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Higgs boson

Candidate Higgs boson events from collisions between protons in the LHC. The top event in the CMS experiment shows a decay into two photons (dashed yellow lines and green towers). The lower event in the ATLAS experiment shows a decay into four muons (red tracks).
Composition	Elementary particle
Statistics	Bosonic
Symbol	H
Theorised	R. Brout, F. Englert, P. Higgs, G. S. Guralnik, C. R. Hagen, and T. W. B. Kibble (1964)
Discovered	Large Hadron Collider (2011–2013)
Mass	125.10 ± 0.14 GeV/c
Mean lifetime	1.56×10 s (predicted) 1.2 - 4.6 x 10 s (tentatively measured at sigma 3.2 (1 in 1000) significance)
Decays into	Bottom-antibottom pair (observed) Two W bosons (observed) Two gluons (predicted) Tau-antitau pair (observed) Two Z bosons (observed) Two photons (observed) Two leptons and a photon (Dalitz decay via virtual photon) (tentatively observed at sigma 3.2 (1 in 1000) significance)  Muon-antimuon pair (predicted) Various other decays (predicted)
Electric charge	0 e
Colour charge	0
Spin	0
Weak isospin	−⁠1/2⁠
Weak hypercharge	+1
Parity	+1

The Higgs boson, sometimes called the Higgs particle, is an elementary particle in the Standard Model of particle physics produced by the quantum excitation of the Higgs field, one of the fields in particle physics theory. In the Standard Model, the Higgs particle is a massive scalar boson with zero spin, even (positive) parity, no electric charge, and no colour charge, that couples to (interacts with) mass. It is also very unstable, decaying into other particles almost immediately.

The Higgs field is a scalar field, with two neutral and two electrically charged components that form a complex doublet of the weak isospin SU(2) symmetry. Its "Mexican hat-shaped" potential has a nonzero value everywhere (including otherwise empty space), which breaks the weak isospin symmetry of the electroweak interaction, and via the Higgs mechanism gives some particles mass.

Both the field and the boson are named after physicist Peter Higgs, who in 1964 along with five other scientists in three teams, proposed the Higgs mechanism, a way that some particles can acquire mass. (All fundamental particles known at the time should be massless at very high energies, but fully explaining how some particles gain mass at lower energies, had been extremely difficult.) If these ideas were correct, a particle known as a scalar boson should also exist, with certain properties. This particle was called the Higgs boson, and could be used to test whether the Higgs field was the correct explanation.

After a 40 year search, a subatomic particle with the expected properties was discovered in 2012 by the ATLAS and CMS experiments at the Large Hadron Collider (LHC) at CERN near Geneva, Switzerland. The new particle was subsequently confirmed to match the expected properties of a Higgs boson. Physicists from two of the three teams, Peter Higgs and François Englert, were awarded the Nobel Prize in Physics in 2013 for their theoretical predictions. Although Higgs's name has come to be associated with this theory, several researchers between about 1960 and 1972 independently developed different parts of it.

In the mainstream media, the Higgs boson has often been called the "God particle" from the 1993 book The God Particle by Nobel Laureate Leon Lederman, although the nickname is not endorsed by many physicists.

Introduction

Standard Model of particle physics
Elementary particles of the Standard Model
BackgroundParticle physics Standard Model Quantum field theory Gauge theory Spontaneous symmetry breaking Higgs mechanism
ConstituentsElectroweak interaction Quantum chromodynamics CKM matrix Standard Model mathematics
LimitationsStrong CP problem Hierarchy problem Neutrino oscillations Physics beyond the Standard Model
Scientists Rutherford Thomson Chadwick Bose Sudarshan Davis Jr Anderson Fermi Dirac Feynman Rubbia Gell-Mann Kendall Taylor Friedman Powell Anderson Glashow Iliopoulos Lederman Maiani Meer Cowan Nambu Chamberlain Cabibbo Schwartz Perl Majorana Weinberg Lee Ward Salam Kobayashi Maskawa Mills Yang Yukawa 't Hooft Veltman Gross Pais Pauli Politzer Reines Schwinger Wilczek Cronin Fitch Vleck Higgs Englert Brout Hagen Guralnik Kibble de Mayolo Lattes Zweig
v t e

The Standard Model

Physicists explain the fundamental particles and forces of our universe in terms of the Standard Model – a widely accepted framework based on quantum field theory that predicts almost all known particles and forces other than gravity with great accuracy. (A separate theory, general relativity, is used for gravity.) In the Standard Model, the particles and forces in nature (other than gravity) arise from properties of quantum fields, known as gauge invariance and symmetries. Forces in the Standard Model are transmitted by particles known as gauge bosons.

Gauge invariant theories and symmetries

"It is only slightly overstating the case to say that physics is the study of symmetry" – Philip Anderson, Nobel Prize Physics

Gauge invariant theories are theories which have a useful feature, that some kinds of changes to the value of certain items don't make any difference to the outcomes or the measurements we make. An example is that changing voltages in an electromagnet by +100 volts, doesn't cause any change to the magnetic field it produces. Similarly, measuring the speed of light in a vacuum seems to give the identical result whatever the location in time and space, and whatever the local gravitational field. In these kinds of theories, the gauge is an item whose value we can change, the fact that some changes leave the results we measure unchanged means it is a gauge invariant theory, and symmetries are the specific kinds of changes to the gauge, which have this effect of leaving measurements unchanged. (More precisely, these transformations of the gauge component do not change the energy). Symmetries of this kind are powerful tools for deep understanding of the fundamental forces and particles of our physical world, and gauge invariance is therefore an important property within particle physics theory. They are closely connected to conservation laws, and mathematically, are described using group theory. Quantum field theory and the Standard Model are both gauge invariant theories – meaning they focus on properties of our universe that demonstrate this property of gauge invariance, and the symmetries which are involved.

