Fundamental Forces. David Morrissey. Key Concepts, March 15, 2013

Size: px
Start display at page:

Download "Fundamental Forces. David Morrissey. Key Concepts, March 15, 2013"

Transcription

1 Fundamental Forces David Morrissey Key Concepts, March 15, 2013

2 Not a fundamental force...

3 Also not a fundamental force...

4 What Do We Mean By Fundamental? Example: Electromagnetism (EM) electric forces magnetic forces Van der Waals forces radio waves rainbows... These different phenomena are all manifestations of EM. EM is said to be a fundamental force.

5 The Four Fundamental Forces * 1. Electromagnetism (EM) binds atoms, light, shocks 2. Strong holds nuclei together 3. Weak source of nuclear decays 4. Gravity why you re sitting here * Force = way for particles to interact

6 Four Fundamental Forces * 1. Electromagnetism (EM) binds atoms, light, shocks 2. Strong holds nuclei together 3. Weak source of nuclear decays 4. Gravity why you re sitting here The Cold Hard Truth: These forces might not actually be fundamental. There may be more (or less) than four. * Force = way for particles to interact

7 How Do We Measure Forces? 1. Pull two particles apart: how much energy V(r) does this take? Need really good tweezers Scatter particles: Stronger Force Weaker Force Stronger Force More Scattering

8 Forces and Scattering dσ d(cosθ) (p 1,p 2 ) = differential scattering cross-section = prob. for particles to scatter with angle θ A 2 A is the quantum mechanical amplitude. p 1, p 2 are the initial momenta of the particles. p 1 p 1 θ p 2 p 2

9 For non-relativistic scattering, A d 3 x e i q x V( x) Ṽ( q) where q = ( p p ) is the momentum transfer. Ṽ( q) is the Fourier Transform of the potential. Also: V( x) = d 3 q (2π) 3e i q x Ṽ( q). Scattering experiments teach us about forces!

10 Electromagnetism (Relativistic) Scattering experiments yield A Ṽ(p) = Q 1Q 2 e 2 p 2, where p = (E, p) is the transferred 4-momentum, (Q 1 e) and (Q 2 e) are the electric charges of the particles. Fourier transforming (in the non-relativistic limit) gives V( x) = Q 1Q 2 e 2 4π 1 r. Science works (...)!

11 In relativistic quantum mechanics, A = 1 p 2 m 2, p2 = E 2 p 2 is the amplitude for a particle of mass m to propagate with momentum p. Interpret the electromagnetic force as being mediated by a massless particle - the photon. e e γ e e The photon travels at the speed of light. In fact, the photon is a particle of light (or EM radiation).

12 Feynman Diagram electron scattering: e e γ e e Feynman Diagram Compton scattering: γ γ e e e

13 Electromagnetism has a U(1) em gauge symmetry. The Hamiltonian for EM is invariant under: ψ(x) e iqα ψ(x) (charged particle wavefnctn) φ(x) φ(x) 1 α (scalar EM potential) e t A(x) A(x) 1 α (vector EM potential) e for any function α(x). This symmetry COMPLETELY fixes how the photon couples to charged matter. all of electromagnetism follows from this simple gauge symmetry principle!

14 Aside: General Structure of Ṽ(p) We ll see that Ṽ(p) has the same general structure for all forces we will look at: Ṽ(p) = g 2 S 1 p 2 m 2 Here, g = dimensionless coupling strength of the force S = dependence on particle spins 1 p 2 m 2 = propagation of the force mediator I won t say much at all about S today.

15 The Strong Force Binds quarks into baryons and mesons, holds nuclei together. baryon = qqq bound state e.g. p = (uud), n = (udd) meson = q q bound state e.g. π 0 = (uū, d d), K + = (u s) A ZX nucleus = [Zp + (A-Z)n] bound state e.g. 4 2 He = 2p+2n, 16 8 O = 8p+8n Of the elementary particles we have discovered, only quarks and gluons feel the strong force.

16 Elementary Particles of the Standard Model: Fermions Bosons u c t γ d s b g ν e e ν µ ν µ τ τ W Z + 0 h

17 In stuffed toy form:

18 Scattering experiments tell us that: Ṽ(p) = g 2 s (p2 ) p 2, p 2 GeV 2, quark scattering gnnπ 2 p 2 m 2, p 2 GeV 2, nucleon scattering π Why do we think both come from the same basic force? Why don t we see quarks at low energies?

