Physics 492 Lecture 28

Size: px
Start display at page:

Download "Physics 492 Lecture 28"

Transcription

1 Physics 492 Lecture 28 Main points of last lecture: Feynman diagrams. Main points of today s lecture:. Nuclear forces: charge exchange pion exchange Yukawa force deuteron charge independence, isospin symmetry Introduction to H.E.P

2 Strong interaction diagrams The short range of the nuclear force suggests that it can result from the exchange of a massive particle. candidate is pion 3 such particles Range of force Born Approximation

3 NN forces Relevant diagrams for NN forces in one pion exchange limit:

4 Charge exchange in N-N scattering n-p differential cross section is backward peaked.

5 Charge symmetry Pions have nearly equal masses: m(π + )= m(π -- ) m(π 0 ): (m(u)=m(d)) charge symmetry for Z=N±1

6 Charge symmetry is general feature Charge independence Similar (analogue) states

7 Charge independence: Isospin Symmetry Consider p and n to be two different states of a nucleon. T 3 =-1 T 3 =1 6 He 0 + g.s. 6 Li 0 + ex.s. 6 Be 0 + g.s.

8 Deuteron Deuteron is also T=0 isospin is completely analogous to spin The reason for this formalism is that charged pion exchange switches neutrons into protons and vice versa; it is useful to consider neutrons and protons to be different states of a nucleon or to consider their quark substructure where u and d quarks have equal masses.

9 Physics 492 Lecture 29 Main points of last lecture: Nuclear forces: charge exchange pion exchange Yukawa force deuteron charge independence, isospin symmetry Main points of today s lecture: Short lived particles. measurements of unstable particles. Measurements of resonances. Quark model spin ½ nucleons pseudoscaler mesons vector mesons. spin 3/2 baryons

10 Deuteron Deuteron is also T=0 isospin is completely analogous to spin The reason for this formalism is that charged pion exchange switches neutrons into protons and vice versa; it is useful to consider neutrons and protons to be different states of a nucleon or to consider their quark substructure where u and d quarks have equal masses.

11 Detection of fast particles Tools for measurement: de/dx for charged particles silicon use magnets to measure p + h+ e-

12 TPC: 3-D coordinates, event reconstruction Z coordinate from drift time in Electric field X coordinate and y coordinates from charge induced on cathode pad below the wire plane 3 dimensional event reconstruction, with energies and particle types. B v z π track E v projected track y B v E v x wire plane and pads below

13 neutral particles? neutrals? Use Time of Flight (TOF)

14 Very Short lived particles Study resonances ( )( ( ) ( ) 2 p p p p 2 2 p k p k p k p k p g c m k p p π π ν π ν μ π μ μν Δ μ π μ μ Δ v v + = + + = + =

15 Quark model Define constituents: quarks start with lightest quarks u and d: Organize particles and resonances: Baryons (First nucleons)

16 Nucleon Wavefunction Skematic wavefunction in terms of quarks: Need another quantum number (color) to satisfy Pauli principle: Explains charge of nucleon. How about spin? What is probability of 2 u quark spin up and one d quark spin down?

17 Quark model Mesons first pions

18 Intrinsic Parity

19 Physics 492 Lecture 30 Main points of last lecture: Short lived particles. measurements of unstable particles. Measurements of resonances. Quark model spin ½ nucleons Main points of today s lecture: Quark model pseudoscaler mesons vector mesons. spin 3/2 baryons Quark-flow diagrams for reactions S- quarks mesons baryons Production and decay of strange particles C and B quarks

20 From last lecture: Pion quark wave function

21 η (eta) meson

22 Progress so far

23 Vector Mesons The quark-quark interaction is spin dependent. Baryons with spins aligned have higher energies.

24 S=3/2 Baryons Aligned spins have higher energies. Color is needed to satisfy Pauli exclusion principle.

25 Higher L?

26 Quark-flow diagrams Particle production can be described by following the quark lines.

27 Strangeness s quark Mesons:

28 Baryons Strangeness

29 Overall picture: strange baryons

Hadronic Resonances in a Hadronic Picture. Daisuke Jido (Nuclear physics group)

Hadronic Resonances in a Hadronic Picture. Daisuke Jido (Nuclear physics group) Daisuke Jido (Nuclear physics group) Hadrons (particles interacting with strong interactions) are composite objects of quarks and gluons. It has been recently suggested that the structures of some hadrons

More information

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

Electron-positron pairs can be produced from a photon of energy > twice the rest energy of the electron. Particle Physics Positron - discovered in 1932, same mass as electron, same charge but opposite sign, same spin but magnetic moment is parallel to angular momentum. Electron-positron pairs can be produced

More information

Gian Gopal Particle Attributes Quantum Numbers 1

Gian Gopal Particle Attributes Quantum Numbers 1 Particle Attributes Quantum Numbers Intro Lecture Quantum numbers (Quantised Attributes subject to conservation laws and hence related to Symmetries) listed NOT explained. Now we cover Electric Charge