The problem of gauge boson mass

Quantum field theories based on gauge invariance had been used with great success in understanding the electromagnetic and strong forces, but by around 1960 all attempts to create a gauge invariant theory for the weak force (and its combination with the electromagnetic force, known together as the electroweak interaction) had consistently failed, with gauge theories thereby starting to fall into disrepute as a result. The problem was that the symmetry requirements for these two forces incorrectly predicted that the weak force's gauge bosons (W and Z) would have zero mass. But experiments showed that the W and Z gauge bosons had non-zero mass. A further problem was that many promising solutions seemed to require extra particles known as Goldstone bosons to exist. But evidence suggested these did not exist either. This meant that either gauge invariance was an incorrect approach, or something else – unknown – was giving the weak force's W and Z bosons their mass, and doing it in a way that did not create Goldstone bosons either. By the late 1950s and early 1960s, physicists were still completely at a loss how to resolve these issues, or how to create a comprehensive theory for particle physics.

Symmetry breaking

In the late 1950s, Yoichiro Nambu recognised that spontaneous symmetry breaking, a process where a symmetric system becomes asymmetric, could occur under certain conditions. Symmetry breaking is when a change that previously didn't change the measured results (it was originally a "symmetry") now does change the measured results (it's now "broken" and no longer a symmetry). In 1962 physicist Philip Anderson, an expert in condensed matter physics, observed that symmetry breaking played a role in superconductivity, and suggested it could also be part of the answer to the problem of gauge invariance in particle physics. Specifically, he suggested that the Goldstone bosons that would result from symmetry breaking might instead, in some circumstances, be "absorbed" by the massless W and Z bosons. If so, perhaps the Goldstone bosons would not exist, and the W and Z bosons could gain mass, solving both problems at once. Similar behaviour was already theorised in superconductivity. In 1963, this was shown to be theoretically possible by physicists Abraham Klein and Benjamin Lee, at least for some limited (non-relativistic) cases. These findings were formally published in April 1963 (Anderson) and March 1964 (Klein and Lee).

Higgs mechanism

Following the 1963 and early 1964 papers, three groups of researchers independently developed these theories more completely, in what became known as the 1964 PRL symmetry breaking papers. All three groups reached 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, there would be no Goldstone bosons and some existing bosons 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. This non-zero value could in theory break electroweak symmetry. 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 1972 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. During the 1970s these theories rapidly became the Standard Model of particle physics.

Higgs field

The Standard Model includes a field of the kind needed to "break" electroweak symmetry and give particles their correct mass. This field, called the "Higgs Field", exists throughout space, and it breaks some symmetry laws of the electroweak interaction, triggering the Higgs mechanism. It therefore causes the W and Z gauge bosons of the weak force to be massive at all temperatures below an extreme high value. When the weak force bosons acquire mass, this affects the distance they can freely travel, which becomes very small, also matching experimental findings. Furthermore, it was later realised that the same field would also explain, in a different way, why other fundamental constituents of matter (including electrons and quarks) have mass.

Unlike all other known fields such as the electromagnetic field, the Higgs field is a scalar field, and has a non-zero average value in vacuum.

The "central problem"

There was not yet any direct evidence that the Higgs field existed, but even without direct proof, the accuracy of its predictions led scientists to believe the theory might be true. By the 1980s the question of whether the Higgs field existed, and therefore whether the entire Standard Model was correct, had come to be regarded as one of the most important unanswered questions in particle physics.

For many decades, scientists had no way to determine whether 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.

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".

The hypothesised Higgs theory made several key predictions. One crucial prediction was that a matching particle, called the "Higgs boson", should also exist. Proving the existence of the Higgs boson would prove whether the Higgs field existed, and therefore finally prove whether the Standard Model's explanation was correct. Therefore, there was an extensive search for the Higgs boson, as a way to prove the Higgs field itself existed.

Search and discovery

Although the Higgs field would exist everywhere, proving its existence was far from easy. In principle, it can be proved to exist by detecting its excitations, which manifest as Higgs particles (the Higgs boson), but these are extremely difficult to produce and detect, due to the energy required to produce them and their very rare production even if the energy is sufficient. It was therefore several decades before the first evidence of the Higgs boson could be found. Particle colliders, detectors, and computers capable of looking for Higgs bosons took more than 30 years (c. 1980–2010) to develop.

The importance of this fundamental question led to a 40-year search, and the construction of one of the world's most expensive and complex experimental facilities to date, CERN's Large Hadron Collider, in an attempt to create Higgs bosons and other particles for observation and study. On 4 July 2012, the discovery of a new particle with a mass between 125 and 127 GeV/c was announced; physicists suspected that it was the Higgs boson. Since then, the particle has been shown to behave, interact, and decay in many of the ways predicted for Higgs particles by the Standard Model, as well as having even parity and zero spin, two fundamental attributes of a Higgs boson. This also means it is the first elementary scalar particle discovered in nature.

By March 2013, the existence of the Higgs boson was confirmed, and therefore, the concept of some type of Higgs field throughout space is strongly supported.

The presence of the field, now confirmed by experimental investigation, explains why some fundamental particles have mass, despite the symmetries controlling their interactions implying that they should be massless. It also resolves several other long-standing puzzles, such as the reason for the extremely short distance travelled by the weak force bosons, and therefore the weak force's extremely short range.

As of 2018, in-depth research shows the particle continuing to behave in line with predictions for the Standard Model Higgs boson. More studies are needed to verify with higher precision that the discovered particle has all of the properties predicted, or whether, as described by some theories, multiple Higgs bosons exist.

The nature and properties of this field are now being investigated further, using more data collected at the LHC.

Interpretation

Various analogies have been used to describe the Higgs field and boson, including analogies with well-known symmetry-breaking effects such as the rainbow and prism, electric fields, and ripples on the surface of water.

Other analogies based on resistance of macro objects moving through media (such as people moving through crowds, or some objects moving through syrup or molasses) are commonly used but misleading, since the Higgs field does not actually resist particles, and the effect of mass is not caused by resistance.

Overview of Higgs boson and field properties

In the Standard Model, the Higgs boson is a massive scalar boson whose mass must be found experimentally. Its mass has been determined to be 125.35 ± 0.15 GeV. It is the only particle that remains massive even at very high energies. It has zero spin, even (positive) parity, no electric charge, no colour charge, and couples to (interacts with) mass. It is also very unstable, decaying into other particles almost immediately via several possible pathways.

