Introduction to the Standard Model. 1. e+e- annihilation and QCD. M. E. Peskin PiTP Summer School July 2005

Similar documents
Quantum Field Theory 2 nd Edition

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

Event Generator Physics 2

Particle Physics. Lecture 11: Mesons and Baryons

Tercera Sesión. XI Escuela de Física Fundamental. Universidad Veracruzana, Xalapa. 28 de Septiembre de 2016

Particle Physics. Dr Victoria Martin, Spring Semester 2012 Lecture 10: QCD at Colliders

Physics at LHC. lecture one. Sven-Olaf Moch. DESY, Zeuthen. in collaboration with Martin zur Nedden

IX. Electroweak unification

Introduction to Elementary Particles

Particle Physics I Lecture Exam Question Sheet

The achievements of the CERN proton antiproton collider

Standard Model of Particle Physics SS 2013

Standard Model of Particle Physics SS 2013

Standard Model of Particle Physics SS 2012

Introduction to the Standard Model New Horizons in Lattice Field Theory IIP Natal, March 2013

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

AN INTRODUCTION TO QCD

Physics at Hadron Colliders Partons and PDFs

The Strong Interaction and LHC phenomenology

PG lectures- Particle Physics Introduction. C.Lazzeroni

Search for a Z at an e + e - Collider Thomas Walker

1 The pion bump in the gamma reay flux

Physique des Particules Avancées 2

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

Deep Inelastic Scattering in Lepton-Hadron Collisions Probing the Parton Structure of the Nucleon with Leptons Basic Formalism (indep.

2. HEAVY QUARK PRODUCTION

Standard Model of Particle Physics SS 2012

Energy-energy and transversal energy-energy correlations in e + e and pp collisions

Understanding Parton Showers

QCD and Rescattering in Nuclear Targets Lecture 2

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

Elementary Particle Physics

Lecture 3 Cross Section Measurements. Ingredients to a Cross Section

PHY357 Lecture 14. Applications of QCD. Varying coupling constant. Jets and Gluons. Quark-Gluon plasma. Colour counting

Massive Quarks in Vincia. M. Ritzmann in collaboration with A. Gehrmann-De Ridder and P. Skands

e e Collisions at ELIC

Standard Model of Particle Physics SS 2013

Part II Particle and Nuclear Physics Examples Sheet 1

High Energy Physics. Lecture 9. Deep Inelastic Scattering Scaling Violation. HEP Lecture 9 1

Introduction to particle physics Lecture 7

Beyond the Standard Model

Lecture 03. The Standard Model of Particle Physics. Part II The Higgs Boson Properties of the SM

Introduction to Elementary Particle Physics I

PRECISION&MEASUREMENTS&

Experimental results on nucleon structure Lecture I. National Nuclear Physics Summer School 2013

Electron-Positron Annihilation

Chapter 1. Introduction

ISR physics at BABAR

Subatomic Physics: Particle Physics Study Guide

Nicolas Berger SLAC, Menlo Park, California, U.S.A.

Name : Physics 490. Practice Final (closed book; calculator, one notecard OK)

BRIEF INTRODUCTION TO HERA PHYSICS

Option 212: UNIT 2 Elementary Particles

The Electro-Strong Interaction

An Introduction to the Standard Model of Particle Physics

Zhong-Bo Kang Los Alamos National Laboratory

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

Kern- und Teilchenphysik I Lecture 13:Quarks and QCD

Introduction to Quantum ChromoDynamics and the parton model

Matching Matrix Elements and Parton Showers with HERWIG and PYTHIA

Lecture 3 (Part 1) Physics 4213/5213

The simplest observations. How do we know we made a W boson? Easier: How do we know we made a Z boson? Let s consider pp Z + e + e...