More information

The Development of Particle Physics. Dr. Vitaly Kudryavtsev E45, Tel.:

The Development of Particle Physics. Dr. Vitaly Kudryavtsev E45, Tel.: The Development of Particle Physics Dr. Vitaly Kudryavtsev E45, Tel.: 0114 2224531 v.kudryavtsev@sheffield.ac.uk Previous lecture New unstable particles discovered in 40s-50s. First hyperons (particles

More information

Problem Set # 1 SOLUTIONS

Problem Set # 1 SOLUTIONS Wissink P640 Subatomic Physics I Fall 2007 Problem Set # 1 S 1. Iso-Confused! In lecture we discussed the family of π-mesons, which have spin J = 0 and isospin I = 1, i.e., they form the isospin triplet

More information

Nuclear and Particle Physics 3: Particle Physics. Lecture 1: Introduction to Particle Physics February 5th 2007

Nuclear and Particle Physics 3: Particle Physics. Lecture 1: Introduction to Particle Physics February 5th 2007 Nuclear and Particle Physics 3: Particle Physics Lecture 1: Introduction to Particle Physics February 5th 2007 Particle Physics (PP) a.k.a. High-Energy Physics (HEP) 1 Dr Victoria Martin JCMB room 4405

More information

January 31, PHY357 Lecture 8. Quark composition of hadrons. Hadron magnetic moments. Hadron masses

January 31, PHY357 Lecture 8. Quark composition of hadrons. Hadron magnetic moments. Hadron masses January 3, 08 PHY357 Lecture 8 Quark composition of hadrons Hadron magnetic moments Hadron masses January 3, 08 Quark rules for building Hadrons! Three types of stable quark configurations established!

More information

Lecture 8. CPT theorem and CP violation

Lecture 8. CPT theorem and CP violation Lecture 8 CPT theorem and CP violation We have seen that although both charge conjugation and parity are violated in weak interactions, the combination of the two CP turns left-handed antimuon onto right-handed

More information

Lecture 3: Quarks and Symmetry in Quarks

Lecture 3: Quarks and Symmetry in Quarks Lecture 3: Quarks and Symmetry in Quarks Quarks Cross Section, Fermions & Bosons, Wave Eqs. Symmetry: Rotation, Isospin (I), Parity (P), Charge Conjugate (C), SU(3), Gauge symmetry Conservation Laws: http://faculty.physics.tamu.edu/kamon/teaching/phys627/

More information

Discovery of charged bottomonium-like Z b states at Belle

Discovery of charged bottomonium-like Z b states at Belle Discovery of charged bottomonium-like Z b states at Belle Antje Peters 1 Christoph Rosenbaum 2 1 Goethe-Universität Frankfurt am Main 2 Justus-Liebig-Universität Giessen HGS-HIRe Lecture Week on Hadron

More information

Clebsch-Gordan Coefficients

Clebsch-Gordan Coefficients Phy489 Lecture 7 Clebsch-Gordan Coefficients 2 j j j2 m m m 2 j= j j2 j + j j m > j m > = C jm > m = m + m 2 2 2 Two systems with spin j and j 2 and z components m and m 2 can combine to give a system

More information

Evidence for the Strong Interaction

Evidence for the Strong Interaction Evidence for the Strong Interaction Scott Wilbur Scott Wilbur Evidence for the Strong Interaction 1 Overview Continuing search inside fundamental particles Scott Wilbur Evidence for the Strong Interaction

More information

Lecture 9. Isospin The quark model

Lecture 9. Isospin The quark model Lecture 9 Isospin The quark model There is one more symmetry that applies to strong interactions. isospin or isotopic spin It was useful in formulation of the quark picture of known particles. We can consider

More information

3. Introductory Nuclear Physics 1; The Liquid Drop Model

3. Introductory Nuclear Physics 1; The Liquid Drop Model 3. Introductory Nuclear Physics 1; The Liquid Drop Model Each nucleus is a bound collection of N neutrons and Z protons. The mass number is A = N + Z, the atomic number is Z and the nucleus is written

More information

Lecture 8. CPT theorem and CP violation

Lecture 8. CPT theorem and CP violation Lecture 8 CPT theorem and CP violation We have seen that although both charge conjugation and parity are violated in weak interactions, the combination of the two CP turns left-handed antimuon onto right-handed

More information

Quarks and the Baryons

Quarks and the Baryons Quarks and the Baryons A Review of Chapter 15 of Particles and Nuclei by Povh Evan Phelps University of South Carolina Department of Physics and Astronomy phelps@physics.sc.edu March 18, 2009 Evan Phelps

More information

Dr Victoria Martin, Prof Steve Playfer Spring Semester 2013

Dr Victoria Martin, Prof Steve Playfer Spring Semester 2013 Particle Physics Dr Victoria Martin, Prof Steve Playfer Spring Semester 2013 Lecture 12: Mesons and Baryons Mesons and baryons Strong isospin and strong hypercharge SU(3) flavour symmetry Heavy quark states

