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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 between these particles and the forces. It also provides an introduction to the interactions of particles in matter and how they are detected and identified in the experiments at modern particle colliders.
The Standard Model of particle physics
Particle physics is at the heart of our understanding of the laws of nature. It is concerned with the fundamental constituents of the Universe, the elementary particles, and the interactions between them, the forces. Our current understanding is embodied in the Standard Model of particle physics, which provides a unified picture where the forces between particles are themselves described by the exchange of particles. Remarkably, the Standard Model provides a successful description of all current experimental data and represents one of the triumphs of modern physics.
The fundamental particles
In general, physics aims to provide an effective mathematical description of a physical system, appropriate to the energy scale being considered. The world around us appears to be formed from just a few different particles. Atoms are the bound states of negatively charged electrons (e−) which orbit around a central nucleus composed of positively charged protons (p) and electrically neutral neutrons (n). The electrons are bound to the nucleus by the electrostatic attraction between opposite charges, which is the low-energy manifestation of the fundamental theory of electromagnetism, namely Quantum Electrodynamics (QED).
The success of the Standard Model of particle physics in describing the wide range of precise experimental measurements is a remarkable achievement. However, the Standard Model is just a model and there are many unanswered questions. This short concluding chapter provides a broad overview of the current state of our understanding of particle physics and describes some of the more important open issues.
The Standard Model
The ultimate theory of particle physics might consist of a (simple) equation with relatively few free parameters, from which everything else followed. Whilst the Standard Model (SM) is undoubtedly one of the great triumphs of modern physics, it is not this ultimate theory. It is a model constructed from a number of beautiful and profound theoretical ideas put together in a somewhat ad hoc fashion in order to reproduce the experimental data. The essential ingredients of the Standard Model, indicated in Figure 18.1, are: the Dirac equation of relativistic quantum mechanics that describes the dynamics of the fermions; Quantum Field Theory that provides a fundamental description of the particles and their interactions; the local gauge principle that determines the exact nature of these interactions; the Higgs mechanism of electroweak symmetry breaking that generates particle masses; and the wide-reaching body of experimental results that guide the way in which the Standard Model is constructed. The recent precision tests of the Standard Model and the discovery of the Higgs boson have firmly established the validity of the Standard Model at energies up to the electroweak scale. Despite this success, there are many unanswered questions.
In e+e− collisions, the initial-state particles are fundamental fermions. Consequently, the cross sections for processes such as e+e− annihilation are determined by the QED matrix element and the event kinematics (phase space) alone. Calculations of cross sections for collisions involving protons, for example at an electron–proton collider or a hadron collider, also need to account for the composite nature of the proton. This chapter describes low-energy electron–proton elastic scattering. The main purpose is to provide an introduction to a number of concepts which form the starting point for the description of the high-energy interactions of protons that is the main topic of the following chapter.
Probing the structure of the proton
Electron–proton scattering provides a powerful tool for probing the structure of the proton. At low energies, the dominant process is elastic scattering where the proton remains intact. Elastic scattering is described by the coherent interaction of a virtual photon with the proton as a whole, and thus provides a probe of the global properties of the proton, such as its charge radius. At high energies, the dominant process is deep inelastic scattering, where the proton breaks up. Here the underlying process is the elastic scattering of the electron from one of the quarks within the proton. Consequently, deep inelastic scattering provides a probe of the momentum distribution of the quarks.
The precise nature of the e−p → e−p scattering process depends on the wavelength of the virtual photon in comparison to the radius of the proton.
This chapter focusses on the properties of neutrinos and in particular the phenomenon of neutrino oscillations, whereby neutrinos undergo flavour transitions as they propagate over large distances. Neutrino oscillations are a quantum-mechanical phenomenon and can be described in terms of the relationship between the eigenstates of the weak interaction νe, νμ and ντ, and the eigenstates of the free-particle Hamiltonian, known as the mass eigenstates, ν1, ν2 and ν3. The mathematical description of neutrino oscillations is first introduced for two flavours and then extended to three flavours. The predictions are compared to the recent experimental data from reactor and long-baseline neutrino oscillation experiments.
Neutrino flavours
Unlike the charged leptons, which can be detected from the continuous track defined by the ionisation of atoms as they traverse matter, neutrinos are never directly observed; they are only detected through their weak interactions. Different neutrino flavours can only be distinguished by the flavours of charged lepton produced in charged-current weak interactions. Consequently, the electron neutrino νe, is defined as the neutrino state produced in a charged-current weak interaction along with an electron. Similarly, by definition, the weak charged-current interactions of a νe will produce an electron. For many years it was assumed that the νe, νμ and ντ were massless fundamental particles. This assumption was based, at least in part, on experimental evidence. For example, it was observed that the interactions of the neutrino/antineutrino produced along with a positron/electron in a nuclear β-decay, would produce an electron/positron as indicated in Figure 13.1.
The Higgs mechanism and the associated Higgs boson are essential parts of the Standard Model. The Higgs mechanism is the way that the W and Z bosons acquire mass without breaking the local gauge symmetry of the Standard Model. It also gives mass to the fundamental fermions. This chapter describes the Higgs mechanism and the discovery of the Higgs boson at the LHC. The Higgs mechanism is subtle and to gain a full understanding requires the additional theoretical background material covered in the sections on Lagrangians and local gauge invariance in quantum field theory.
The need for the Higgs boson
The apparent violation of unitarity in the e+e− → W+W− cross section was resolved by the introduction of the Z boson. A similar issue arises in the W+W− → W+W− scattering process, where the cross section calculated from the Feynman diagrams shown in Figure 17.1 violates unitarity at a centre-of-mass energy of about 1 TeV. The unitarity violating amplitudes originate from WLWL → WLWL scattering, where the W bosons are longitudinally polarised. Consequently, unitary violation in WW scattering can be associated with the W bosons being massive, since longitudinal polarisation states do not exist for massless particles. The unitarity violation of the WLWL → WLWL cross section can be cancelled by the diagrams involving the exchange of a scalar particle, shown in Figure 17.2. In the Standard Model this scalar is the Higgs boson.
This chapter provides an introduction to the weak interaction, which is mediated by the massive W+ and W− bosons. The main topics covered are: the origin of parity violation; the V−A form of the interaction vertex; and the connection to Fermi theory, which is the effective low-energy description of the weak charged current. The calculation of the decay rate of the charged pion is used to illustrate the rôle of helicity in weak decays. The purpose of this chapter is to describe the overall structure of the weak interaction; the applications are described in the following chapters on charged-current interactions, neutrino oscillations and CP violation in the weak decays of neutral mesons.
The weak charged-current interaction
At the fundamental level, QED and QCD share a number of common features. Both interactions are mediated by massless neutral spin-1 bosons and the spinor part of the QED and QCD interaction vertices have the same ū(p′)γμu(p) form. The charged-current weak interaction differs in almost all respects. It is mediated by massive charged W± bosons and consequently couples together fermions differing by one unit of electric charge. It is also the only place in the Standard Model where parity is not conserved. The parity violating nature of the interaction can be directly related to the form of the interaction vertex, which differs from that of QED and QCD.
Parity
The parity operation is equivalent to spatial inversion through the origin, x → −x.