19 Start with quark scattering (p GeV): Ṽ(p) g2 s p 2 1/p 2 massless mediator the gluon. g s describes the strength of the strong force. It depends on p : g s 1 GeV At p 1GeV the coupling blows up! This confines quarks and gluons into baryons and mesons: V( x) 1 r +Λ2 r, Λ GeV fm 1. p

20 At lower energies, look at nucleon scattering (p GeV) Ṽ(p) = g2 NNπ p 2 m 2 π The force is mediated (mostly) by pions. g NNπ is the residue of the strong force after confinement. (Like van der Waals forces between neutral atoms.) N N π N N

21 Fourier transforming Ṽ(p) gives V( x) = g2 Nππ 4π 1 r e m πr Yukawa force with range r 1/m π 1fm. This is the typical separation between nucleons in nuclei! (Yukawa proposed the pion based on the range of the force.)

22 The strong force is based on a SU(3) c gauge symmetry. U(1) = 1 1 unitary matrices = phase transformations. SU(N) = N N unitary matrices with (determinant = 1). SU(3) c interchanges the 3 colour charges carried by quarks. strong force = quantum chromodynamics = QCD This symmetry COMPLETELY fixes the strong force! Gluons also carry colour charge. (Photons have no EM charge.)

23 The Weak Force Allows decays forbidden by the EM and strong forces: n p ν e e π ν µ µ b c ν e e µ ν µ ν e e (d u ν e e at the quark level) (dū ν µ µ at the quark level) These decays are very slow compared to EM or strong, but they are the only ones that mix flavours. The weak force is much more interesting above 100GeV.

24 At lower energies, p 100GeV, scattering gives Ṽ(p) constant G F g2 w m 2 W with g w 0.6, m W 80GeV. Fourier transforming gives V( x) G F δ (3) ( x) zero range point interaction

25 The party starts at higher energies, p 100GeV: Ṽ(p) g 2 w p 2 m 2 W, g 2 w p 2 m 2 Z with g w 0.65, m W 80.4GeV, m Z 91.2GeV. For p m W this reduces to what we had before. Looks like a force mediated by particles with masses m W, m Z. W, Z W ± and Z 0 spin 1 bosons were discovered in the 1980 s.

26

27 Electroweak Unification A gauge symmetry principle joins the weak and EM forces into a single electroweak force. The symmetry group is SU(2) L U(1) Y, contains U(1) em. Most of this symmetry is hidden at low energies. Only the U(1) em subgroup of EM remains unhidden. Hiding the symmetry means: W ± and Z 0 gauge bosons acquire masses the weak force has a finite range m 1 W the weak force is much weaker than EM for p m W

28 SU(2) L U(1) Y has coupling constants g and g. They are related to g w and e by g w = g, e = gg / g 2 +g 2. A spin 0 Higgs boson particle is thought to induce this electroweak symmetry breaking. We re trying really hard to find it, but no luck so far.

29 More Forces, and not so Fundamental The Higgs is also thought to generate fermion masses. If it does, there are also new Higgs forces. For scattering of two fermions with masses m 1 and m 2, Ṽ(p) = (m 1m 2 /v 2 ) p 2 m 2 h with m h 100GeV and v = 174GeV. This is a new Yukawa-type force: V( x) = (m 1m 2 /v 2 ) 4π 1 r e m hr. The coupling strength to a fermion of mass m is m/v.

30 Strong and Electroweak Couplings: g s > g > g. This is at p 100GeV. (g s 1, g 0.65, g 0.35) All three couplings depend on the scattering energy: g s decreases going to higher energies g, g increase going to higher energies Does the strong force get weaker than the weak force? Maybe depends on what new physics is around.

31 With no new physics (except maybe a little supersymmetry): g s g? g 1 GeV 10 GeV It looks like the couplings all meet at a point! Maybe the strong and EW forces have a common origin? 16 p SU(3) c SU(2) L U(1) Y SU(5), SO(10), E 6,... gauge unification into a single force with coupling g U? Symmetry breaking would split them into components.

32 Gravity Much weaker than the other three fundamental forces. almost always negligible in laboratory experiments Scattering of masses m 1 and m 2 gives (p M Pl ) Ṽ(p) m 1m 2 M 2 Pl 1 p 2, with M Pl GeV = 1/ 8πG N. This gives Yay! V( x) = G Nm 1 m 2 r

33 Interpret gravity as being mediated by a graviton. massless spin 2 particle The graviton coupling strength to matter is m/m Pl. Graviton couplings are fixed by a gauge symmetry. Symmetry Group = Local Coordinate Transformations x x (x) This reproduces General Relativity at the classical level. We don t know what gravity does at energies above M Pl, where quantum corrections become important.