The Lund Model. and some extensions. Department of Astronomy and Theoretical Physics Lund University Sölvegatan 14A, SE Lund, Sweden

Gian Gopal Particle Attributes Quantum Numbers 1

Zhong-Bo Kang Los Alamos National Laboratory

Physics at the Large Hadron Collider

R-hadrons and Highly Ionising Particles: Searches and Prospects

Pion Form Factor Measurement at BESIII

Weak interactions. Chapter 7

The Role of Heavy Quarks in Light Hadron Fragmentation. HUGS Manuel Epele Instituto de Física La Plata

3 Dimensional String Theory

Kern- und Teilchenphysik II Lecture 1: QCD

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

Particle Physics WS 2012/13 ( )

Overview and Status of Measurements of F 3π at COMPASS

Physics 161 Homework 2 - Solutions Wednesday August 31, 2011

DEEP INELASTIC SCATTERING

PHY492: Nuclear & Particle Physics. Lecture 24. Exam 2 Particle Detectors

Heavy flavour in Pythia 8 Heavy flavour in showers only

Discovery of Pions and Kaons in Cosmic Rays in 1947

Physics at Hadron Colliders Part II

The W-mass Measurement at CDF

Particle Physics WS 2012/13 ( )

Standard Model of Particle Physics SS 2013

Split SUSY and the LHC

Introductory Lectures on Collider Physics

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

Physics 4213/5213 Lecture 1

arxiv:hep-ex/ v1 16 Jun 2004

129 Lecture Notes More on Dirac Equation

Elementary Particles, Flavour Physics and all that...

Intro to Nuclear and Particle Physics (5110)

Lepton and gamma nuclear reactions. J.P. Wellisch, CERN/EP, Geant4 Users Workshop, SLAC, Feb 2002

The Quark Parton Model

Introduction to Monte Carlo Techniques in High Energy Physics

Introduction to Perturbative QCD

Overview of Elementary Particle Physics

4. The Standard Model

Speculations on extensions of symmetry and interctions to GUT energies Lecture 16

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

Transcription:

Introduction to the Standard Model 1. e+e- annihilation and QCD M. E. Peskin PiTP Summer School July 2005

In these lectures, I will describe the phenomenology of the Standard Model of particle physics. I will discuss mainly processes seen in e+e- annihilation at CM energies from 10 to 200 GeV. Later in the school, you will hear about proton-proton collisions at very high energy. But e+e- reactions are much simpler, so this is a good place to start. Even at 10 GeV, the energy is high enough that we can ignore the masses of most of the quarks and leptons. Then we can see the Standard Model gauge interactions in a pure form and relate phenomena directly to the Standard Model Lagrangian.

You know the Standard Model as a 4-d SU(3) x SU(2) x U(1) non-supersymmetric gauge theory that is chiral but anomaly-free in which masses are forbidden by SU(2) x U(1) symmetry and therefore arise only by spontaneous symmetry breaking. Fine. But, what do the particles of the Standard Model actually look like in the lab?

Begin with the leptons: e, µ, τ + ν e, ν µ, ν τ Begin, in fact, with the simplest reaction involving leptons e + e µ + µ in QED At high energy, ignore all masses. Then, helicity h = S ˆP is a Lorentz-invariant. Fermions are described as left-handed right-handed e + L e R The is the antiparticle of the and vice versa.

The amplitudes for helicity are very simple: e + e µ + µ between states of definite k 1 im(e L e+ R µ L µ+ R ) p 1 that is, = 2i e2 q 2 [2p 1 k 2 2p 2 k 1 ] 1/2 = ie 2 (1 + cos θ) (1) im(e L e+ R µ L µ+ R ) = im(e R e+ L µ R µ+ L ) = ie2 (1 + cos θ) im(e L e+ R µ R µ+ L ) = im(e R e+ L µ L µ+ R ) = ie2 (1 cos θ) k 2 p 2

These formulae lead to the regularities: dσ d cos θ (1 + cos2 θ) σ = 4πα2 3s = 87. fb (E CM TeV) 2 s = q 2 = (E CM ) 2 with. The second formula sets the size of cross sections for all QED and electroweak processes. Here are some examples of e+e- annihilation to leptons e + e µ + µ e + e τ + τ e + e e + e and the related process of Bhabha scattering: +