The Higgs field is a scalar field, with two neutral and two electrically charged components that form a complex doublet of the weak isospin SU(2) symmetry. Unlike any other known quantum field, it has a "Mexican hat-shaped" potential. This shape means that below extremely high energies of about 159.5±1.5 GeV  such as those seen during the first picosecond (10 s) of the Big Bang, the Higgs field in its ground state takes less energy to have a nonzero vacuum expectation (value) than a zero value. Therefore in today's universe the Higgs field has a nonzero value everywhere (including otherwise empty space). This nonzero value in turn breaks the weak isospin SU(2) symmetry of the electroweak interaction everywhere. (Technically the non-zero expectation value converts the Lagrangian's Yukawa coupling terms into mass terms.) When this happens, three components of the Higgs field are "absorbed" by the SU(2) and U(1) gauge bosons (the "Higgs mechanism") to become the longitudinal components of the now-massive W and Z bosons of the weak force. The remaining electrically neutral component either manifests as a Higgs boson, or may couple separately to other particles known as fermions (via Yukawa couplings), causing these to acquire mass as well.

Significance

Evidence of the Higgs field and its properties has been extremely significant for many reasons. The importance of the Higgs boson is largely that it is able to be examined using existing knowledge and experimental technology, as a way to confirm and study the entire Higgs field theory. Conversely, proof that the Higgs field and boson did not exist would have also been significant.

Particle physics

Validation of the Standard Model

The Higgs boson validates the Standard Model through the mechanism of mass generation. As more precise measurements of its properties are made, more advanced extensions may be suggested or excluded. As experimental means to measure the field's behaviours and interactions are developed, this fundamental field may be better understood. If the Higgs field had not been discovered, the Standard Model would have needed to be modified or superseded.

Related to this, a belief generally exists among physicists that there is likely to be "new" physics beyond the Standard Model, and the Standard Model will at some point be extended or superseded. The Higgs discovery, as well as the many measured collisions occurring at the LHC, provide physicists a sensitive tool to search their data for any evidence that the Standard Model seems to fail, and could provide considerable evidence guiding researchers into future theoretical developments.

Symmetry breaking of the electroweak interaction

Below an extremely high temperature, electroweak symmetry breaking causes the electroweak interaction to manifest in part as the short-ranged weak force, which is carried by massive gauge bosons. In the history of the universe, electroweak symmetry breaking is believed to have happened at about 1 picosecond (10 s) after the Big Bang, when the universe was at a temperature 159.5±1.5 GeV. This symmetry breaking is required for atoms and other structures to form, as well as for nuclear reactions in stars, such as our Sun. The Higgs field is responsible for this symmetry breaking.

Particle mass acquisition

The Higgs field is pivotal in generating the masses of quarks and charged leptons (through Yukawa coupling) and the W and Z gauge bosons (through the Higgs mechanism).

It is worth noting that the Higgs field does not "create" mass out of nothing (which would violate the law of conservation of energy), nor is the Higgs field responsible for the mass of all particles. For example, approximately 99% of the mass of baryons (composite particles such as the proton and neutron), is due instead to quantum chromodynamic binding energy, which is the sum of the kinetic energies of quarks and the energies of the massless gluons mediating the strong interaction inside the baryons. In Higgs-based theories, the property of "mass" is a manifestation of potential energy transferred to fundamental particles when they interact ("couple") with the Higgs field, which had contained that mass in the form of energy.

Scalar fields and extension of the Standard Model

The Higgs field is the only scalar (spin 0) field to be detected; all the other fields in the Standard Model are spin 1⁄2 fermions or spin 1 bosons. According to Rolf-Dieter Heuer, director general of CERN when the Higgs boson was discovered, this existence proof of a scalar field is almost as important as the Higgs's role in determining the mass of other particles. It suggests that other hypothetical scalar fields suggested by other theories, from the inflaton to quintessence, could perhaps exist as well.

Cosmology

Inflaton

There has been considerable scientific research on possible links between the Higgs field and the inflaton – a hypothetical field suggested as the explanation for the expansion of space during the first fraction of a second of the universe (known as the "inflationary epoch"). Some theories suggest that a fundamental scalar field might be responsible for this phenomenon; the Higgs field is such a field, and its existence has led to papers analysing whether it could also be the inflaton responsible for this exponential expansion of the universe during the Big Bang. Such theories are highly tentative and face significant problems related to unitarity, but may be viable if combined with additional features such as large non-minimal coupling, a Brans–Dicke scalar, or other "new" physics, and they have received treatments suggesting that Higgs inflation models are still of interest theoretically.

Nature of the universe, and its possible fates

In the Standard Model, there exists the possibility that the underlying state of our universe – known as the "vacuum" – is long-lived, but not completely stable. In this scenario, the universe as we know it could effectively be destroyed by collapsing into a more stable vacuum state. This was sometimes misreported as the Higgs boson "ending" the universe. If the masses of the Higgs boson and top quark are known more precisely, and the Standard Model provides an accurate description of particle physics up to extreme energies of the Planck scale, then it is possible to calculate whether the vacuum is stable or merely long-lived. A 125–127 GeV Higgs mass seems to be extremely close to the boundary for stability, but a definitive answer requires much more precise measurements of the pole mass of the top quark. New physics can change this picture.

If measurements of the Higgs boson suggest that our universe lies within a false vacuum of this kind, then it would imply – more than likely in many billions of years – that the universe's forces, particles, and structures could cease to exist as we know them (and be replaced by different ones), if a true vacuum happened to nucleate. It also suggests that the Higgs self-coupling λ and its β_λ function could be very close to zero at the Planck scale, with "intriguing" implications, including theories of gravity and Higgs-based inflation. A future electron–positron collider would be able to provide the precise measurements of the top quark needed for such calculations.

Vacuum energy and the cosmological constant

More speculatively, the Higgs field has also been proposed as the energy of the vacuum, which at the extreme energies of the first moments of the Big Bang caused the universe to be a kind of featureless symmetry of undifferentiated, extremely high energy. In this kind of speculation, the single unified field of a Grand Unified Theory is identified as (or modelled upon) the Higgs field, and it is through successive symmetry breakings of the Higgs field, or some similar field, at phase transitions that the presently known forces and fields of the universe arise.