34 Summary Fundamental Forces The 4FF are all based on gauge symmetries. But we think there are more forces out there. And the fundamental forces might not be fundamental. We hope to learn much more at the LHC!

35

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

Overview. The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions. Overview The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions. Our understanding is about to take a giant leap.. the Large Hadron Collider

More information

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

1 Introduction. 1.1 The Standard Model of particle physics The fundamental particles 1 Introduction The purpose of this chapter is to provide a brief introduction to the Standard Model of particle physics. In particular, it gives an overview of the fundamental particles and the relationship

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

FUNDAMENTAL PARTICLES CLASSIFICATION! BOSONS! QUARKS! FERMIONS! Gauge Bosons! Fermions! Strange and Charm! Top and Bottom! Up and Down!

FUNDAMENTAL PARTICLES CLASSIFICATION! BOSONS! QUARKS! FERMIONS! Gauge Bosons! Fermions! Strange and Charm! Top and Bottom! Up and Down! FUNDAMENTAL PARTICLES CLASSIFICATION! BOSONS! --Bosons are generally associated with radiation and are sometimes! characterized as force carrier particles.! Quarks! Fermions! Leptons! (protons, neutrons)!

More information

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

FACULTY OF SCIENCE. High Energy Physics. WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON FACULTY OF SCIENCE High Energy Physics WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON AIM: To explore nature on the smallest length scales we can achieve Current status (10-20 m)

More information

Particle Physics Lectures Outline

Particle Physics Lectures Outline Subatomic Physics: Particle Physics Lectures Physics of the Large Hadron Collider (plus something about neutrino physics) 1 Particle Physics Lectures Outline 1 - Introduction The Standard Model of particle

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

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

Cosmology and particle physics

Cosmology and particle physics Cosmology and particle physics Lecture notes Timm Wrase Lecture 5 The thermal universe - part I In the last lecture we have shown that our very early universe was in a very hot and dense state. During

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

INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS

INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS Class Mechanics My office (for now): Dantziger B Room 121 My Phone: x85200 Office hours: Call ahead, or better yet, email... Even better than office

More information

Particle Physics Lecture 1 : Introduction Fall 2015 Seon-Hee Seo

Particle Physics Lecture 1 : Introduction Fall 2015 Seon-Hee Seo Particle Physics Lecture 1 : Introduction Fall 2015 Seon-Hee Seo Particle Physics Fall 2015 1 Course Overview Lecture 1: Introduction, Decay Rates and Cross Sections Lecture 2: The Dirac Equation and Spin

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

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

A first trip to the world of particle physics

A first trip to the world of particle physics A first trip to the world of particle physics Itinerary Massimo Passera Padova - 13/03/2013 1 Massimo Passera Padova - 13/03/2013 2 The 4 fundamental interactions! Electromagnetic! Weak! Strong! Gravitational

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

Photon Coupling with Matter, u R

Photon Coupling with Matter, u R 1 / 16 Photon Coupling with Matter, u R Consider the up quark. We know that the u R has electric charge 2 3 e (where e is the proton charge), and that the photon A is a linear combination of the B and

More information

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

9.2.E - Particle Physics. Year 12 Physics 9.8 Quanta to Quarks + 9.2.E - Particle Physics Year 12 Physics 9.8 Quanta to Quarks + Atomic Size n While an atom is tiny, the nucleus is ten thousand times smaller than the atom and the quarks and electrons are at least

More information

Chapter 32 Lecture Notes

Chapter 32 Lecture Notes Chapter 32 Lecture Notes Physics 2424 - Strauss Formulas: mc 2 hc/2πd 1. INTRODUCTION What are the most fundamental particles and what are the most fundamental forces that make up the universe? For a brick

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

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

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

1. Introduction. Particle and Nuclear Physics. Dr. Tina Potter. Dr. Tina Potter 1. Introduction 1

1. Introduction. Particle and Nuclear Physics. Dr. Tina Potter. Dr. Tina Potter 1. Introduction 1 1. Introduction Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 1. Introduction 1 In this section... Course content Practical information Matter Forces Dr. Tina Potter 1. Introduction 2 Course