A relativistic muon is a minimum ionizing particle, giving a continuous small energy loss in matter: The muon is long-lived and essentially stable in high energy experiments. τ = 2.2 10 6 sec Electrons emit hard gamma rays, and gammas convert to electron-positron pairs in a characteristic distance called a radiation length. In heavy materials, X 0 de dx 1 GeV/m cτ = 660 m The result is an electromagnetic shower: X 0 cm An electromagnetic calorimeter collects the resulting ionization, which gives a measure of the total energy of the original particle.

e + e _ e + Z 0 e _ SLD

e + e µ + µ BaBar

e e + _ + _ Z 0 SLD

For the The τ τ lepton, τ = 2.9 10 13 sec cτ = 0.087 mm rapidly decays through weak interactions τ ν τ ν e e ν τ ν µ µ ν τ ud, ν τ us ν τ π, ν τ ρ, ν τ a 1, π π 0 3π This produces a variety of τ events

e + e τ + τ eµνν

Leptonic reactions are modified by radiative corrections. I would like to examine in particular the diagrams giving initialstate radiation (ISR) q becomes singular when p 0 (p + q) 2 = 2p q + p 2 2p 2

In the limit in which the and are almost collinear, we can isolate the sigularity for γ emission. Its coefficient has the form: xp e L and this leads to the following approximate expression with p f(x) = α 2π dp 2 p 2 e (1-x)p 1 + (1 x) 2 x γ = σ(e (p 1 )e + (p 2 ) γ + e e + γ + X) = 1 0 + ie ie 2(1 x) x(1 x) p = α 2π log s m 2 e γ L 2(1 x) x p γ R dx f(x) σ(e ((1 x)p 1 ) + e + (p 2 ) X) 1 0 dx f(x) σ(e (p 1 ) + e + ((1 x)p 2 ) X) 1 + (1 x)2 x

These singular terms give enhanced radiation in directions parallel to the momenta of the initial state particles (ISR) and also parallel to the momenta of the final state particles (FSR).

Here is a BaBar hadronic event with ISR

In addition to the leptonic processes, we also have e + e qq How do these reactions appear? Quarks are not seen in isolation. If isolated quarks could be produced in e+e- annihilation, it would be obvious, because quarks carry fractional charge.

A property of the strong coupling phase of gauge theories is that the gauge charge is permanently confined into gauge singlet states. A way to picture this is that the electric flux of the gauge field cannot spread into the vacuum. Since this flux is conserved, we have states such as _ d u This object is a relativistic string. It has E L As the string becomes longer, it becomes energetically favorable to create an additional pair. qq

This leads to a first picture of the time development of a state created in e+e- annihilation: qq _ d u _ d d _ d u _ d s _ s u _ u d _ d u Asymptotic freedom implies that all of these nonperturbative effects take place with no large momentum transfer. Then, the final momenta are approximately collinear and parallel to the original quark directions.

Thus, we expect e + e qq the final states in jets of mesons and baryons should look like the angular distribution of the axes of the jets should be dσ d cos θ (1 + cos2 θ) the cross section for such jet-like events should be σ = 4πα2 3s 3 f Q 2 f

e + e qq BaBar

SLD

SLD

θ

7 's 's Burkhardt, Pietrzyk 2005 6 5 4 Rhad 3 2 1 0 0.9 s in GeV Bacci et al. Cosme et al. PLUTO CESR, DORIS MARK I CRYSTAL BALL MD-1 VEPP-4 VEPP-2M ND DM2 BES 1999 BES 2001 CMD-2 2004 KLOE 2005 15 5.9 6 1.4 rel. err. cont. 0 1 2 3 4 5 6 7 8 9 10