The relationship (if any) between the Higgs field and the presently observed vacuum energy density of the universe has also come under scientific study. As observed, the present vacuum energy density is extremely close to zero, but the energy densities predicted from the Higgs field, supersymmetry, and other current theories are typically many orders of magnitude larger. It is unclear how these should be reconciled. This cosmological constant problem remains a major unanswered problem in physics.

History

The six authors of the 1964 PRL papers, who received the 2010 J. J. Sakurai Prize for their work; from left to right: Kibble, Guralnik, Hagen, Englert, Brout; right image: Higgs.

Theorisation

Particle physicists study matter made from fundamental particles whose interactions are mediated by exchange particles – gauge bosons – acting as force carriers. At the beginning of the 1960s a number of these particles had been discovered or proposed, along with theories suggesting how they relate to each other, some of which had already been reformulated as field theories in which the objects of study are not particles and forces, but quantum fields and their symmetries. However, attempts to produce quantum field models for two of the four known fundamental forces – the electromagnetic force and the weak nuclear force – and then to unify these interactions, were still unsuccessful.

One known problem was that gauge invariant approaches, including non-abelian models such as Yang–Mills theory (1954), which held great promise for unified theories, also seemed to predict known massive particles as massless. Goldstone's theorem, relating to continuous symmetries within some theories, also appeared to rule out many obvious solutions, since it appeared to show that zero-mass particles known as Goldstone bosons would also have to exist that simply were "not seen". According to Guralnik, physicists had "no understanding" how these problems could be overcome.

Particle physicist and mathematician Peter Woit summarised the state of research at the time:

Yang and Mills work on non-abelian gauge theory had one huge problem: in perturbation theory it has massless particles which don't correspond to anything we see. One way of getting rid of this problem is now fairly well understood, the phenomenon of confinement realized in QCD, where the strong interactions get rid of the massless "gluon" states at long distances. By the very early sixties, people had begun to understand another source of massless particles: spontaneous symmetry breaking of a continuous symmetry. What Philip Anderson realized and worked out in the summer of 1962 was that, when you have both gauge symmetry and spontaneous symmetry breaking, the massless Nambu–Goldstone mode can combine with the massless gauge field modes to produce a physical massive vector field . This is what happens in superconductivity, a subject about which Anderson was (and is) one of the leading experts.

The Higgs mechanism is a process by which vector bosons can acquire rest mass without explicitly breaking gauge invariance, as a byproduct of spontaneous symmetry breaking. Initially, the mathematical theory behind spontaneous symmetry breaking was conceived and published within particle physics by Yoichiro Nambu in 1960 (and somewhat anticipated by Ernst Stueckelberg in 1938), and the concept that such a mechanism could offer a possible solution for the "mass problem" was originally suggested in 1962 by Philip Anderson, who had previously written papers on broken symmetry and its outcomes in superconductivity. Anderson concluded in his 1963 paper on the Yang–Mills theory, that "considering the superconducting analog... hese two types of bosons seem capable of canceling each other out... leaving finite mass bosons"), and in March 1964, Abraham Klein and Benjamin Lee showed that Goldstone's theorem could be avoided this way in at least some non-relativistic cases, and speculated it might be possible in truly relativistic cases.

These approaches were quickly developed into a full relativistic model, independently and almost simultaneously, by three groups of physicists: by François Englert and Robert Brout in August 1964; by Peter Higgs in October 1964; and by Gerald Guralnik, Carl Hagen, and Tom Kibble (GHK) in November 1964. Higgs also wrote a short, but important, response published in September 1964 to an objection by Gilbert, which showed that if calculating within the radiation gauge, Goldstone's theorem and Gilbert's objection would become inapplicable. Higgs later described Gilbert's objection as prompting his own paper. Properties of the model were further considered by Guralnik in 1965, by Higgs in 1966, by Kibble in 1967, and further by GHK in 1967. The original three 1964 papers demonstrated that when a gauge theory is combined with an additional charged scalar field that spontaneously breaks the symmetry, the gauge bosons may consistently acquire a finite mass. In 1967, Steven Weinberg and Abdus Salam independently showed how a Higgs mechanism could be used to break the electroweak symmetry of Sheldon Glashow's unified model for the weak and electromagnetic interactions, (itself an extension of work by Schwinger), forming what became the Standard Model of particle physics. Weinberg was the first to observe that this would also provide mass terms for the fermions.

At first, these seminal papers on spontaneous breaking of gauge symmetries were largely ignored, because it was widely believed that the (non-Abelian gauge) theories in question were a dead-end, and in particular that they could not be renormalised. In 1971–72, Martinus Veltman and Gerard 't Hooft proved renormalisation of Yang–Mills was possible in two papers covering massless, and then massive, fields. Their contribution, and the work of others on the renormalisation group – including "substantial" theoretical work by Russian physicists Ludvig Faddeev, Andrei Slavnov, Efim Fradkin, and Igor Tyutin – was eventually "enormously profound and influential", but even with all key elements of the eventual theory published there was still almost no wider interest. For example, Coleman found in a study that "essentially no-one paid any attention" to Weinberg's paper prior to 1971 and discussed by David Politzer in his 2004 Nobel speech. – now the most cited in particle physics – and even in 1970 according to Politzer, Glashow's teaching of the weak interaction contained no mention of Weinberg's, Salam's, or Glashow's own work. In practice, Politzer states, almost everyone learned of the theory due to physicist Benjamin Lee, who combined the work of Veltman and 't Hooft with insights by others, and popularised the completed theory. In this way, from 1971, interest and acceptance "exploded" and the ideas were quickly absorbed in the mainstream.

The resulting electroweak theory and Standard Model have accurately predicted (among other things) weak neutral currents, three bosons, the top and charm quarks, and with great precision, the mass and other properties of some of these. Many of those involved eventually won Nobel Prizes or other renowned awards. A 1974 paper and comprehensive review in Reviews of Modern Physics commented that "while no one doubted the correctness of these arguments, no one quite believed that nature was diabolically clever enough to take advantage of them", adding that the theory had so far produced accurate answers that accorded with experiment, but it was unknown whether the theory was fundamentally correct. By 1986 and again in the 1990s it became possible to write that understanding and proving the Higgs sector of the Standard Model was "the central problem today in particle physics".