More information

Fundamental Particles and Forces

Fundamental Particles and Forces Fundamental Particles and Forces A Look at the Standard Model and Interesting Theories André Gras PHYS 3305 SMU 1 Overview Introduction to Fundamental Particles and Forces Brief History of Discovery The

More information

Particles in the Early Universe

Particles in the Early Universe Particles in the Early Universe David Morrissey Saturday Morning Physics, October 16, 2010 Using Little Stuff to Explain Big Stuff David Morrissey Saturday Morning Physics, October 16, 2010 Can we explain

More information

The God particle at last? Astronomy Ireland, Oct 8 th, 2012

The God particle at last? Astronomy Ireland, Oct 8 th, 2012 The God particle at last? Astronomy Ireland, Oct 8 th, 2012 Cormac O Raifeartaigh Waterford Institute of Technology CERN July 4 th 2012 (ATLAS and CMS ) A new particle of mass 125 GeV I The Higgs boson

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

Fundamental Interactions (Forces) of Nature

Fundamental Interactions (Forces) of Nature Chapter 14 Fundamental Interactions (Forces) of Nature Interaction Gauge Boson Gauge Boson Mass Interaction Range (Force carrier) Strong Gluon 0 short-range (a few fm) Weak W ±, Z M W = 80.4 GeV/c 2 short-range

More information

PH5211: High Energy Physics. Prafulla Kumar Behera Room: HSB-304B

PH5211: High Energy Physics. Prafulla Kumar Behera Room: HSB-304B PH5211: High Energy Physics Prafulla Kumar Behera E-mail:behera@iitm.ac.in Room: HSB-304B Information Class timing: Wed. 11am, Thur. 9am, Fri. 8am The course will be graded as follows: 1 st quiz (20 marks)

More information

Particle Physics. Tommy Ohlsson. Theoretical Particle Physics, Department of Physics, KTH Royal Institute of Technology, Stockholm, Sweden

Particle Physics. Tommy Ohlsson. Theoretical Particle Physics, Department of Physics, KTH Royal Institute of Technology, Stockholm, Sweden Particle Physics Tommy Ohlsson Theoretical Particle Physics, Department of Physics, KTH Royal Institute of Technology, Stockholm, Sweden International Baccalaureate T. Ohlsson (KTH) Particle Physics 1/

More information

Quantum Field Theory 2 nd Edition

Quantum Field Theory 2 nd Edition Quantum Field Theory 2 nd Edition FRANZ MANDL and GRAHAM SHAW School of Physics & Astromony, The University of Manchester, Manchester, UK WILEY A John Wiley and Sons, Ltd., Publication Contents Preface

More information

4. The Standard Model

4. The Standard Model 4. The Standard Model Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 4. The Standard Model 1 In this section... Standard Model particle content Klein-Gordon equation Antimatter Interaction

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

Quark model. Jan 30, 2006 Lecture 8 1

Quark model. Jan 30, 2006 Lecture 8 1 Quark model Jan 30, 2006 Lecture 8 1 Quark model of hadrons!!!! Developed long before QCD was recognized as the appropriate quantum field theory of the strong interactions Postulate that 1.! All baryons

More information

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS LSN 7-3: THE STRUCTURE OF MATTER Questions From Reading Activity? Essential Idea: It is believed that all the matter around us is made up of fundamental

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

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

The God particle at last? Science Week, Nov 15 th, 2012

The God particle at last? Science Week, Nov 15 th, 2012 The God particle at last? Science Week, Nov 15 th, 2012 Cormac O Raifeartaigh Waterford Institute of Technology CERN July 4 th 2012 (ATLAS and CMS ) A new particle of mass 125 GeV Why is the Higgs particle

More information

The Scale-Symmetric Theory as the Origin of the Standard Model

The Scale-Symmetric Theory as the Origin of the Standard Model Copyright 2017 by Sylwester Kornowski All rights reserved The Scale-Symmetric Theory as the Origin of the Standard Model Sylwester Kornowski Abstract: Here we showed that the Scale-Symmetric Theory (SST)

More information

The Physics of Particles and Forces David Wilson

The Physics of Particles and Forces David Wilson The Physics of Particles and Forces David Wilson Particle Physics Masterclass 21st March 2018 Overview David Wilson (TCD) Particles & Forces 2/30 Overview of Hadron Spectrum Collaboration (HadSpec) scattering

More information

Astronomy, Astrophysics, and Cosmology

Astronomy, Astrophysics, and Cosmology Astronomy, Astrophysics, and Cosmology Luis A. Anchordoqui Department of Physics and Astronomy Lehman College, City University of New York Lesson IX April 12, 2016 arxiv:0706.1988 L. A. Anchordoqui (CUNY)

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

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

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

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

Particle Physics. Dr Victoria Martin, Spring Semester 2012 Lecture 1: The Mysteries of Particle Physics, or Why should I take this course?

