclear Chemistry Nuclear Stability and Modes of Decay

The IC electrons are mono-energetic. Their kinetic energy is equal to the energy of the transition minus the binding energy of the electron.

H 1. Nuclear Physics. Nuclear Physics. 1. Parts of Atom. 2. Isotopes. AstroPhysics Notes. Dr. Bill Pezzaglia. Rough draft. A.

Nuclear Medicine Treatments and Clinical Applications

Nuclear Physics for Applications

Introduction to Nuclear Engineering. Ahmad Al Khatibeh

Radioactivity and energy levels

Chapter 3 Radioactivity

Radioactive Decay and Radiometric Dating

β and γ decays, Radiation Therapies and Diagnostic, Fusion and Fission Final Exam Surveys New material Example of β-decay Beta decay Y + e # Y'+e +

RADIOACTIVITY. Nature of Radioactive Emissions

Chapter 19 - Nuclear Chemistry Nuclear Stability and Modes of Decay

Absorber Alpha emission Alpha particle Atom. Atomic line spectra Atomic mass unit Atomic number Atomic structure. Background radiation

The number of protons in the nucleus is known as the atomic number Z, and determines the chemical properties of the element.

Chapter 25. Nuclear Chemistry. Types of Radiation

Nuclear Physics. PHY232 Remco Zegers Room W109 cyclotron building.

Nuclides with excess neutrons need to convert a neutron to a proton to move closer to the line of stability.

1.1 ALPHA DECAY 1.2 BETA MINUS DECAY 1.3 GAMMA EMISSION 1.4 ELECTRON CAPTURE/BETA PLUS DECAY 1.5 NEUTRON EMISSION 1.6 SPONTANEOUS FISSION

Objectives: Atomic Structure: The Basics

3 Types of Nuclear Decay Processes

PHYSICS A2 UNIT 2 SECTION 1: RADIOACTIVITY & NUCLEAR ENERGY

RFSS: Lecture 2 Nuclear Properties

Chapter 12: Nuclear Reaction

Particles. Constituents of the atom

Nuclear Decays. Alpha Decay

Transcription:

Introduction to Nuclear Science PIXIE-PAN Summer Science Program University of Notre Dame 2006 Tony Hyder, Professor of Physics

Topics we will discuss Ground-state properties of the nucleus Radioactivity size, shape, stability, binding energies, angular momenta alpha, beta, and gamma decay The nuclear force Nuclear reactions the compound nucleus, Q values, excited states Decay modes of an excited nucleus

The radius of the nucleus

X(x,y)Y Q = (m x +m X -m y -m Y ) c 2

Some examples 10 Be + 14 N* 12 C + d 10 Be + 14 13 n

Cross section for the 10 Be + α reaction the resonances correspond to excited states of 14 N

The same kind of information about excited states of 14 N can be obtained by inelastic proton scattering

The effect of resonances on the cross section (here the neutron-capture on silver, can be quite dramatic. The dashed line is an extension of the1/v behavior expected in the absence of resonances

Before we leave this, look at the flipped version of the plot of B/A vs A that we saw earlier. Note that the rest energy per nucleon is less for intermediate mass nuclei than for very heavy or light ones.the key to fission

Of the 3000 or so known nuclides, there are only 266 whose ground states are stable. The rest are radioactive

Any idea what this is about?

Radioactivity For a nucleus to be radioactive at all, its mass must be greater than the sum of the masses of the decay products. We will look briefly at three types of decay: alpha, beta, and gamma Many of the heavy nuclei are unstable to alpha decay, and because the Coulomb barrier inhibits the decay process, the half life for alpha decay can be very long if the decay energy is small. All very heavy nuclei (Z>83) are theoretically unstable to α decay since the mass of the parent is greater than the sum of the masses of the decay products

Alpha decay The broken line is the line of stability, i.e., the floor of the energy valley we saw earlier

The alpha-particle spectrum from 227 Th the highest energy alpha particles corresponds to decay to the ground state of 223 Ra

The energy levels of 223 Ra can be determined from the measurement of the alpha-particle energies we saw in the pervious slide. Not all of the gamma-ray transitions are shown

Beta decay β decay: β + decay: A Z X N A Z+1 X N 1 + β A neutron changes into a proton and emits an electron A Z X N A Z 1 X N +1 + A proton changes into a neutron and emits a positron + ν e Q = (M P -M D )c 2 + β + e ν Q = (M P -M D + 2m e )c 2 Electron capture: a process that competes with β + decay in which a proton in the nucleus captures an atomic electron and changes into a neutron with the emission of a neutrino

The energy spectrum of electrons emitted in beta decay

Gamma decay A process in which a nucleus in an excited state decays to a lower energy state of the same isotope by the emission of a photon. We saw an example of this earlier in the decay of 223 Ra Internal conversion is a competing process especially for lower-lying energy states, in which the excitation energy of the state is transferred to an orbital electron which is ejected from the atom. The ejected electron is observed to have a kinetic energy equal to the nuclear transition energy minus the electron s atomic binding energy

The Nuclear Force About a hundred times stronger than the Coulomb force Very short range goes to zero beyond about 3 fm Charge independent does not matter if the particles are protons or neutrons Saturated is constant at about 8 MeV/nucleon above A=20 or so Depends on the spin orientation of the nucleons Suspected to be an exchange force in which the attraction is due to an exchange of pions

The nuclear shell model It is an independent-particle model, similar to that used for assigning energy states to atomic electrons, but opne that makes use of a strong spin-orbit coupling for each nucleon. It accounts for the shell-like structure of protons and neutrons and explains the magic numbers

Summary It s been a quick trip, but I hope a not too boring one. I tried to touch on a number of topics: Ground-state properties of the nucleus Radioactivity Nuclear reactions Decay modes of an excited nucleus, and The nuclear force I hope that there was something in there that you found interesting. If questions arise during the school year, please call (574.631.8591) or drop me a note at ahyder@nd.edu Tony Hyder