More information

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

Particle Physics Outline the concepts of particle production and annihilation and apply the conservation laws to these processes. Particle Physics 12.3.1 Outline the concept of antiparticles and give examples 12.3.2 Outline the concepts of particle production and annihilation and apply the conservation laws to these processes. Every

More information

2007 Section A of examination problems on Nuclei and Particles

2007 Section A of examination problems on Nuclei and Particles 2007 Section A of examination problems on Nuclei and Particles 1 Section A 2 PHYS3002W1 A1. A fossil containing 1 gramme of carbon has a radioactivity of 0.03 disintegrations per second. A living organism

More information

wave functions PhD seminar- FZ Juelich, Feb 2013

wave functions PhD seminar- FZ Juelich, Feb 2013 SU(3) symmetry and Baryon wave functions Sedigheh Jowzaee PhD seminar- FZ Juelich, Feb 2013 Introduction Fundamental symmetries of our universe Symmetry to the quark model: Hadron wave functions q q Existence

More information

The Standard Model (part I)

The Standard Model (part I) The Standard Model (part I) Speaker Jens Kunstmann Student of Physics in 5 th year at Greifswald University, Germany Location Sommerakademie der Studienstiftung, Kreisau 2002 Topics Introduction The fundamental

More information

The SU(3) Group SU(3) and Mesons Contents Quarks and Anti-quarks SU(3) and Baryons Masses and Symmetry Breaking Gell-Mann Okubo Mass Formulae Quark-Mo

The SU(3) Group SU(3) and Mesons Contents Quarks and Anti-quarks SU(3) and Baryons Masses and Symmetry Breaking Gell-Mann Okubo Mass Formulae Quark-Mo Lecture 2 Quark Model The Eight Fold Way Adnan Bashir, IFM, UMSNH, Mexico August 2014 Culiacán Sinaloa The SU(3) Group SU(3) and Mesons Contents Quarks and Anti-quarks SU(3) and Baryons Masses and Symmetry

More information

Nuclear Force. Spin dependent difference in neutron scattering. Compare n-p to n-n and p-p Charge independence of nuclear force.

Nuclear Force. Spin dependent difference in neutron scattering. Compare n-p to n-n and p-p Charge independence of nuclear force. Nuclear Force Spin dependent difference in neutron scattering cross sections of ortho- and para-hydrogen. Compare n-p to n-n and p-p Charge independence of nuclear force. Nuclear and Radiation Physics,

More information

Physics 125 Course Notes Identical Particles Solutions to Problems F. Porter

Physics 125 Course Notes Identical Particles Solutions to Problems F. Porter Physics 5 Course Notes Identical Particles Solutions to Problems 00 F. Porter Exercises. Let us use the Pauli exclusion principle, and the combination of angular momenta, to find the possible states which

More information

Quantum ChromoDynamics (Nobel Prize 2004) Chris McLauchlin

Quantum ChromoDynamics (Nobel Prize 2004) Chris McLauchlin Quantum ChromoDynamics (Nobel Prize 2004) Chris McLauchlin Outline The Four Fundamental Forces The Strong Force History of the Strong Force What These People Did Experimental Support 1 Fundamental Forces

More information

Homework 3: Group Theory and the Quark Model Due February 16

Homework 3: Group Theory and the Quark Model Due February 16 Homework 3: Group Theory and the Quark Model Due February 16 1. Lorentz Group. From the defining requirement that a Lorentz transformation implemented by a matrix Λ leave the metric invariant: Λ µ ρη ρσ

More information

DEEP INELASTIC SCATTERING

DEEP INELASTIC SCATTERING DEEP INELASTIC SCATTERING Electron scattering off nucleons (Fig 7.1): 1) Elastic scattering: E = E (θ) 2) Inelastic scattering: No 1-to-1 relationship between E and θ Inelastic scattering: nucleon gets

More information

Particle Physics. All science is either physics or stamp collecting and this from a 1908 Nobel laureate in Chemistry

Particle Physics. All science is either physics or stamp collecting and this from a 1908 Nobel laureate in Chemistry Particle Physics JJ Thompson discovered electrons in 1897 Rutherford discovered the atomic nucleus in 1911 and the proton in 1919 (idea of gold foil expt) All science is either physics or stamp collecting

More information

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

Quantum Numbers. Elementary Particles Properties. F. Di Lodovico c 1 EPP, SPA6306. Queen Mary University of London. Quantum Numbers. F. Elementary Properties 1 1 School of Physics and Astrophysics Queen Mary University of London EPP, SPA6306 Outline Most stable sub-atomic particles are the proton, neutron (nucleons) and electron. Study