Particle Physics. Dr Victoria Martin, Spring Semester 2012 Lecture 1: The Mysteries of Particle Physics, or Why should I take this course? Particle Physics Dr Victoria Martin, Spring Semester 2012 Lecture 1: The Mysteries of Particle Physics, or Why should I take this course? Contents: Review of the Standard Model! What we know! What we don

More information

Mass. Chris Quigg Fermi National Accelerator Laboratory

Mass. Chris Quigg Fermi National Accelerator Laboratory Mass Chris Quigg Fermi National Accelerator Laboratory YITP@40 Stony Brook 4 May 2007 I. Newton (1687) Mass: the quantity of matter arising from its density and bulk conjointly F = ma + Universal Gravitation

More information

Physics 7730: Particle Physics

Physics 7730: Particle Physics Physics 7730: Particle Physics! Instructor: Kevin Stenson (particle physics experimentalist)! Office: Duane F317 (Gamow tower)! Email: kevin.stenson@colorado.edu! Phone: 303-492-1106! Web page: http://www-hep.colorado.edu/~stenson/!

More information

Introduction to Elementary Particles

Introduction to Elementary Particles David Criffiths Introduction to Elementary Particles Second, Revised Edition WILEY- VCH WILEY-VCH Verlag GmbH & Co. KGaA Preface to the First Edition IX Preface to the Second Edition XI Formulas and Constants

More information

STANDARD MODEL and BEYOND: SUCCESSES and FAILURES of QFT. (Two lectures)

STANDARD MODEL and BEYOND: SUCCESSES and FAILURES of QFT. (Two lectures) STANDARD MODEL and BEYOND: SUCCESSES and FAILURES of QFT (Two lectures) Lecture 1: Mass scales in particle physics - naturalness in QFT Lecture 2: Renormalisable or non-renormalisable effective electroweak

More information

Electroweak Physics. Krishna S. Kumar. University of Massachusetts, Amherst

Electroweak Physics. Krishna S. Kumar. University of Massachusetts, Amherst Electroweak Physics Krishna S. Kumar University of Massachusetts, Amherst Acknowledgements: M. Grunewald, C. Horowitz, W. Marciano, C. Quigg, M. Ramsey-Musolf, www.particleadventure.org Electroweak Physics

More information

IX. Electroweak unification

IX. Electroweak unification IX. Electroweak unification The problem of divergence A theory of weak interactions only by means of W ± bosons leads to infinities e + e - γ W - W + e + W + ν e ν µ e - W - µ + µ Divergent integrals Figure

More information

Beyond Standard Models Higgsless Models. Zahra Sheikhbahaee

Beyond Standard Models Higgsless Models. Zahra Sheikhbahaee Beyond Standard Models Higgsless Models Zahra Sheikhbahaee Standard Model There are three basic forces in the Universe: 1. Electroweak force, including electromagnetic force, 2. Strong nuclear force, 3.

More information

AN OVERVIEW OF QUANTUM CHROMODYNAMICS UNIVERSITY OF WASHINGTON PHYS575 FARRAH TAN 12/10/2015

AN OVERVIEW OF QUANTUM CHROMODYNAMICS UNIVERSITY OF WASHINGTON PHYS575 FARRAH TAN 12/10/2015 AN OVERVIEW OF QUANTUM CHROMODYNAMICS UNIVERSITY OF WASHINGTON PHYS575 FARRAH TAN 12/10/2015 1 AGENDA SOME DEFINITIONS (QCD, FUNDAMENTAL FORCES) SOME HISTORY (THEORY, SLAC) GAUGE THEORY FLAVORS AND COLORS

More information

PHY-105: Introduction to Particle and Nuclear Physics

PHY-105: Introduction to Particle and Nuclear Physics M. Kruse, Spring 2011, Phy-105 PHY-105: Introduction to Particle and Nuclear Physics Up to 1900 indivisable atoms Early 20th century electrons, protons, neutrons Around 1945, other particles discovered.