Summary and impact of the PRL papers

The three papers written in 1964 were each recognised as milestone papers during Physical Review Letters's 50th anniversary celebration. Their six authors were also awarded the 2010 J. J. Sakurai Prize for Theoretical Particle Physics for this work. (A controversy also arose the same year, because in the event of a Nobel Prize only up to three scientists could be recognised, with six being credited for the papers.) Two of the three PRL papers (by Higgs and by GHK) contained equations for the hypothetical field that eventually would become known as the Higgs field and its hypothetical quantum, the Higgs boson. Higgs' subsequent 1966 paper showed the decay mechanism of the boson; only a massive boson can decay and the decays can prove the mechanism.

In the paper by Higgs the boson is massive, and in a closing sentence Higgs writes that "an essential feature" of the theory "is the prediction of incomplete multiplets of scalar and vector bosons". (Frank Close comments that 1960s gauge theorists were focused on the problem of massless vector bosons, and the implied existence of a massive scalar boson was not seen as important; only Higgs directly addressed it.) In the paper by GHK the boson is massless and decoupled from the massive states. In reviews dated 2009 and 2011, Guralnik states that in the GHK model the boson is massless only in a lowest-order approximation, but it is not subject to any constraint and acquires mass at higher orders, and adds that the GHK paper was the only one to show that there are no massless Goldstone bosons in the model and to give a complete analysis of the general Higgs mechanism. All three reached similar conclusions, despite their very different approaches: Higgs' paper essentially used classical techniques, Englert and Brout's involved calculating vacuum polarisation in perturbation theory around an assumed symmetry-breaking vacuum state, and GHK used operator formalism and conservation laws to explore in depth the ways in which Goldstone's theorem may be worked around. Some versions of the theory predicted more than one kind of Higgs fields and bosons, and alternative "Higgsless" models were considered until the discovery of the Higgs boson.

Experimental search

To produce Higgs bosons, two beams of particles are accelerated to very high energies and allowed to collide within a particle detector. Occasionally, although rarely, a Higgs boson will be created fleetingly as part of the collision byproducts. Because the Higgs boson decays very quickly, particle detectors cannot detect it directly. Instead the detectors register all the decay products (the decay signature) and from the data the decay process is reconstructed. If the observed decay products match a possible decay process (known as a decay channel) of a Higgs boson, this indicates that a Higgs boson may have been created. In practice, many processes may produce similar decay signatures. Fortunately, the Standard Model precisely predicts the likelihood of each of these, and each known process, occurring. So, if the detector detects more decay signatures consistently matching a Higgs boson than would otherwise be expected if Higgs bosons did not exist, then this would be strong evidence that the Higgs boson exists.

Because Higgs boson production in a particle collision is likely to be very rare (1 in 10 billion at the LHC), and many other possible collision events can have similar decay signatures, the data of hundreds of trillions of collisions needs to be analysed and must "show the same picture" before a conclusion about the existence of the Higgs boson can be reached. To conclude that a new particle has been found, particle physicists require that the statistical analysis of two independent particle detectors each indicate that there is lesser than a one-in-a-million chance that the observed decay signatures are due to just background random Standard Model events – i.e., that the observed number of events is more than five standard deviations (sigma) different from that expected if there was no new particle. More collision data allows better confirmation of the physical properties of any new particle observed, and allows physicists to decide whether it is indeed a Higgs boson as described by the Standard Model or some other hypothetical new particle.

To find the Higgs boson, a powerful particle accelerator was needed, because Higgs bosons might not be seen in lower-energy experiments. The collider needed to have a high luminosity in order to ensure enough collisions were seen for conclusions to be drawn. Finally, advanced computing facilities were needed to process the vast amount of data (25 petabytes per year as of 2012) produced by the collisions. For the announcement of 4 July 2012, a new collider known as the Large Hadron Collider was constructed at CERN with a planned eventual collision energy of 14 TeV – over seven times any previous collider – and over 300 trillion (3×10) LHC proton–proton collisions were analysed by the LHC Computing Grid, the world's largest computing grid (as of 2012), comprising over 170 computing facilities in a worldwide network across 36 countries.

Search before 4 July 2012

The first extensive search for the Higgs boson was conducted at the Large Electron–Positron Collider (LEP) at CERN in the 1990s. At the end of its service in 2000, LEP had found no conclusive evidence for the Higgs. This implied that if the Higgs boson were to exist it would have to be heavier than 114.4 GeV/c.

The search continued at Fermilab in the United States, where the Tevatron – the collider that discovered the top quark in 1995 – had been upgraded for this purpose. There was no guarantee that the Tevatron would be able to find the Higgs, but it was the only supercollider that was operational since the Large Hadron Collider (LHC) was still under construction and the planned Superconducting Super Collider had been cancelled in 1993 and never completed. The Tevatron was only able to exclude further ranges for the Higgs mass, and was shut down on 30 September 2011 because it no longer could keep up with the LHC. The final analysis of the data excluded the possibility of a Higgs boson with a mass between 147 GeV/c and 180 GeV/c. In addition, there was a small (but not significant) excess of events possibly indicating a Higgs boson with a mass between 115 GeV/c and 140 GeV/c.

The Large Hadron Collider at CERN in Switzerland, was designed specifically to be able to either confirm or exclude the existence of the Higgs boson. Built in a 27 km tunnel under the ground near Geneva originally inhabited by LEP, it was designed to collide two beams of protons, initially at energies of 3.5 TeV per beam (7 TeV total), or almost 3.6 times that of the Tevatron, and upgradeable to 2 × 7 TeV (14 TeV total) in future. Theory suggested if the Higgs boson existed, collisions at these energy levels should be able to reveal it. As one of the most complicated scientific instruments ever built, its operational readiness was delayed for 14 months by a magnet quench event nine days after its inaugural tests, caused by a faulty electrical connection that damaged over 50 superconducting magnets and contaminated the vacuum system.

