Units and dimensions

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

INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS

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

Space-Time Symmetries

Physics 4213/5213 Lecture 1

Lecture 01. Introduction to Elementary Particle Physics

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

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

Introduction to Elementary Particles

Weak interactions, parity, helicity

Lecture 3. lecture slides are at:

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

The Standard Model (part I)

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

Lecture 3. lecture slides are at:

Properties of Elementary Particles

Outline. Charged Leptonic Weak Interaction. Charged Weak Interactions of Quarks. Neutral Weak Interaction. Electroweak Unification

Some fundamental questions

4. The Standard Model

A first trip to the world of particle physics

Option 212: UNIT 2 Elementary Particles

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

Lecture 3: Quarks and Symmetry in Quarks

Topics in Standard Model. Alexey Boyarsky Autumn 2013

Interactions/Weak Force/Leptons

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

Energy Level Energy Level Diagrams for Diagrams for Simple Hydrogen Model

Fundamental Interactions (Forces) of Nature

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

Invariance Principles and Conservation Laws

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

Interactions/Weak Force/Leptons

What is matter and how is it formed?

Dr Victoria Martin, Spring Semester 2013

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

Cosmology and particle physics

1. What does this poster contain?

A Brief History of Modern Physics

Introduction to Particle Physics. HST July 2016 Luis Alvarez Gaume 1

Feynman Diagrams. e + e µ + µ scattering

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

Weak interactions. Chapter 7

Modern physics 1 Chapter 13

Elementary particles and typical scales in high energy physics

Quantum Physics 2006/07

. Thus his equation would have to be of the form. 2 t. but must also satisfy the relativistic energy-momentum relation. H 2 φ = ( p 2 + m 2 )φ (3)

Fundamental Particles

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

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

An Introduction to Particle Physics

Particle Physics. Michaelmas Term 2011 Prof. Mark Thomson. Handout 2 : The Dirac Equation. Non-Relativistic QM (Revision)

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

Introduction. Read: Ch 1 of M&S

Interactions and Fields

Particle Physics Dr. Alexander Mitov Handout 2 : The Dirac Equation

Matter: it s what you have learned that makes up the world Protons, Neutrons and Electrons

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

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

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

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

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

Chapter 46 Solutions

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

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

Chapter 32 Lecture Notes

PG lectures- Particle Physics Introduction. C.Lazzeroni

Quantum Gravity and Entanglement

SECTION A: NUCLEAR AND PARTICLE PHENOMENOLOGY

Quantum Field Theory

Quantum Field Theory

2.4 Parity transformation

Quantum Field Theory

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

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

Particle Physics. Dr Victoria Martin, Spring Semester 2012 Lecture 14: CP and CP Violation

Lecture 3. Experimental Methods & Feynman Diagrams

The Building Blocks of Nature

THE STANDARD MODEL OF MATTER

OUTLINE. CHARGED LEPTONIC WEAK INTERACTION - Decay of the Muon - Decay of the Neutron - Decay of the Pion

Physics 214 Experimental Particle Physics. Lecture 1 What to expect.

Physics 214 Experimental Particle Physics. Lecture 1 What to expect.

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

Introduction. Introduction to Elementary Particle Physics. Diego Bettoni Anno Accademico

Outline. Charged Leptonic Weak Interaction. Charged Weak Interactions of Quarks. Neutral Weak Interaction. Electroweak Unification

Modern Physics. Luis A. Anchordoqui. Department of Physics and Astronomy Lehman College, City University of New York. Lesson XI November 19, 2015

Introduction to Elementary Particle Physics. Note 01 Page 1 of 8. Natural Units

Einstein s Theory Relativistic 0 < v < c. No Absolute Time. Quantization, Zero point energy position & momentum obey Heisenberg uncertainity rule

Review Chap. 18: Particle Physics

THERMAL HISTORY OF THE UNIVERSE

PhysicsAndMathsTutor.com 1

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 Dr. Rainer J. Fries

PHY-105: Introduction to Particle and Nuclear Physics

Physics 129 LECTURE 6 January 23, Particle Physics Symmetries (Perkins Chapter 3)

FYS3510 Subatomic Physics. Exam 2016

Physics 214 Experimental Particle Physics. Lecture 1 What to expect.