More information

Lecture 9 Valence Quark Model of Hadrons

Lecture 9 Valence Quark Model of Hadrons Lecture 9 Valence Quark Model of Hadrons Isospin symmetry SU(3) flavour symmetry Meson & Baryon states Hadronic wavefunctions Masses and magnetic moments Heavy quark states 1 Isospin Symmetry Strong interactions

More information

Option 212: UNIT 2 Elementary Particles

Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy Option 212: UNIT 2 Elementary Particles SCHEDULE 26-Jan-15 13.00pm LRB Intro lecture 28-Jan-15 12.00pm LRB Problem solving (2-Feb-15 10.00am E Problem Workshop) 4-Feb-15

More information

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

Quantum Numbers. F. Di Lodovico 1 EPP, SPA6306. Queen Mary University of London. Quantum Numbers. F. Di Lodovico. Quantum Numbers. 1 1 School of Physics and Astrophysics Queen Mary University of London EPP, SPA6306 Outline : Number Conservation Rules Based on the experimental observation of particle interactions a number of particle

More information

Hadron Physics & Quantum Chromodynamics Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora

Hadron Physics & Quantum Chromodynamics Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora Hadron Physics & Quantum Chromodynamics Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora Hadron Physics & QCD Part 1: First Encounter With Hadrons: Introduction to Mesons & Baryons, The Quark

More information

Lecture PowerPoint. Chapter 32 Physics: Principles with Applications, 6 th edition Giancoli

Lecture PowerPoint. Chapter 32 Physics: Principles with Applications, 6 th edition Giancoli Lecture PowerPoint Chapter 32 Physics: Principles with Applications, 6 th edition Giancoli 2005 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the

More information

The Electro-Strong Interaction

The Electro-Strong Interaction The Electro-Strong Interaction Taking into account the Planck Distribution Law of the electromagnetic oscillators, we can explain the electron/proton mass rate and the Weak and Strong Interactions. Lattice

More information

13. Basic Nuclear Properties

13. Basic Nuclear Properties 13. Basic Nuclear Properties Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 13. Basic Nuclear Properties 1 In this section... Motivation for study The strong nuclear force Stable nuclei Binding

More information

FYS3510 Subatomic Physics. Exam 2016

FYS3510 Subatomic Physics. Exam 2016 FYS3510 Subatomic Physics VS 2015 Farid Ould-Saada Exam 2016 In addition to the items marked in blue, don t forget all examples and related material given in the slides, including the ones presented during

More information

PHYS 3446 Lecture #17

PHYS 3446 Lecture #17 PHY 3446 Lecture #7 Monday, Nov. 6, 26 Dr.. Elementary Particle Properties Quantum Numbers trangeness Isospin Gell-Mann-Nishijima Relations Production and Decay of Resonances Monday, Nov. 6, 26 PHY 3446,

More information

1 Nucleon-Nucleon Scattering

1 Nucleon-Nucleon Scattering Lecture Notes: NN Scattering Keegan Sherman 1 Nucleon-Nucleon Scattering In the previous lecture, we were talking about nucleon-nucleon (NN) scattering events and describing them through phase shifts.

More information

Coupling of Angular Momenta Isospin Nucleon-Nucleon Interaction

Coupling of Angular Momenta Isospin Nucleon-Nucleon Interaction Lecture 5 Coupling of Angular Momenta Isospin Nucleon-Nucleon Interaction WS0/3: Introduction to Nuclear and Particle Physics,, Part I I. Angular Momentum Operator Rotation R(θ): in polar coordinates the

More information

Space-Time Symmetries

Space-Time Symmetries Space-Time Symmetries Outline Translation and rotation Parity Charge Conjugation Positronium T violation J. Brau Physics 661, Space-Time Symmetries 1 Conservation Rules Interaction Conserved quantity strong

More information

The Quark Parton Model

The Quark Parton Model The Quark Parton Model Quark Model Pseudoscalar J P = 0 Mesons Vector J P = 1 Mesons Meson Masses J P = 3 /2 + Baryons J P = ½ + Baryons Resonances Resonance Detection Discovery of the ω meson Dalitz Plots

More information

A Measurement of the Induced polarization of electro-produced Λ(1116) with CLAS

A Measurement of the Induced polarization of electro-produced Λ(1116) with CLAS A Measurement of the Induced polarization of electro-produced Λ(1116) with CLAS Marianna Gabrielyan Florida International University HUGS 2008 Why study electromagnetic production of kaons? Formalism.