More information

Remainder of Course. 4/22 Standard Model; Strong Interaction 4/24 Standard Model; Weak Interaction 4/27 Course review 5/01 Final Exam, 3:30 5:30 PM

Remainder of Course. 4/22 Standard Model; Strong Interaction 4/24 Standard Model; Weak Interaction 4/27 Course review 5/01 Final Exam, 3:30 5:30 PM Remainder of Course 4/22 Standard Model; Strong Interaction 4/24 Standard Model; Weak Interaction 4/27 Course review 5/01 Final Exam, 3:30 5:30 PM Practice Final on Course Web Page See HW #12 (not to be

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

Elementary particles and typical scales in high energy physics

Elementary particles and typical scales in high energy physics Elementary particles and typical scales in high energy physics George Jorjadze Free University of Tbilisi Zielona Gora - 23.01.2017 GJ Elementary particles and typical scales in HEP Lecture 1 1/18 Contents

More information

11 Group Theory and Standard Model

11 Group Theory and Standard Model Physics 129b Lecture 18 Caltech, 03/06/18 11 Group Theory and Standard Model 11.2 Gauge Symmetry Electromagnetic field Before we present the standard model, we need to explain what a gauge symmetry is.

More information

PG lectures- Particle Physics Introduction. C.Lazzeroni

PG lectures- Particle Physics Introduction. C.Lazzeroni PG lectures- Particle Physics Introduction C.Lazzeroni Outline - Properties and classification of particles and forces - leptons and hadrons - mesons and baryons - forces and bosons - Relativistic kinematics

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

Lecture 3: Propagators

Lecture 3: Propagators Lecture 3: Propagators 0 Introduction to current particle physics 1 The Yukawa potential and transition amplitudes 2 Scattering processes and phase space 3 Feynman diagrams and QED 4 The weak interaction

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

PARTICLE PHYSICS Major Option

PARTICLE PHYSICS Major Option PATICE PHYSICS Major Option Michaelmas Term 00 ichard Batley Handout No 8 QED Maxwell s equations are invariant under the gauge transformation A A A χ where A ( φ, A) and χ χ ( t, x) is the 4-vector potential

More information

Particle Physics. experimental insight. Paula Eerola Division of High Energy Physics 2005 Spring Semester Based on lectures by O. Smirnova spring 2002

Particle Physics. experimental insight. Paula Eerola Division of High Energy Physics 2005 Spring Semester Based on lectures by O. Smirnova spring 2002 experimental insight e + e - W + W - µνqq Paula Eerola Division of High Energy Physics 2005 Spring Semester Based on lectures by O. Smirnova spring 2002 Lund University I. Basic concepts Particle physics

More information

Elementary (?) Particles

Elementary (?) Particles Elementary (?) Particles Dan Styer; 12 December 2018 This document summarizes the so-called standard model of elementary particle physics. It cannot, in seven pages, even touch upon the copious experimental

More information

6. QED. Particle and Nuclear Physics. Dr. Tina Potter. Dr. Tina Potter 6. QED 1

6. QED. Particle and Nuclear Physics. Dr. Tina Potter. Dr. Tina Potter 6. QED 1 6. QED Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 6. QED 1 In this section... Gauge invariance Allowed vertices + examples Scattering Experimental tests Running of alpha Dr. Tina Potter

More information

Unit 8.1 Nuclear Chemistry - Nuclear Reactions. Review. Radioactivity. State College Area School District Teacher: Van Der Sluys

Unit 8.1 Nuclear Chemistry - Nuclear Reactions. Review. Radioactivity. State College Area School District Teacher: Van Der Sluys Unit 8. Nuclear Chemistry - Nuclear Reactions State College Area School District Teacher: Van Der Sluys Review Atoms consist of electrons, protons and neutrons Atoms of elements are distinguished by the

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

Subatomic Physics: Particle Physics Study Guide

Subatomic Physics: Particle Physics Study Guide Subatomic Physics: Particle Physics Study Guide This is a guide of what to revise for the exam. The other material we covered in the course may appear in uestions but it will always be provided if reuired.