Quantum Physics and General Relativity

Neutron Decay Disagree

Lecture 4: Antiparticles

Introduction to Nuclear and Particle Physics

Transcription:

Particles and Fields Particles and Antiparticles Bosons and Fermions Interactions and cross sections The Standard Model Beyond the Standard Model Neutrinos and their oscillations

Particle Hierarchy Everyday objects are made of molecules Molecules are made of atoms Atoms are made of nuclei and electrons Nuclei are made of protons and neutrons Protons and neutrons are made of quarks Quarks and electrons are fundamental?

Macro and Micro worlds Modern cosmology and particle physics are deeply connected: astroparticle physics is the scientific area that deals with the interplay between the microscopic and macroscopic worlds Particle physics is the study of the fundamental constituents of matter and their interactions. The modern theory - Standard Model - explains the properties and interactions of the building blocks of matter (they are assumed to be elementary, not made by smaller constituents): - quarks and leptons: fermions of spin angular momentum 1/2 (h) - gauge bosons: the force carriers with spin 1 or integer The spin is a quantum number: fermions/bosons obey the Fermi-Dirac/Bose- Einstein statistics (the wavefunction describing a pair of identical fermions is antysimmetric/symmetric under their exchange - Spin-statistics theorem by Pauli 1940) Ψ 1 2 Ψ fermions Ψ 1 2 Ψ bosons Consequently: Pauli exclusion principle 2 identical fermions cannot exist in the same quantum state (otherwise their wavefunction should be symmetric) hence on an atomic level there can be 2 electrons with opposite spins

1 fm = 10-15 m 1 barn = 10-28 m 2 Units and dimensions 1 ev = 1.6 10-19 J (1 GeV = 10 9 ev, 1 TeV = 10 12 ev, 1 PeV= 10 15 ev, 1EeV= 10 18 ev) Since E = mc 2 (rest energy) masses are measured often in MeV/c 2 h = h/(2π) = reduced Plank constant =6.582 10-25 GeV s p=h/λ E = hν De Broglie Uncertainty principle ΔxΔp h ΔtΔE h Natural units: h = 1 c = 1 All quantities have the dimension of a power of the energy: M = E c L = hc 2 E T = h E Hence a quantity than in MKS has dimensions M p L q T r has dimensions E p-q-r Example: Thompson scattering (photon scattering on free electrons when E γ <<m e c 2 ) to have area dimensions σ = 8π 3 α 2 m e 2 = 8π 3 α 2 m e 2 ha c b = 8π 3 α 2 (hc) 2 (m e 2 c 2 ) 2 = 6.65 10 29 m 2 m e c 2

Matter and Anti-matter Antiparticles look and behave just like their corresponding matter particles, but have opposite charges. For instance, a proton is electrically positive whereas an antiproton is electrically negative. Gravity affects matter and antimatter the same way because gravity is not a charged property and a matter particle has the same mass as its antiparticle. When a matter particle and antimatter particle meet, they annihilate into pure energy! In 1928 Dirac proposed the relativistic equation whose solutions are 4-component wavefunctions corresponding to 2 spin ±1/2 substates of positive and negative energy describing free electrons. Positrons are the states of negative energy. They were discovered in 1933 by Anderson in a cloud chamber experiment with cosmic rays

Matter and Anti-matter asymmetry Matter is the result of the tiny asymmetry of order of 10-9 between matter and antimatter that emerged from the earliest universe. This asymmetry can arise from a baryon non-conserving process. One of the main mysteries of modern cosmology is what caused this tiny difference: it may be tied to proton decay or to a slight preference for the formation of matter over antimatter such as CP violation C=charge-conjugation operator: transforms a particle in its antiparticle; P = parity = spatial inversion of coordinates PΨ(r) Ψ( r) Theories of Grand Unification foresee p decay with a lifetime of 10 35 yrs and experimental limits are currently roughly 10 32-33 yrs. CP violation, initially observed in the K-meson system and found also in the B-meson system, is allowed in the SM but the magnitude of the violation cannot account for the present asymmetry between matter-antimatter in the universe. A new source of CP (or T) violation would be needed such as the existence of electric dipole moments of the electron and the neutron (eg a n is uncharged so It could arise from an asymmetry between positive and negative charge clouds relative to the spin direction).