More information

Weak interactions, parity, helicity

Weak interactions, parity, helicity Lecture 10 Weak interactions, parity, helicity SS2011: Introduction to Nuclear and Particle Physics, Part 2 2 1 Weak decay of particles The weak interaction is also responsible for the β + -decay of atomic

More information

Physics 4213/5213 Lecture 1

Physics 4213/5213 Lecture 1 August 28, 2002 1 INTRODUCTION 1 Introduction Physics 4213/5213 Lecture 1 There are four known forces: gravity, electricity and magnetism (E&M), the weak force, and the strong force. Each is responsible

More information

Weak interactions and vector bosons

Weak interactions and vector bosons Weak interactions and vector bosons What do we know now about weak interactions? Theory of weak interactions Fermi's theory of weak interactions V-A theory Current - current theory, current algebra W and

More information

Discrete Transformations: Parity

Discrete Transformations: Parity Phy489 Lecture 8 0 Discrete Transformations: Parity Parity operation inverts the sign of all spatial coordinates: Position vector (x, y, z) goes to (-x, -y, -z) (eg P(r) = -r ) Clearly P 2 = I (so eigenvalues

More information

{ } or. ( ) = 1 2 ψ n1. ( ) = ψ r2 n1,n2 (, r! 1 ), under exchange of particle label r! 1. ψ r1 n1,n2. ψ n. ψ ( x 1

{ } or. ( ) = 1 2 ψ n1. ( ) = ψ r2 n1,n2 (, r! 1 ), under exchange of particle label r! 1. ψ r1 n1,n2. ψ n. ψ ( x 1 Practice Modern Physics II, W08, Set 3 Question : Symmetric (Boson) and Anti-symmetric (Fermions) Wavefunction A) Consider a system of two fermions Which of the following wavefunctions can describe the

More information

T 1! p k. = T r! k., s k. ', x' ] = i!, s y. ', s y

T 1! p k. = T r! k., s k. ', x' ] = i!, s y. ', s y Time Reversal r k ' = r k = T r k T 1 p k ' = p k, s k ' = s k T cannot be represented by an unitary operator. Unitary opera$ons preserve algebraic rela$ons between operators, while T changes the sign

More information

Lecture 11 Weak interactions, Cabbibo-angle. angle. SS2011: Introduction to Nuclear and Particle Physics, Part 2

Lecture 11 Weak interactions, Cabbibo-angle. angle. SS2011: Introduction to Nuclear and Particle Physics, Part 2 Lecture 11 Weak interactions, Cabbibo-angle angle SS2011: Introduction to Nuclear and Particle Physics, Part 2 1 Neutrino-lepton reactions Consider the reaction of neutrino-electron scattering: Feynman

More information

Lecture 6 Isospin. What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Gell- Mann- Nishijima formula FK

Lecture 6 Isospin. What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Gell- Mann- Nishijima formula FK Lecture 6 Isospin What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Gell- Mann- Nishijima formula FK7003 08 SU() Isospin Isospin introduced based on the observa4on that: m p =

More information

Kern- und Teilchenphysik II Lecture 1: QCD

Kern- und Teilchenphysik II Lecture 1: QCD Kern- und Teilchenphysik II Lecture 1: QCD (adapted from the Handout of Prof. Mark Thomson) Prof. Nico Serra Dr. Marcin Chrzaszcz Dr. Annapaola De Cosa (guest lecturer) www.physik.uzh.ch/de/lehre/phy213/fs2017.html

More information

Introductory Nuclear Physics. Glatzmaier and Krumholz 7 Prialnik 4 Pols 6 Clayton 4.1, 4.4

Introductory Nuclear Physics. Glatzmaier and Krumholz 7 Prialnik 4 Pols 6 Clayton 4.1, 4.4 Introductory Nuclear Physics Glatzmaier and Krumholz 7 Prialnik 4 Pols 6 Clayton 4.1, 4.4 Each nucleus is a bound collection of N neutrons and Z protons. The mass number is A = N + Z, the atomic number

More information

Invariance Principles and Conservation Laws

Invariance Principles and Conservation Laws Invariance Principles and Conservation Laws Outline Translation and rotation Parity Charge Conjugation Charge Conservation and Gauge Invariance Baryon and lepton conservation CPT Theorem CP violation and

More information

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

Visit   for more fantastic resources. AQA. A Level. A Level Physics. Particles (Answers) Name: Total Marks: /30 Visit http://www.mathsmadeeasy.co.uk/ for more fantastic resources. AQA A Level A Level Physics Particles (Answers) Name: Total Marks: /30 Maths Made Easy Complete Tuition Ltd 2017 1. This question explores

More information

SECOND PUBLIC EXAMINATION. Honour School of Physics Part C: 4 Year Course. Honour School of Physics and Philosophy Part C C4: PARTICLE PHYSICS

SECOND PUBLIC EXAMINATION. Honour School of Physics Part C: 4 Year Course. Honour School of Physics and Philosophy Part C C4: PARTICLE PHYSICS 754 SECOND PUBLIC EXAMINATION Honour School of Physics Part C: 4 Year Course Honour School of Physics and Philosophy Part C C4: PARTICLE PHYSICS TRINITY TERM 04 Thursday, 9 June,.30 pm 5.45 pm 5 minutes

More information

Introduction to particle physics Lecture 4

Introduction to particle physics Lecture 4 Introduction to particle physics Lecture 4 Frank Krauss IPPP Durham U Durham, Epiphany term 2009 Outline 1 Mesons and Isospin 2 Strange particles 3 Resonances 4 The quark model Nuclei, nucleons, and mesons

