# STANDARD MODEL PDF

elementary particles. 2. Theoretical foundation of the standard model of particle physics. 3. Limitations of the standard model. 4. Beyond the standard model. While there are several reasons to believe that the Standard Model is These lectures provide a basic introduction to the Standard Model (SM) of particle. An important feature of the Standard Model (SM) is that “it works”: it is consistent . a free Dirac fermion, and add interactions, to construct the Standard Model.

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The Standard Model of particle physics provides the most accurate The fundamental matter particles in the Standard Model are the quarks. The Standard Model summarizes the current knowledge in Particle Physics. It is the quantum theory that includes the theory of strong interactions (quantum. Beyond the Standard Model. A.N. Schellekens. [Word cloud by wfhm.info]. Last modified 12 June 1.

Symmetry breaking[ edit ] By the early s, physicists had realised that a given symmetry law might not always be followed under certain conditions, at least in some areas of physics. Symmetry breaking can lead to surprising and unexpected results. If electroweak symmetry was somehow being broken, it might explain why electromagnetism's boson is massless, yet the weak force bosons have mass, and solve the problems.

Shortly afterwards, in , this was shown to be theoretically possible, at least for some limited non-relativistic cases.

Main article: Higgs mechanism Following the and papers, three groups of researchers independently published the PRL symmetry breaking papers with similar conclusions and for all cases, not just some limited cases. They showed that the conditions for electroweak symmetry would be "broken" if an unusual type of field existed throughout the universe, and indeed, some fundamental particles would acquire mass.

The field required for this to happen which was purely hypothetical at the time became known as the Higgs field after Peter Higgs , one of the researchers and the mechanism by which it led to symmetry breaking, known as the Higgs mechanism.

A key feature of the necessary field is that it would take less energy for the field to have a non-zero value than a zero value, unlike all other known fields, therefore, the Higgs field has a non-zero value or vacuum expectation everywhere. It was the first proposal capable of showing how the weak force gauge bosons could have mass despite their governing symmetry, within a gauge invariant theory.

Although these ideas did not gain much initial support or attention, by they had been developed into a comprehensive theory and proved capable of giving "sensible" results that accurately described particles known at the time, and which, with exceptional accuracy, predicted several other particles discovered during the following years.

## Mathematics and Particle Physics

There was not yet any direct evidence that the Higgs field existed, but even without proof of the field, the accuracy of its predictions led scientists to believe the theory might be true. By the s the question of whether or not the Higgs field existed, and therefore whether or not the entire Standard Model was correct, had come to be regarded as one of the most important unanswered questions in particle physics.

Higgs field[ edit ] According to the Standard Model, a field of the necessary kind the Higgs field exists throughout space and breaks certain symmetry laws of the electroweak interaction.

When the weak force bosons acquire mass, this affects their range, which becomes very small. For many decades, scientists had no way to determine whether or not the Higgs field existed, because the technology needed for its detection did not exist at that time.

If the Higgs field did exist, then it would be unlike any other known fundamental field, but it also was possible that these key ideas, or even the entire Standard Model, were somehow incorrect. Unlike other known fields such as the electromagnetic field , the Higgs field is scalar and has a non-zero constant value in vacuum.

The existence of the Higgs field became the last unverified part of the Standard Model of particle physics, and for several decades was considered "the central problem in particle physics".

It also resolves several other long-standing puzzles, such as the reason for the extremely short range of the weak force. Although the Higgs field is non-zero everywhere and its effects are ubiquitous, proving its existence was far from easy.

Due to renormalization the coupling constants of each of these symmetries vary with the energy at which they are measured. This has led to speculation that above this energy the three gauge symmetries of the standard model are unified in one single gauge symmetry with a simple group gauge group, and just one coupling constant.

Below this energy the symmetry is spontaneously broken to the standard model symmetries. Generically, grand unified theories predict the creation of magnetic monopoles in the early universe, [19] and instability of the proton.

## Symmetry and the Standard Model

Main article: Supersymmetry Supersymmetry extends the Standard Model by adding another class of symmetries to the Lagrangian. These symmetries exchange fermionic particles with bosonic ones.