What do we see in such a jet? The components are: π. K, p cτ(k + ) = 3.7 m π 0 2γ with cτ = 2.5 10 6 cm Long-lived charged hadrons: π 0 s : Long-lived neutral hadrons: n, KL 0 Short-lived hadrons with : Charged particles appear as tracks. γ cτ few cm K 0 S, Λ, Σ, Ξ s appear as energy deposited in an electromagnetic calorimeter Hadrons appear as energy deposition in a hadron calorimeter thick enough to allow many hadron interaction lengths X 0 = 0.56 cm (Pb), 1.76 cm (Fe), 35.3 cm (Be) λ I = 17.1 cm (Pb), 16.8 cm (Fe), 40.7 cm (Be) so by choosing different materials, it possible to separately measure the various components of the jet

Up to now we have ignored the asymptotically free QCD coupling α s = g 2 s/4π α s Let s now compute the effects of order : These include diagrams with virtual gluons and diagrams with real gluon emission: setting E q = x q s 2 E q = x q s 2 the gluon emission diagrams predict: dσ dx q dx q = σ 0 2α s 3π E g = x g s 2 x 2 q + x 2 q (1 x q )(1 x q )

Notice that the gluon emission is singular as These are configurations in which the gluon is collinear with the antiquark or quark. It is possible integrate up the total cross section by working in Then the real gluon emission gives in all σ = σ 0 2α s 3π d = 4 + ɛ ( 8 ɛ 2 + 1 [4 log s ɛ M 2 6] + log 2 s M 2 3 log The virtual diagrams { give σ = σ 0 1 + 2α ( s 3π 8 ɛ 2 1 [4 log s ɛ log 2 s M 2 + 3 log σ = σ 0 (1 + 2α s 3π 3 2 ) = σ 0 (1 + α s π ) x q, x q 1 s M 2 7π2 6 + 57 6 M 2 6] ) s M 2 + 7π2 6 8 )}

The final result, and its generalization to higher orders, gives a small positive modification of the cross section for e + e qq σ = σ 0 (1 + α s(s) π + 1.441 ( ) 2 αs (s) 12.8 π ( ) 3 αs (s) + ) π Gluon emission at wide angles gives 3-jet events at a rate proportional to 4-jet events at a rate proportional to α s α 2 s etc.

SLD 3-jet event

SLD 4-jet event

1/N dn/dx 3 1/N dn/dx 1 15 10 3 96 8121A3 5 0 0.6 0.8 1.0 4 2 0 0 (a) (c) x 1 0.2 0.4 0.6 x 3 SLD HERWIG 5.7 1/N dn/dx 2 1/N dn/dcos EK 6 4 2 0 3 2 1 0 0 (b) 0.6 0.8 1.0 (d) x 2 0.4 0.8 cos EK

e + e qq If a large fraction of events contain gluon emissions, we need a systematic way to identify jets and to count the number of jets in an event. Actually, since we only observe hadrons and not quarks, we need such a procedure anyway, to give a systematic way to compute, e.g., the orientation of the jet axis. Among many possible ways to do this, a particularly useful one is based on thrust T = max ˆn j ˆn p j j p j The axis that gives the maximum (the thrust axis) is a reasonable definition of the event axis. QCD predicts in leading order dσ dt = σ 0 2α { s 2(3T 2 3T + 2) 3π T (1 T ) log 2T 1 1 T 3((3T 2)(2 T ) (1 T ) }

Particle distribution from the thrust axis, from the BaBar experiment ( ECM = 10.58 GeV)

For multi-jet events, we need a way to partition the hadrons in the event into jets. Here is a particular method; later in the school, we will discuss other possible algorithms. Let y ij = (p i + p j ) 2 s Choose the 2 particles in the final state s.t. is minimal. Merge them and replace them with 1 particle with p = (p i + p j ). Continue until Then the resulting jet momenta. 2p i p j s 1 2 x ix j (1 cos θ ij ) (p i + p j ) 2 (p i + p j ) 2 can be taken as the operationally defined Jets in QCD have a fractal structure, with more structure revealed as is decreased. y cut p i s > y cut