More information

A.A. Godizov. Institute for High Energy Physics, Protvino, Russia

A.A. Godizov. Institute for High Energy Physics, Protvino, Russia arxiv:1410.886v1 [hep-ph] 0 Oct 2014 QCD and nuclear physics. How to explain the coincidence between the radius of the strong interaction of nucleons and the characteristic scale of neutron-neutron electrostatic

More information

1. (a) An ion of plutonium Pu has an overall charge of C. (iii) electrons... (3) (2) (Total 5 marks)

1. (a) An ion of plutonium Pu has an overall charge of C. (iii) electrons... (3) (2) (Total 5 marks) AQA Questions from 2004 to 2006 Particle Physics 239 94 1. (a) An ion of plutonium Pu has an overall charge of +1.6 10 19 C. For this ion state the number of (i) protons... neutrons... (iii) electrons...

More information

Modern Physics: Standard Model of Particle Physics (Invited Lecture)

Modern Physics: Standard Model of Particle Physics (Invited Lecture) 261352 Modern Physics: Standard Model of Particle Physics (Invited Lecture) Pichet Vanichchapongjaroen The Institute for Fundamental Study, Naresuan University 1 Informations Lecturer Pichet Vanichchapongjaroen

More information

Kern- und Teilchenphysik I Lecture 13:Quarks and QCD

Kern- und Teilchenphysik I Lecture 13:Quarks and QCD Kern- und Teilchenphysik I Lecture 13:Quarks and QCD (adapted from the Handout of Prof. Mark Thomson) Prof. Nico Serra Dr. Patrick Owen, Dr. Silva Coutinho http://www.physik.uzh.ch/de/lehre/phy211/hs2016.html

More information

SU(3) symmetry and Baryon wave functions

SU(3) symmetry and Baryon wave functions INTERNATIONAL PHD PROJECTS IN APPLIED NUCLEAR PHYSICS AND INNOVATIVE TECHNOLOGIES This project is supported by the Foundation for Polish Science MPD program, co-financed by the European Union within the

More information

PhysicsAndMathsTutor.com 1

PhysicsAndMathsTutor.com 1 Q1. (a) The K meson has strangeness 1. State the quark composition of a meson... State the baryon number of the K meson... (iii) What is the quark composition of the K meson?.... The figure below shows

More information

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

Isospin. K.K. Gan L5: Isospin and Parity 1 Isospin Isospin is a continuous symmetry invented by Heisenberg: Explain the observation that the strong interaction does not distinguish between neutron and proton. Example: the mass difference between

More information

Properties of the proton and neutron in the quark model

Properties of the proton and neutron in the quark model Properties of the proton and neutron in the quark model A good way to introduce the ideas encoded in the quark model is to understand how it simply explains properties of the ground-state baryons and mesons

More information

CHAPTER 7 TEST REVIEW

CHAPTER 7 TEST REVIEW IB PHYSICS Name: Period: Date: # Marks: 94 Raw Score: IB Curve: DEVIL PHYSICS BADDEST CLASS ON CAMPUS CHAPTER 7 TEST REVIEW 1. An alpha particle is accelerated through a potential difference of 10 kv.

More information

M. Cobal, PIF 2006/7. Quarks

M. Cobal, PIF 2006/7. Quarks M. Cobal, PIF 2006/7 Quarks Quarks Quarks are s = ½ fermions, subject to all kind of interactions. They have fractional electric charges Quarks and their bound states are the only particles which interact

More information

L. David Roper

L. David Roper The Heavy Proton L. David Roper mailto:roperld@vt.edu Introduction The proton is the nucleus of the hydrogen atom, which has one orbiting electron. The proton is the least massive of the baryons. Its mass

More information

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

Contents. Preface to the First Edition Preface to the Second Edition Contents Preface to the First Edition Preface to the Second Edition Notes xiii xv xvii 1 Basic Concepts 1 1.1 History 1 1.1.1 The Origins of Nuclear Physics 1 1.1.2 The Emergence of Particle Physics: the

More information

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

Most of Modern Physics today is concerned with the extremes of matter: Most of Modern Physics today is concerned with the extremes of matter: Very low temperatures, very large numbers of particles, complex systems Æ Condensed Matter Physics Very high temperatures, very large

More information

cgrahamphysics.com Particles that mediate force Book pg Exchange particles

cgrahamphysics.com Particles that mediate force Book pg Exchange particles Particles that mediate force Book pg 299-300 Exchange particles Review Baryon number B Total # of baryons must remain constant All baryons have the same number B = 1 (p, n, Λ, Σ, Ξ) All non baryons (leptons

More information

FYS3510 Subatomic Physics. Exam 2016

FYS3510 Subatomic Physics. Exam 2016 FYS3510 Subatomic Physics VS 2015 Farid Ould-Saada Exam 2016 In addition to the items marked in blue, don t forget all examples and related material given in the slides, including the ones presented during