Data collection at the LHC finally commenced in March 2010. By December 2011 the two main particle detectors at the LHC, ATLAS and CMS, had narrowed down the mass range where the Higgs could exist to around 116–130 GeV (ATLAS) and 115–127 GeV (CMS). There had also already been a number of promising event excesses that had "evaporated" and proven to be nothing but random fluctuations. However, from around May 2011, both experiments had seen among their results, the slow emergence of a small yet consistent excess of gamma and 4-lepton decay signatures and several other particle decays, all hinting at a new particle at a mass around 125 GeV. By around November 2011, the anomalous data at 125 GeV was becoming "too large to ignore" (although still far from conclusive), and the team leaders at both ATLAS and CMS each privately suspected they might have found the Higgs. On 28 November 2011, at an internal meeting of the two team leaders and the director general of CERN, the latest analyses were discussed outside their teams for the first time, suggesting both ATLAS and CMS might be converging on a possible shared result at 125 GeV, and initial preparations commenced in case of a successful finding. While this information was not known publicly at the time, the narrowing of the possible Higgs range to around 115–130 GeV and the repeated observation of small but consistent event excesses across multiple channels at both ATLAS and CMS in the 124–126 GeV region (described as "tantalising hints" of around 2–3 sigma) were public knowledge with "a lot of interest". It was therefore widely anticipated around the end of 2011, that the LHC would provide sufficient data to either exclude or confirm the finding of a Higgs boson by the end of 2012, when their 2012 collision data (with slightly higher 8 TeV collision energy) had been examined.

Discovery of candidate boson at CERN

Feynman diagrams showing the cleanest channels associated with the low-mass (~125 GeV) Higgs boson candidate observed by ATLAS and CMS at the LHC. The dominant production mechanism at this mass involves two gluons from each proton fusing to a Top-quark Loop, which couples strongly to the Higgs field to produce a Higgs boson. Left: Diphoton channel: Boson subsequently decays into two gamma ray photons by virtual interaction with a W boson loop or top quark loop. Right: The four-lepton "golden channel": Boson emits two Z bosons, which each decay into two leptons (electrons, muons). Experimental analysis of these channels reached a significance of more than five standard deviations (sigma) in both experiments.

On 22 June 2012 CERN announced an upcoming seminar covering tentative findings for 2012, and shortly afterwards (from around 1 July 2012 according to an analysis of the spreading rumour in social media) rumours began to spread in the media that this would include a major announcement, but it was unclear whether this would be a stronger signal or a formal discovery. Speculation escalated to a "fevered" pitch when reports emerged that Peter Higgs, who proposed the particle, was to be attending the seminar, and that "five leading physicists" had been invited – generally believed to signify the five living 1964 authors – with Higgs, Englert, Guralnik, Hagen attending and Kibble confirming his invitation (Brout having died in 2011).

On 4 July 2012 both of the CERN experiments announced they had independently made the same discovery: CMS of a previously unknown boson with mass 125.3 ± 0.6 GeV/c and ATLAS of a boson with mass 126.0 ± 0.6 GeV/c. Using the combined analysis of two interaction types (known as 'channels'), both experiments independently reached a local significance of 5 sigma – implying that the probability of getting at least as strong a result by chance alone is less than one in three million. When additional channels were taken into account, the CMS significance was reduced to 4.9 sigma.

The two teams had been working 'blinded' from each other from around late 2011 or early 2012, meaning they did not discuss their results with each other, providing additional certainty that any common finding was genuine validation of a particle. This level of evidence, confirmed independently by two separate teams and experiments, meets the formal level of proof required to announce a confirmed discovery.

On 31 July 2012, the ATLAS collaboration presented additional data analysis on the "observation of a new particle", including data from a third channel, which improved the significance to 5.9 sigma (1 in 588 million chance of obtaining at least as strong evidence by random background effects alone) and mass 126.0 ± 0.4 (stat) ± 0.4 (sys) GeV/c, and CMS improved the significance to 5-sigma and mass 125.3 ± 0.4 (stat) ± 0.5 (sys) GeV/c.

The new particle tested as a possible Higgs boson

Following the 2012 discovery, it was still unconfirmed whether the 125 GeV/c particle was a Higgs boson. On one hand, observations remained consistent with the observed particle being the Standard Model Higgs boson, and the particle decayed into at least some of the predicted channels. Moreover, the production rates and branching ratios for the observed channels broadly matched the predictions by the Standard Model within the experimental uncertainties. However, the experimental uncertainties currently still left room for alternative explanations, meaning an announcement of the discovery of a Higgs boson would have been premature. To allow more opportunity for data collection, the LHC's proposed 2012 shutdown and 2013–14 upgrade were postponed by seven weeks into 2013.

In November 2012, in a conference in Kyoto researchers said evidence gathered since July was falling into line with the basic Standard Model more than its alternatives, with a range of results for several interactions matching that theory's predictions. Physicist Matt Strassler highlighted "considerable" evidence that the new particle is not a pseudoscalar negative parity particle (consistent with this required finding for a Higgs boson), "evaporation" or lack of increased significance for previous hints of non-Standard Model findings, expected Standard Model interactions with W and Z bosons, absence of "significant new implications" for or against supersymmetry, and in general no significant deviations to date from the results expected of a Standard Model Higgs boson. However some kinds of extensions to the Standard Model would also show very similar results; so commentators noted that based on other particles that are still being understood long after their discovery, it may take years to be sure, and decades to fully understand the particle that has been found.

These findings meant that as of January 2013, scientists were very sure they had found an unknown particle of mass ~125 GeV/c, and had not been misled by experimental error or a chance result. They were also sure, from initial observations, that the new particle was some kind of boson. The behaviours and properties of the particle, so far as examined since July 2012, also seemed quite close to the behaviours expected of a Higgs boson. Even so, it could still have been a Higgs boson or some other unknown boson, since future tests could show behaviours that do not match a Higgs boson, so as of December 2012 CERN still only stated that the new particle was "consistent with" the Higgs boson, and scientists did not yet positively say it was the Higgs boson. Despite this, in late 2012, widespread media reports announced (incorrectly) that a Higgs boson had been confirmed during the year.

In January 2013, CERN director-general Rolf-Dieter Heuer stated that based on data analysis to date, an answer could be possible 'towards' mid-2013, and the deputy chair of physics at Brookhaven National Laboratory stated in February 2013 that a "definitive" answer might require "another few years" after the collider's 2015 restart. In early March 2013, CERN Research Director Sergio Bertolucci stated that confirming spin-0 was the major remaining requirement to determine whether the particle is at least some kind of Higgs boson.