Jet Fraction 1 0.8 OPAL (91 GeV) Durham 0.6 0.4 2-jet 3-jet 4-jet 5-jet PYTHIA HERWIG 0.2 0 10-4 10-3 10-2 10-1 y cut

Jet Fraction 1 0.8 OPAL (197 GeV) Durham 0.6 0.4 2-jet 3-jet 4-jet 5-jet PYTHIA HERWIG 0.2 0 10-4 10-3 10-2 10-1 y cut

Thinking about how multiple gluons are emitted by a quark, we can arrive at a less naive model of how a qq state in e+e- annihilation evolves into a state of many hadrons. Define the fragmentation function: For a hadron h in the final state of e+e- annihilation, let longitudinal fraction z = E h /( 1 2 s) Then let f h (z)dz be the probability of finding a hadron in the final state with longitudinal fraction z. p h zp

10 2 10 1 SLD u,d,s Jets + K p K + (x0.1) p (x0.02) (1/2N evts ) dn/dx p 10 0 10-1 10-2 10-3 10-4 0.04 0.1 0.4 1 8-2003 8675A13 x p fragmentation functions measured by SLD

The variable z gives the fraction of the original quark energy that ends up in a final handron. With QCD, we have studied the first stage of the degradation of the energy of the quark, due to gluon emission. Let s look again at the formula for gluon radiation dσ dx q dx q = σ 0 2α s 3π x q 1 x q (1 x g ) In the limit (q+g collinear; ), integrating over, this becomes x q dσ σ 0 4 dx g 3 α s 2π log x 2 q + x 2 q (1 x q )(1 x q ) s m 2 1 + (1 x g) 2 (qg) min x g This is the same radiation formula that we saw in QED.

This calculation describes the emission of one approximately collinear gluon. By repeating the process, we can describe multiple gluon emissions. These multiple gluons build up the structure of a quark jet. p The quark first emits hard gluons. As we go to smaller or smaller virtualities, the quarks and gluons emit further quarks and gluons.

Each emission degrades the energy of the final hadrons. This effect of collinear gluon emission from the quark is described by the Gribov-Lipatov equation df q (x, Q) d log Q = α s π Here P(z) is the splitting function P q q (z) = 4 3 1 ( 1 + z 2 (1 z) ) Aδ(1 z) where A is determined by the condition of quark number 1 conservation dzp q q (z) = 0 0 The singularity is normally treated in QCD by defining a distribution that agrees with 1/(1-z) for z < 1 such that 1 0 dz 0 dz z P q q(z) f q ( x z, Q) 1 (1 z) + = 0

The full dynamics of QCD contains a number of possible collinear splitting processes. Each leads to a characteristic kernel, the splitting functions P q q (z) = 4 ( 1 + z 2 + 3 ) δ(1 z) 3 (1 z) + 2 P g q (z) = 4 ( ) 1 + (1 z) 2 3 z P q g (z) = 1 ( z 2 + (1 z) 2) 2 ( 1 z z P g g (z) = 6 + + z(1 z) + ( 11 z (1 z) + 12 n ) f )δ(1 z) 18 Putting these effects together, we obtain the Altarelli-Parisi equations. For example df h q (x, Q) d log Q = α s π 1 0 dz z {P q q (z) f h q ( x z, Q) + P g q(z) f h g ( x z, Q) }

According to this equation, fragmentation functions evolve as a function of s. This effect is observed.

PDG (Biebel and Webber) compilation

Finally, we can ask about the value of needed to explain the various QCD effects we have discussed in this lecture. α s The hallmark of a gauge theory is that there is a single unified coupling constant. Is experiment consistent with this?

e+e- event shape variables only

All techniques Bethke

We have now seen that the strong interactions at high energy show very directly the quark-gluon structure of an SU(3) gauge theory - QCD. In the next lecture, we will examine the weak interactions at high energy. We will see that these also reflect the gauge stuctures of the Standard Model.