More information

M. Cobal, PIF 2006/7. Quarks

M. Cobal, PIF 2006/7. Quarks Quarks Quarks Quarks are s = ½ fermions, subject to all kind of interactions. They have fractional electric charges Quarks and their bound states are the only particles which interact strongly Like leptons,

More information

Chapter 5. Par+cle Physics

Chapter 5. Par+cle Physics Chapter 5 Par+cle Physics Types of Forces Force Range (m) Relative Strength Force Carrier Gravitational! 10-38 Graviton Weak 10-18 10-5 W ±, Z 0 Electromagnetic! =1/137 Photon Strong 10-15 1 Gluon What

More information

Concepts of Event Reconstruction

Concepts of Event Reconstruction August 3, 2007 Directly Detectable Particles electrons, positrons: e ±, lightest charged lepton photons: γ, gauge boson for electromagnetic force pions: π ±, lightest mesons kaons: K ±, K L, lightest strange

More information

Essential Physics II. Lecture 14:

Essential Physics II. Lecture 14: Essential Physics II E II Lecture 14: 18-01-16 Last lecture of EP2! Congratulations! This was a hard course. Be proud! Next week s exam Next Monday! All lecture slides on course website: http://astro3.sci.hokudai.ac.jp/~tasker/teaching/ep2

More information

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

Most of Modern Physics today is concerned with the extremes of matter: Most of Modern Physics today is concerned with the extremes of matter: Very low temperatures, very large numbers of particles, complex systems Æ Condensed Matter Physics Very high temperatures, very large

More information

129 Lecture Notes More on Dirac Equation

129 Lecture Notes More on Dirac Equation 19 Lecture Notes More on Dirac Equation 1 Ultra-relativistic Limit We have solved the Diraction in the Lecture Notes on Relativistic Quantum Mechanics, and saw that the upper lower two components are large

More information

1. What does this poster contain?

1. What does this poster contain? This poster presents the elementary constituents of matter (the particles) and their interactions, the latter having other particles as intermediaries. These elementary particles are point-like and have

More information

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

Books: - Martin, B.R. & Shaw, G Particle Physics (Wiley) (recommended) - Perkins, D.H. Introduction to High Energy Physics (CUP) (advanced) PC 3 Foundations of Particle Physics Lecturer: Dr F. Loebinger Books: - Martin, B.R. & Shaw, G Particle Physics (Wiley) (recommended) - Perkins, D.H. Introduction to High Energy Physics (CUP) (advanced)

More information

Lecture 11 Krane Enge Cohen Williams. Beta decay` Ch 9 Ch 11 Ch /4

Lecture 11 Krane Enge Cohen Williams. Beta decay` Ch 9 Ch 11 Ch /4 Lecture 11 Krane Enge Cohen Williams Isospin 11.3 6.7 6.3 8.10 Beta decay` Ch 9 Ch 11 Ch 11 5.3/4 Problems Lecture 11 1 Discuss the experimental evidence for the existence of the neutrino. 2 The nuclide

More information

NATIONAL OPEN UNIVERSITY OF NIGERIA

NATIONAL OPEN UNIVERSITY OF NIGERIA NATIONAL OPEN UNIVERSITY OF NIGERIA SCHOOL OF SCIENCE AND TECHNOLOGY COURSE CODE: PHY 409 COURSE TITLE: ELEMENTARY PARTICLE PHYSICS Course Title Course Developer Course Code PHY 409 ELEMENTARY PARTICLE

More information

The Standard Model. 1 st 2 nd 3 rd Describes 3 of the 4 known fundamental forces. Separates particle into categories

The Standard Model. 1 st 2 nd 3 rd Describes 3 of the 4 known fundamental forces. Separates particle into categories The Standard Model 1 st 2 nd 3 rd Describes 3 of the 4 known fundamental forces. Separates particle into categories Bosons (force carriers) Photon, W, Z, gluon, Higgs Fermions (matter particles) 3 generations

More information

3 Dimensional String Theory

3 Dimensional String Theory 3 Dimensional String Theory New ideas for interactions and particles Abstract...1 Asymmetry in the interference occurrences of oscillators...1 Spontaneously broken symmetry in the Planck distribution law...3

More information

Lecture 6 Isospin. What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Heavier quarks FK

Lecture 6 Isospin. What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Heavier quarks FK Lecture 6 Isospin What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Heavier quarks FK7003 33 SU() Isospin Isospin introduced based on the observa4on that: m p = 0.9383 GeV and

More information

Hadron Spectroscopy Lecture 1 Introduction and Motivation

Hadron Spectroscopy Lecture 1 Introduction and Motivation Hadron Spectroscopy Lecture 1 Introduction and Motivation National Nuclear Physics Summer School at MIT Matthew Shepherd Indiana University Outline 1. Overview and Motivation 1.1.Uniue features of QCD