Relativistic wave equations In quantum theory, a particle with momentum p is described by de Broglie wave function i(p x Et )/h Ψ(x,t) = Ne with N = norm. const. Non relativistically: E = p 2 /2m and Ψ obeys the Shröedinger equation obtained substituting the quantum-mechanical operators p ih = ih r E ih t ih Ψ(x,t) t = h2 2m 2 Ψ(x,t) Is a solution of negative energy and momentum -p: ν = E / h λ = h / p Klein-Gordon Relativistically: E 2 = p 2 c 2 + m 2 c 4 h 2 Ψ(x,t) equation for a = h 2 c 2 2 Ψ(x,t) + m 2 c 4 Ψ(x,t) t 2 spin-0 particle For every solution of momentum p and positive energy of the form above there Ψ (x,t) = Ψ * i( p x +Et )/h (x,t) = Ne

The Dirac equation In 1928 Dirac looked for an equation for spin-1/2 particles of the form i h Ψ(x,t) t ˆ = H(x, ˆ p )Ψ(x,t) Assuming derivatives in space and time of 1st order (required by Lorentz invariance) the equation becomes: ih Ψ(x,t) Ψ = HΨ = ihc α i p = ih hamiltonian + βmc 2 Ψ t i x i Where α i and β are 4 x 4 matrices and Ψ are 4-component wave functions whose values are found imposing solutions of the Dirac are also solution of Klein- Gordon eq. Plane wave solutions of the Dirac equation are: where the 4-component spinor satisfies the eigenvalue equation This equation has 4 solutions: 2 of positive energy corresponding to 2 possible states of spin-1/2 particle and 2 negative energy solutions (positron). This results in the prediction that a pointlike spin-1/2 particle of mass m and charge q has a Dirac magnetic moment µ = qs/m S= spin vector. This provides a test for the point-like nature of any spin-1/2 fermion. For p and n the values indicate that they are not elementary particles µ p = 2.79 e m p S µ n = 1.91 e m n S i(p x Et )/h Ψ(x,t) = u(p)e Hu(p) = ( cα p + βmc 2 )u(p) = Eu(p)

Feynmann diagrams In 1940 Feynman developed a pictorial technique for describing interactions useful for cross-section calculations. They are representations of the amplitudes of particle reactions (i.e. scatterings or decays, particle exchange). Time flows on the right: an arrow towards the right indicates a particle, towards the left an antiparticle. Each vertex contributes to the amplitude with a constant that represents the strength of the interaction (coupling constant) X is a virtual particle and the time it exists is governed by the uncertainty principle

Real processes Classically: interaction at a distance is described by a field due to a source producing an action in the surrounding region. In quantum theory, quanta (bosons) associated to an interaction are exchanged. Since they carry energy and momentum conservation laws are satisfied only if this exchange occurs in a time limited by the Uncertainty Principle: ΔE Δt h These transient quanta are then called virtual. Electromagnetic interactions: the strength of the interaction between charged particles and the photon is given by the fine structure constant α = e2 4πhc = 1 137.0360 In the rest frame of the electron e - (E 0,0) e - (E k, k) + γ(ck,k) E 0 = mc 2 E k = k 2 c + m 2 c 4 tot = k 2 c 2 + m 2 c 4 E tot + kc E 0 rest energy of e - kinetic E of outcoming e - In the case of em interactions the exchanged virtual particle is a photon (scattering of 2 electrons) energy cons. violated (but only for a time compatible with uncertainty principle)