Question 1 (a) is the volume term. It reflects the nearest neighbor interactions. The binding energy is constant within it s value, so.

Similar documents
Particles. Constituents of the atom

Particle Physics Outline the concepts of particle production and annihilation and apply the conservation laws to these processes.

The Electro-Strong Interaction

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

APEX CARE INSTITUTE FOR PG - TRB, SLET AND NET IN PHYSICS

Wesley Smith, U. Wisconsin, January 21, Physics 301: Introduction - 1

CHAPTER 7 TEST REVIEW

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS

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

Introduction to Modern Physics Problems from previous Exams 3

Quantum Numbers. Elementary Particles Properties. F. Di Lodovico c 1 EPP, SPA6306. Queen Mary University of London. Quantum Numbers. F.

Contents. Preface to the First Edition Preface to the Second Edition

Physics 4213/5213 Lecture 1

Option 212: UNIT 2 Elementary Particles

Lecture 2: The First Second origin of neutrons and protons

Liquid Drop Model From the definition of Binding Energy we can write the mass of a nucleus X Z

Overview. The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions.

INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS

PHL424: 4 fundamental forces in nature

cgrahamphysics.com Particles that mediate force Book pg Exchange particles

Propagation in the Galaxy 2: electrons, positrons, antiprotons

Composite Nucleus (Activated Complex)

FYS3510 Subatomic Physics. Exam 2016

Final Exam Practice Solutions

3 Dimensional String Theory

SECTION A Quantum Physics and Atom Models

Chapter 44. Nuclear Structure

2007 Section A of examination problems on Nuclei and Particles

MODERN PHYSICS. A. s c B. dss C. u

UGC ACADEMY LEADING INSTITUE FOR CSIR-JRF/NET, GATE & JAM PHYSICAL SCIENCE TEST SERIES # 4. Atomic, Solid State & Nuclear + Particle

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

Electron-positron pairs can be produced from a photon of energy > twice the rest energy of the electron.

Isospin. K.K. Gan L5: Isospin and Parity 1

Nuclear and Radiation Physics

FYS 3510 Subatomic physics with applications in astrophysics. Nuclear and Particle Physics: An Introduction

PhysicsAndMathsTutor.com 1

.! " # e " + $ e. have the same spin as electron neutrinos, and is ½ integer (fermions).

PHY138Y Nuclear and Radiation

Write down the nuclear equation that represents the decay of neptunium 239 into plutonium 239.

Chapter VI: Beta decay

Option 212: UNIT 2 Elementary Particles

Visit for more fantastic resources. AQA. A Level. A Level Physics. Particles (Answers) Name: Total Marks: /30

Lecture 11. Weak interactions

PHY-105: Introduction to Particle and Nuclear Physics

At this time the quark model consisted of three particles, the properties of which are given in the table.

Thursday, April 23, 15. Nuclear Physics

The Proton Radius Puzzle and the Electro-Strong Interaction

Elementary Particle Physics Glossary. Course organiser: Dr Marcella Bona February 9, 2016

The Particle World. This talk: What is our Universe made of? Where does it come from? Why does it behave the way it does?

Particle Detectors. How to See the Invisible

DISCRETE SYMMETRIES IN NUCLEAR AND PARTICLE PHYSICS. Parity PHYS NUCLEAR AND PARTICLE PHYSICS

PHGN 422: Nuclear Physics Lecture 5: The Liquid Drop Model of the Nucleus

FACULTY OF SCIENCE. High Energy Physics. WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON

The Bohr Model of Hydrogen

Passage of particles through matter

Nuclear Physics and Astrophysics

Lecture 01. Introduction to Elementary Particle Physics

Books: - Martin, B.R. & Shaw, G Particle Physics (Wiley) (recommended) - Perkins, D.H. Introduction to High Energy Physics (CUP) (advanced)

FLAP P9.2 Radioactive decay COPYRIGHT 1998 THE OPEN UNIVERSITY S570 V1.1

Mirror Nuclei: Two nuclei with odd A in which the number of protons in one nucleus is equal to the number of neutrons in the other and vice versa.

The Physics of Particles and Forces David Wilson

Gian Gopal Particle Attributes Quantum Numbers 1

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

Physics 102: Lecture 28

SECTION A: NUCLEAR AND PARTICLE PHENOMENOLOGY

What did you learn in the last lecture?

Episode 536: Vector bosons and Feynman diagrams

1. What does this poster contain?

INTRODUCTION TO NUCLEAR AND PARTICLE PHYSICS

Workout Examples No.of nucleons Binding energy

PhysicsAndMathsTutor.com

2 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.

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

Invariance Principles and Conservation Laws

Chapter 30 Nuclear Physics and Radioactivity

The Charged Liquid Drop Model Binding Energy and Fission

3. Introductory Nuclear Physics 1; The Liquid Drop Model

Chapter 5. Par+cle Physics

Essential Physics II. Lecture 14:

Visit for more fantastic resources. OCR. A Level. A Level Physics. Particle physics (Answers) Name: Total Marks: /30

Alpha decay, ssion, and nuclear reactions

The Proper)es of Nuclei. Nucleons

9.2.E - Particle Physics. Year 12 Physics 9.8 Quanta to Quarks

Class XII - Physics Atoms Chapter-wise Problems

Fermi gas model. Introduction to Nuclear Science. Simon Fraser University Spring NUCS 342 February 2, 2011

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

Nuclear Physics and Nuclear Reactions

Particle Physics (concise summary) QuarkNet summer workshop June 24-28, 2013

1 Introduction. 1.1 The Standard Model of particle physics The fundamental particles

Particle Physics Lectures Outline

Physics 107: Ideas of Modern Physics

Physics 107: Ideas of Modern Physics

General Physics (PHY 2140)

Episode 535: Particle reactions

THE NUCLEUS OF AN ATOM

Quantum Numbers. F. Di Lodovico 1 EPP, SPA6306. Queen Mary University of London. Quantum Numbers. F. Di Lodovico. Quantum Numbers.