More information

hybrids (mesons and baryons) JLab Advanced Study Institute

hybrids (mesons and baryons) JLab Advanced Study Institute hybrids (mesons and baryons) 2000 2000 1500 1500 1000 1000 500 500 0 0 71 the resonance spectrum of QCD or, where are you hiding the scattering amplitudes? real QCD real QCD has very few stable particles

More information

Problem Set # 4 SOLUTIONS

Problem Set # 4 SOLUTIONS Wissink P40 Subatomic Physics I Fall 007 Problem Set # 4 SOLUTIONS 1. Gee! Parity is Tough! In lecture, we examined the operator that rotates a system by 180 about the -axis in isospin space. This operator,

More information

NUCLEAR FORCES. Historical perspective

NUCLEAR FORCES. Historical perspective NUCLEAR FORCES Figure 1: The atomic nucleus made up from protons (yellow) and neutrons (blue) and held together by nuclear forces. Nuclear forces (also known as nuclear interactions or strong forces) are

More information

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

Elementary Particle Physics Glossary. Course organiser: Dr Marcella Bona February 9, 2016 Elementary Particle Physics Glossary Course organiser: Dr Marcella Bona February 9, 2016 1 Contents 1 Terms A-C 5 1.1 Accelerator.............................. 5 1.2 Annihilation..............................

More information

Particle Physics. Michaelmas Term 2009 Prof Mark Thomson. Handout 7 : Symmetries and the Quark Model. Introduction/Aims

Particle Physics. Michaelmas Term 2009 Prof Mark Thomson. Handout 7 : Symmetries and the Quark Model. Introduction/Aims Particle Physics Michaelmas Term 2009 Prof Mark Thomson Handout 7 : Symmetries and the Quark Model Prof. M.A. Thomson Michaelmas 2009 205 Introduction/Aims Symmetries play a central role in particle physics;

More information

Discovery of Pions and Kaons in Cosmic Rays in 1947

Discovery of Pions and Kaons in Cosmic Rays in 1947 Discovery of Pions and Kaons in Cosmic Rays in 947 π + µ + e + (cosmic rays) Points to note: de/dx Bragg Peak Low de/dx for fast e + Constant range (~600µm) (i.e. -body decay) small angle scattering Strange

More information

Hadron Spectroscopy at COMPASS

Hadron Spectroscopy at COMPASS Hadron Spectroscopy at Overview and Analysis Methods Boris Grube for the Collaboration Physik-Department E18 Technische Universität München, Garching, Germany Future Directions in Spectroscopy Analysis

More information

Introduction to Modern Physics Problems from previous Exams 3

Introduction to Modern Physics Problems from previous Exams 3 Introduction to Modern Physics Problems from previous Exams 3 2007 An electron of mass 9 10 31 kg moves along the x axis at a velocity.9c. a. Calculate the rest energy of the electron. b. Calculate its

More information

The Uncertainty Principle and the Quarks

The Uncertainty Principle and the Quarks The Uncertainty Principle and the Quarks Andrei Gritsan Johns Hopkins University August, 2007 JHU Quarknet Meeting Outline The Uncertainty Principle quantum mechanics with elementary particles The Quarks

More information

Introduction to Quantum Chromodynamics (QCD)

Introduction to Quantum Chromodynamics (QCD) Introduction to Quantum Chromodynamics (QCD) Jianwei Qiu Theory Center, Jefferson Lab May 29 June 15, 2018 Lecture One The plan for my four lectures q The Goal: To understand the strong interaction dynamics

More information

Lecture 01. Introduction to Elementary Particle Physics

Lecture 01. Introduction to Elementary Particle Physics Introduction to Elementary Particle Physics Particle Astrophysics Particle physics Fundamental constituents of nature Most basic building blocks Describe all particles and interactions Shortest length

More information

Reminder about invariant mass:

Reminder about invariant mass: Phy489 Lecture 6 Reminder about invariant mass: A system of n particles has a mass defined by M INV c = P TOT P TOT where is the total four momentum of the system P TOT = p 1 + p + p 3 +... + p n P TOT

More information

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

FYS 3510 Subatomic physics with applications in astrophysics. Nuclear and Particle Physics: An Introduction FYS 3510 Subatomic physics with applications in astrophysics Nuclear and Particle Physics: An Introduction Nuclear and Particle Physics: An Introduction, 2nd Edition Professor Brian Martin ISBN: 978-0-470-74275-4

More information

Neutrino Physics. Kam-Biu Luk. Tsinghua University and University of California, Berkeley and Lawrence Berkeley National Laboratory

Neutrino Physics. Kam-Biu Luk. Tsinghua University and University of California, Berkeley and Lawrence Berkeley National Laboratory Neutrino Physics Kam-Biu Luk Tsinghua University and University of California, Berkeley and Lawrence Berkeley National Laboratory 4-15 June, 2007 Outline Brief overview of particle physics Properties of

More information