Confirmation of existence and current status

On 14 March 2013 CERN confirmed the following:

CMS and ATLAS have compared a number of options for the spin-parity of this particle, and these all prefer no spin and even parity . This, coupled with the measured interactions of the new particle with other particles, strongly indicates that it is a Higgs boson.

This also makes the particle the first elementary scalar particle to be discovered in nature.

The following are examples of tests used to confirm that the discovered particle is the Higgs boson:

Findings since 2013

In July 2017, CERN confirmed that all measurements still agree with the predictions of the Standard Model, and called the discovered particle simply "the Higgs boson". As of 2019, the Large Hadron Collider has continued to produce findings that confirm the 2013 understanding of the Higgs field and particle.

The LHC's experimental work since restarting in 2015 has included probing the Higgs field and boson to a greater level of detail, and confirming whether less common predictions were correct. In particular, exploration since 2015 has provided strong evidence of the predicted direct decay into fermions such as pairs of bottom quarks (3.6 σ) – described as an "important milestone" in understanding its short lifetime and other rare decays – and also to confirm decay into pairs of tau leptons (5.9 σ). This was described by CERN as being "of paramount importance to establishing the coupling of the Higgs boson to leptons and represents an important step towards measuring its couplings to third generation fermions, the very heavy copies of the electrons and quarks, whose role in nature is a profound mystery". Published results as of 19 March 2018 at 13 TeV for ATLAS and CMS had their measurements of the Higgs mass at 124.98±0.28 GeV and 125.26±0.21 GeV respectively.

In July 2018, the ATLAS and CMS experiments reported observing the Higgs boson decay into a pair of bottom quarks, which makes up approximately 60% of all of its decays.

Theoretical issues

Theoretical need for the Higgs

Gauge invariance is an important property of modern particle theories such as the Standard Model, partly due to its success in other areas of fundamental physics such as electromagnetism and the strong interaction (quantum chromodynamics). However, before Sheldon Glashow extended the electroweak unification models in 1961, there were great difficulties in developing gauge theories for the weak nuclear force or a possible unified electroweak interaction. Fermions with a mass term would violate gauge symmetry and therefore cannot be gauge invariant. (This can be seen by examining the Dirac Lagrangian for a fermion in terms of left and right handed components; we find none of the spin-half particles could ever flip helicity as required for mass, so they must be massless.) W and Z bosons are observed to have mass, but a boson mass term contains terms which clearly depend on the choice of gauge, and therefore these masses too cannot be gauge invariant. Therefore, it seems that none of the standard model fermions or bosons could "begin" with mass as an inbuilt property except by abandoning gauge invariance. If gauge invariance were to be retained, then these particles had to be acquiring their mass by some other mechanism or interaction.

Additionally, solutions based on spontaneous symmetry breaking appeared to fail, seemingly an inevitable result of Goldstone's theorem. Because there is no potential energy cost to moving around the complex plane's "circular valley" responsible for spontaneous symmetry breaking, the resulting quantum excitation is pure kinetic energy, and therefore a massless boson ("Goldstone boson"), which in turn implies a new long range force. But no new long range forces or massless particles were detected either. So whatever was giving these particles their mass had to not "break" gauge invariance as the basis for other parts of the theories where it worked well, and had to not require or predict unexpected massless particles or long-range forces which did not actually seem to exist in nature.

A solution to all of these overlapping problems came from the discovery of a previously unnoticed borderline case hidden in the mathematics of Goldstone's theorem, that under certain conditions it might theoretically be possible for a symmetry to be broken without disrupting gauge invariance and without any new massless particles or forces, and having "sensible" (renormalisable) results mathematically. This became known as the Higgs mechanism.

The Standard Model hypothesises a field which is responsible for this effect, called the Higgs field (symbol: ${\displaystyle \phi }$), which has the unusual property of a non-zero amplitude in its ground state; i.e., a non-zero vacuum expectation value. It can have this effect because of its unusual "Mexican hat" shaped potential whose lowest "point" is not at its "centre". In simple terms, unlike all other known fields, the Higgs field requires less energy to have a non-zero value than a zero value, so it ends up having a non-zero value everywhere. Below a certain extremely high energy level the existence of this non-zero vacuum expectation spontaneously breaks electroweak gauge symmetry which in turn gives rise to the Higgs mechanism and triggers the acquisition of mass by those particles interacting with the field. This effect occurs because scalar field components of the Higgs field are "absorbed" by the massive bosons as degrees of freedom, and couple to the fermions via Yukawa coupling, thereby producing the expected mass terms. When symmetry breaks under these conditions, the Goldstone bosons that arise interact with the Higgs field (and with other particles capable of interacting with the Higgs field) instead of becoming new massless particles. The intractable problems of both underlying theories "neutralise" each other, and the residual outcome is that elementary particles acquire a consistent mass based on how strongly they interact with the Higgs field. It is the simplest known process capable of giving mass to the gauge bosons while remaining compatible with gauge theories. Its quantum would be a scalar boson, known as the Higgs boson.

Simple explanation of the theory, from its origins in superconductivity

The proposed Higgs mechanism arose as a result of theories proposed to explain observations in superconductivity. A superconductor does not allow penetration by external magnetic fields (the Meissner effect). This strange observation implies that somehow, the electromagnetic field becomes short ranged during this phenomenon. Successful theories arose to explain this during the 1950s, first for fermions (Ginzburg–Landau theory, 1950), and then for bosons (BCS theory, 1957).

In these theories, superconductivity is interpreted as arising from a charged condensate field. Initially, the condensate value does not have any preferred direction, implying it is scalar, but its phase is capable of defining a gauge, in gauge based field theories. To do this, the field must be charged. A charged scalar field must also be complex (or described another way, it contains at least two components, and a symmetry capable of rotating each into the other(s)). In naïve gauge theory, a gauge transformation of a condensate usually rotates the phase. But in these circumstances, it instead fixes a preferred choice of phase. However it turns out that fixing the choice of gauge so that the condensate has the same phase everywhere, also causes the electromagnetic field to gain an extra term. This extra term causes the electromagnetic field to become short range.