More information

Interactions and Fields

Interactions and Fields Interactions and Fields Quantum Picture of Interactions Yukawa Theory Boson Propagator Feynman Diagrams Electromagnetic Interactions Renormalization and Gauge Invariance Strong Interactions Weak and Electroweak

More information

Saturday Morning Physics -- Texas A&M University. What is Matter and what holds it together? Dr. Rainer J. Fries. January 27, 2007

Saturday Morning Physics -- Texas A&M University. What is Matter and what holds it together? Dr. Rainer J. Fries. January 27, 2007 Saturday Morning Physics -- Texas A&M University Particles and Forces What is Matter and what holds it together? Dr. Rainer J. Fries January 27, 2007 Zooming in on the World around us Particles and Forces

More information

Saturday Morning Physics -- Texas A&M University Dr. Rainer J. Fries

Saturday Morning Physics -- Texas A&M University Dr. Rainer J. Fries Saturday Morning Physics -- Texas A&M University Particles and Forces What is Matter and what holds it together? Dr. Rainer J. Fries January 27, 2007 Zooming in on the World around us Particles and Forces

More information

Quantum Field Theory. and the Standard Model. !H Cambridge UNIVERSITY PRESS MATTHEW D. SCHWARTZ. Harvard University

Quantum Field Theory. and the Standard Model. !H Cambridge UNIVERSITY PRESS MATTHEW D. SCHWARTZ. Harvard University Quantum Field Theory and the Standard Model MATTHEW D. Harvard University SCHWARTZ!H Cambridge UNIVERSITY PRESS t Contents v Preface page xv Part I Field theory 1 1 Microscopic theory of radiation 3 1.1

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

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

Chapter 46. Particle Physics and Cosmology

Chapter 46. Particle Physics and Cosmology Chapter 46 Particle Physics and Cosmology Atoms as Elementary Particles Atoms From the Greek for indivisible Were once thought to be the elementary particles Atom constituents Proton, neutron, and electron

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

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

The Particle World. This talk: What is our Universe made of? Where does it come from? Why does it behave the way it does? The Particle World What is our Universe made of? Where does it come from? Why does it behave the way it does? Particle physics tries to answer these questions. This talk: particles as we understand them

More information

Derivation of Electro Weak Unification and Final Form of Standard Model with QCD and Gluons 1 W W W 3

Derivation of Electro Weak Unification and Final Form of Standard Model with QCD and Gluons 1 W W W 3 Derivation of Electro Weak Unification and Final Form of Standard Model with QCD and Gluons 1 W 1 + 2 W 2 + 3 W 3 Substitute B = cos W A + sin W Z 0 Sum over first generation particles. up down Left handed

More information

Elementary Particles, Flavour Physics and all that...

Elementary Particles, Flavour Physics and all that... Elementary Particles, Flavour Physics and all that... 1 Flavour Physics The term Flavour physics was coined in 1971 by Murray Gell-Mann and his student at the time, Harald Fritzsch, at a Baskin-Robbins

More information

The Building Blocks of Nature

The Building Blocks of Nature The Building Blocks of Nature PCES 15.1 Schematic picture of constituents of an atom, & rough length scales. The size quoted for the nucleus here (10-14 m) is too large- a single nucleon has size 10-15

More information

PHYS 420: Astrophysics & Cosmology

PHYS 420: Astrophysics & Cosmology PHYS 420: Astrophysics & Cosmology Dr Richard H. Cyburt Assistant Professor of Physics My office: 402c in the Science Building My phone: (304) 384-6006 My email: rcyburt@concord.edu My webpage: www.concord.edu/rcyburt

More information

The Strong Interaction and LHC phenomenology

The Strong Interaction and LHC phenomenology The Strong Interaction and LHC phenomenology Juan Rojo STFC Rutherford Fellow University of Oxford Theoretical Physics Graduate School course Lecture 2: The QCD Lagrangian, Symmetries and Feynman Rules

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 02. The Standard Model of Particle Physics. Part I The Particles

Lecture 02. The Standard Model of Particle Physics. Part I The Particles Lecture 02 The Standard Model of Particle Physics Part I The Particles The Standard Model Describes 3 of the 4 known fundamental forces Separates particles into categories Bosons (force carriers) Photon,

More information

PhysicsAndMathsTutor.com

PhysicsAndMathsTutor.com OR K π 0 + µ + v ( µ ) M. (a) (i) quark antiquark pair OR qq OR named quark antiquark pair 0 (iii) us (b) (i) Weak any of the following also score mark: weak interaction weak interaction force weak nuclear

More information

Chapter 1. Introduction

Chapter 1. Introduction Chapter 1 Introduction 1.1 Fundamental Forces Particle physics is concerned with the fundamental constituents of matter and the fundamental forces through which the fundamental constituents interact among

More information

Elementary particles, forces and Feynman diagrams

Elementary particles, forces and Feynman diagrams Elementary particles, forces and Feynman diagrams Particles & Forces quarks Charged leptons (e,µ,τ) Neutral leptons (ν) Strong Y N N Electro Magnetic Y Y N Weak Y Y Y Quarks carry strong, weak & EM charge!!!!!