Such a symmetry predicts the existence of supersymmetric particles, abbreviated as sparticles , which include the sleptons , squarks , neutralinos and charginos. Due to the breaking of supersymmetry , the sparticles are much heavier than their ordinary counterparts; they are so heavy that existing particle colliders may not be powerful enough to produce them.

Neutrinos[ edit ] In the standard model, neutrinos have exactly zero mass. This is a consequence of the standard model containing only left-handed neutrinos.

## Geometry of the Standard Model

With no suitable right-handed partner, it is impossible to add a renormalizable mass term to the standard model. These measurements only give the mass differences between the different flavours. The right-handed neutrinos have to be sterile , meaning that they do not participate in any of the standard model interactions. Because they have no charges, the right-handed neutrinos can act as their own anti-particles, and have a Majorana mass term.

Like the other Dirac masses in the standard model, the neutrino Dirac mass is expected to be generated through the Higgs mechanism, and is therefore unpredictable. The standard model fermion masses differ by many orders of magnitude; the Dirac neutrino mass has at least the same uncertainty.

On the other hand, the Majorana mass for the right-handed neutrinos does not arise from the Higgs mechanism, and is therefore expected to be tied to some energy scale of new physics beyond the standard model, for example the Planck scale.

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The correction due to these suppressed processes effectively gives the left-handed neutrinos a mass that is inversely proportional to the right-handed Majorana mass, a mechanism known as the see-saw. However, due to the uncertainty in the Dirac neutrino masses, the right-handed neutrino masses can lie anywhere.

For example, they could be as light as keV and be dark matter , [26] they can have a mass in the LHC energy range [27] [28] and lead to observable lepton number violation, [29] or they can be near the GUT scale, linking the right-handed neutrinos to the possibility of a grand unified theory. Unlike the quark mixing, which is almost minimal, the mixing of the neutrinos appears to be almost maximal. This has led to various speculations of symmetries between the various generations that could explain the mixing patterns.

These phases could potentially create a surplus of leptons over anti-leptons in the early universe, a process known as leptogenesis. This asymmetry could then at a later stage be converted in an excess of baryons over anti-baryons, and explain the matter-antimatter asymmetry in the universe.

Simulations of structure formation show that they are too hot—i. The simulations show that neutrinos can at best explain a few percent of the missing dark matter.

## Beyond the standard model with the LHC

However, the heavy sterile right-handed neutrinos are a possible candidate for a dark matter WIMP. Preon models generally postulate some additional new particles which are further postulated to be able to combine to form the quarks and leptons of the standard model.

One of the earliest preon models was the Rishon model. Theories of everything[ edit ] Main article: Theory of everything Theoretical physics continues to strive toward a theory of everything, a theory that fully explains and links together all known physical phenomena, and predicts the outcome of any experiment that could be carried out in principle.

In practical terms the immediate goal in this regard is to develop a theory which would unify the Standard Model with General Relativity in a theory of quantum gravity. Additional features, such as overcoming conceptual flaws in either theory or accurate prediction of particle masses, would be desired. The challenges in putting together such a theory are not just conceptual - they include the experimental aspects of the very high energies needed to probe exotic realms.

Several notable attempts in this direction are supersymmetry , string theory, and loop quantum gravity. Main article: String theory Extensions, revisions, replacements, and reorganizations of the Standard Model exist in attempt to correct for these and other issues. String theory is one such reinvention, and many theoretical physicists think that such theories are the next theoretical step toward a true Theory of Everything.

Theories of quantum gravity such as loop quantum gravity and others are thought by some to be promising candidates to the mathematical unification of quantum field theory and general relativity, requiring less drastic changes to existing theories.Close banner Close. Distinguishing spins in decay chains at the Large Hadron Collider. Because they have no charges, the right-handed neutrinos can act as their own anti-particles, and have a Majorana mass term.

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But because every experiment contains some degree of statistical and systemic uncertainty, and the theoretical predictions themselves are also almost never calculated exactly and are subject to uncertainties in measurements of the fundamental constants of the Standard Model some of which are tiny and others of which are substantial , it is mathematically expected that some of the hundreds of experimental tests of the Standard Model will deviate to some extent from it, even if there were no new physics to be discovered.

However, the heavy sterile right-handed neutrinos are a possible candidate for a dark matter WIMP. Yet, no mechanism sufficient to explain this asymmetry exists in the Standard Model.

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