Nuclear and Particle Physics

FYS3510 Subatomic Physics. Exam 2016

Most of Modern Physics today is concerned with the extremes of matter:

A

Transcription:

Question (a) is the volume term. It reflects the nearest neighbor interactions. The binding energy is constant within it s value, so. + is the surface term. The volume term has to subtract this term since the nucleons at the surface feels a smaller nuclear force, as there are lesser neighbours. So 4. is the Coulomb term, the charge potential. The potential energy of the assumed uniformly charged sphere is. It is not, because the electrostatic repulsion will only exist for more than protons. So. is the symmetry term. It accounts for the fact that equal number of protons and neutrons in a nucleus seems to be stable for light nuclei. It is found that too many neutrons in the nucleus reduce the binding energy. However, the effect is small in light nuclei. It can be derived from the Fermi gas model, where Fermi energy is the maximum energy a particle can have in a potential well. This term is the difference between the total energy of the neutrons and protons with the energy for equal number of nucleons. is the pairing term. The binding energy is found to have the properties of, >, >,. So we consider this term as an addition to the, binding energy for even-even nuclei, and a subtraction when there are odd-odd nuclei. Question (b) (i) For large, the Coulomb term is very small. and are both very small, and when they multiply each other, that term is negligible. So = = 3 = 3

Question (b) (ii) For the nd term, PC33 Nuclear & Particle Physics AY/ Exam Solutions = = 3 = 3 For the 4 th term, = = 4 + 4 4 +4 = 4+ 4 +4 4 = 4 = 3, =4. Question (b) (iii) The first nuclei has even and even. So =. The second nuclei has odd and even. Since both have the same value of, then =. The difference in their neutron separation energies, Δ = = For large nuclei, Δ = + 3 4 =3 Question (a) 0, 3 0 =.

Question (b) (i) 5 5 + +, Δ=0,Δ=no It is an allowed decay. 5 + +, Δ=,Δ=no It is a nd forbidden decay. Question (b) (ii) and have odd number of neutrons, while protons. has odd number of Question (c) (i) 7 7 3 Question (c) (ii) Δ=,Δ=yes st forbidden decay Δ=,Δ=no nd forbidden decay There will be more of the excited state, because st forbidden decay means that it has a higher probability to decay compared to nd forbidden decay. Question (c) (iii) 4 7, Δ=yes 4,5,6,7 Question (d) (i) It is through weak interaction, a quark converts to a quark. Question (d) (ii) 3

Question 3 (a) Photopeak Compton continuum Double escape peak Single escape peak : rays lose all their energies in the detector. : happens when rays undergo Compton scattering and leave before they deposit all their energy. : occurs when a pair-production followed by position annihilation, producing photons and both photons escape. : same as double escape peak, but only one photon escapes. Question 3 (b) There are no escape peaks, since <.0MeV. The Compton edge, = + =0.478MeV. Question 3 (c) (i) 5 = 4 + + = 5 + = 5 = 5 = 4

Question 3 (c) (ii) 4 = + 4 + = = PC33 Nuclear & Particle Physics AY/ Exam Solutions Question 3 (d) (i) First scattering, = + = Second scattering, = + + + = + + 4 Question 3 (d) (ii) 4 = + 4 = +4 Question 4 (a) (i) = +, + = + + = + + 0 + + = + + = + + = = + + + Question 4 (a) (ii) + ++Higgs = 4 =7440 =7440GeV The threshold energy is freakin high. The colliding proton needs to be accelerated to such an enormous value of energy, which is quite impossible. If we use colliding beams instead, it will only require 0 =60GeV of energy, and so it is better to use colliding beams. 5

Question 4 (b) (i) Firstly, the particle should be, because the lepton generation number was violated. Next its corresponding arrow should be pointing outward, as it the lepton number was not conserved. Question 4 (b) (ii) Question 4 (c) (i) Charge conservation means that the initial charge and final charge must be the same. In the given examples, both equations obey this conservation since the charges before and after the reaction are the same. Charge conjugation is an operation to change the sign of charges by converting its particle to its anti-particle. It changes all internal quantum numbers: charge, baryon number, lepton number and strangeness, while keeping mass, energy, momentum and spin untouched. It is not conserved in weak interaction. The converstion of the first equation to the second equation is charge conjugation. Question 4 (c) (ii) Because neutrinos are left-handed. Question 4 (c) (iii) We introduce a parity change in the equation. 6

Question 4 (d) An anti-baryon has 3 anti quarks. Anti quarks have either charge or. We observe by mixing and matching, there are only 4 possible charges for antibaryons: 3 3 3 = 3 3 + 3 = 3 + 3 + 3 =0 3 + 3 + 3 = = for an anti-baryon is not allowed. Solutions provided by: John Soo (Qa-bi, ciii, 4c-d) Bong Kok Wei (Qbii-iii, a-cii, d, 3, 4a-b) 0, NUS Physics Society. 7