More information

Lecture 2: The First Second origin of neutrons and protons

Lecture 2: The First Second origin of neutrons and protons Lecture 2: The First Second origin of neutrons and protons Hot Big Bang Expanding and cooling Soup of free particles + anti-particles Symmetry breaking Soup of free quarks Quarks confined into neutrons

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

The Discovery of the Higgs boson Matthew Herndon, University of Wisconsin Madison Physics 301: Physics Today. M. Herndon, Phys

The Discovery of the Higgs boson Matthew Herndon, University of Wisconsin Madison Physics 301: Physics Today. M. Herndon, Phys The Discovery of the Higgs boson Matthew Herndon, University of Wisconsin Madison Physics 301: Physics Today M. Herndon, Phys 301 2018 1 The Periodic Table: The early 20 th century understanding of the

More information

The Four Fundamental Forces. The Four Fundamental Forces. Gravitational Force. The Electrical Force. The Photon (γ) Unification. Mass.

The Four Fundamental Forces. The Four Fundamental Forces. Gravitational Force. The Electrical Force. The Photon (γ) Unification. Mass. The Four Fundamental Forces What are the four fundamental forces? The Four Fundamental Forces What are the four fundamental forces? Weaker Stronger Gravitational, Electromagnetic, Strong and Weak Nuclear

More information

An Introduction to the Standard Model of Particle Physics

An Introduction to the Standard Model of Particle Physics An Introduction to the Standard Model of Particle Physics W. N. COTTINGHAM and D. A. GREENWOOD Ж CAMBRIDGE UNIVERSITY PRESS Contents Preface. page xiii Notation xv 1 The particle physicist's view of Nature

More information

Particles and Interactions. Prof. Marina Cobal Corso Particelle ed interazioni fondamentali 2013/2014

Particles and Interactions. Prof. Marina Cobal Corso Particelle ed interazioni fondamentali 2013/2014 Particles and Interactions Prof. Marina Cobal Corso Particelle ed interazioni fondamentali 2013/2014 What is the world made of? In the ancient time: 4 elements 19 century atoms Beginning 20 th century

More information

- ~200 times heavier than the e GeV µ travels on average. - does not interact strongly. - does emit bremsstrahlung in

- ~200 times heavier than the e GeV µ travels on average. - does not interact strongly. - does emit bremsstrahlung in Muons M. Swartz 1 Muons: everything you ve ever wanted to know The muon was first observed in cosmic ray tracks in a cloud chamber by Carl Anderson and Seth Neddermeyer in 1937. It was eventually shown

More information

Beyond the standard model? From last time. What does the SM say? Grand Unified Theories. Unifications: now and the future

Beyond the standard model? From last time. What does the SM say? Grand Unified Theories. Unifications: now and the future From last time Quantum field theory is a relativistic quantum theory of fields and interactions. Fermions make up matter, and bosons mediate the forces by particle exchange. Lots of particles, lots of

More information

Weak interactions. Chapter 7

Weak interactions. Chapter 7 Chapter 7 Weak interactions As already discussed, weak interactions are responsible for many processes which involve the transformation of particles from one type to another. Weak interactions cause nuclear

More information

Introduction. Read: Ch 1 of M&S

Introduction. Read: Ch 1 of M&S Introduction What questions does this field address? Want to know the basic law of nature. Can we unify all the forces with one equation or one theory? Read: Ch 1 of M&S K.K. Gan L1: Introduction 1 Particle

More information

Back to Gauge Symmetry. The Standard Model of Par0cle Physics

Back to Gauge Symmetry. The Standard Model of Par0cle Physics Back to Gauge Symmetry The Standard Model of Par0cle Physics Laws of physics are phase invariant. Probability: P = ψ ( r,t) 2 = ψ * ( r,t)ψ ( r,t) Unitary scalar transformation: U( r,t) = e iaf ( r,t)

More information