Once attention was drawn to this theory within particle physics, the parallels were clear. A change of the usually long range electromagnetic field to become short ranged, within a gauge invariant theory, was exactly the needed effect sought for the weak force bosons (because a long range force has massless gauge bosons, and a short ranged force implies massive gauge bosons, suggesting that a result of this interaction is that the field's gauge bosons acquired mass, or an similar and equivalent effect). The features of a field required to do this was also quite well defined – it would have to be a charged scalar field, with at least two components, and complex in order to support a symmetry able to rotate these into each other.

(Goldstone's theorem also plays a role in such theories. The connection is technically, when a condensate breaks a symmetry, then the state reached by acting with a symmetry generator on the condensate has the same energy as before. This means that some kinds of oscillation will not involve change of energy. Oscillations with unchanged energy imply that excitations (particles) associated with the oscillation are massless. Therefore the outcome is that new massless particles should exist, known as Goldstone bosons. Because zero mass gauge bosons always mediate long range interactions, a new long range force should exist as well.)

Alternative models

The Minimal Standard Model as described above is the simplest known model for the Higgs mechanism with just one Higgs field. However, an extended Higgs sector with additional Higgs particle doublets or triplets is also possible, and many extensions of the Standard Model have this feature. The non-minimal Higgs sector favoured by theory are the two-Higgs-doublet models (2HDM), which predict the existence of a quintet of scalar particles: two CP-even neutral Higgs bosons h and H, a CP-odd neutral Higgs boson A, and two charged Higgs particles H. Supersymmetry ("SUSY") also predicts relations between the Higgs-boson masses and the masses of the gauge bosons, and could accommodate a 125 GeV/c neutral Higgs boson.

The key method to distinguish between these different models involves study of the particles' interactions ("coupling") and exact decay processes ("branching ratios"), which can be measured and tested experimentally in particle collisions. In the Type-I 2HDM model one Higgs doublet couples to up and down quarks, while the second doublet does not couple to quarks. This model has two interesting limits, in which the lightest Higgs couples to just fermions ("gauge-phobic") or just gauge bosons ("fermiophobic"), but not both. In the Type-II 2HDM model, one Higgs doublet only couples to up-type quarks, the other only couples to down-type quarks. The heavily researched Minimal Supersymmetric Standard Model (MSSM) includes a Type-II 2HDM Higgs sector, so it could be disproven by evidence of a Type-I 2HDM Higgs.

In other models the Higgs scalar is a composite particle. For example, in technicolor the role of the Higgs field is played by strongly bound pairs of fermions called techniquarks. Other models feature pairs of top quarks (see top quark condensate). In yet other models, there is no Higgs field at all and the electroweak symmetry is broken using extra dimensions.

Further theoretical issues and hierarchy problem

The Standard Model leaves the mass of the Higgs boson as a parameter to be measured, rather than a value to be calculated. This is seen as theoretically unsatisfactory, particularly as quantum corrections (related to interactions with virtual particles) should apparently cause the Higgs particle to have a mass immensely higher than that observed, but at the same time the Standard Model requires a mass of the order of 100 to 1000 GeV to ensure unitarity (in this case, to unitarise longitudinal vector boson scattering). Reconciling these points appears to require explaining why there is an almost-perfect cancellation resulting in the visible mass of ~ 125 GeV, and it is not clear how to do this. Because the weak force is about 10 times stronger than gravity, and (linked to this) the Higgs boson's mass is so much less than the Planck mass or the grand unification energy, it appears that either there is some underlying connection or reason for these observations which is unknown and not described by the Standard Model, or some unexplained and extremely precise fine-tuning of parameters – however at present neither of these explanations is proven. This is known as a hierarchy problem. More broadly, the hierarchy problem amounts to the worry that a future theory of fundamental particles and interactions should not have excessive fine-tunings or unduly delicate cancellations, and should allow masses of particles such as the Higgs boson to be calculable. The problem is in some ways unique to spin-0 particles (such as the Higgs boson), which can give rise to issues related to quantum corrections that do not affect particles with spin. A number of solutions have been proposed, including supersymmetry, conformal solutions and solutions via extra dimensions such as braneworld models.

There are also issues of quantum triviality, which suggests that it may not be possible to create a consistent quantum field theory involving elementary scalar particles. However, if quantum triviality is avoided, triviality constraints may set bounds on the Higgs Boson mass.

Properties

Properties of the Higgs field

In the Standard Model, the Higgs field is a scalar tachyonic field – scalar meaning it does not transform under Lorentz transformations, and tachyonic meaning the field (but not the particle) has imaginary mass, and in certain configurations must undergo symmetry breaking. It consists of four components: Two neutral ones and two charged component fields. Both of the charged components and one of the neutral fields are Goldstone bosons, which act as the longitudinal third-polarisation components of the massive W, W, and Z bosons. The quantum of the remaining neutral component corresponds to (and is theoretically realised as) the massive Higgs boson. This component can interact with fermions via Yukawa coupling to give them mass as well.

Mathematically, the Higgs field has imaginary mass and is therefore a tachyonic field. While tachyons (particles that move faster than light) are a purely hypothetical concept, fields with imaginary mass have come to play an important role in modern physics. Under no circumstances do any excitations ever propagate faster than light in such theories – the presence or absence of a tachyonic mass has no effect whatsoever on the maximum velocity of signals (there is no violation of causality). Instead of faster-than-light particles, the imaginary mass creates an instability: Any configuration in which one or more field excitations are tachyonic must spontaneously decay, and the resulting configuration contains no physical tachyons. This process is known as tachyon condensation, and is now believed to be the explanation for how the Higgs mechanism itself arises in nature, and therefore the reason behind electroweak symmetry breaking.

Although the notion of imaginary mass might seem troubling, it is only the field, and not the mass itself, that is quantised. Therefore, the field operators at spacelike separated points still commute (or anticommute), and information and particles still do not propagate faster than light. Tachyon condensation drives a physical system that has reached a local limit – and might naively be expected to produce physical tachyons – to an alternate stable state where no physical tachyons exist. Once a tachyonic field such as the Higgs field reaches the minimum of the potential, its quanta are not tachyons any more but rather are ordinary particles such as the Higgs boson.

Properties of the Higgs boson

This section needs to be updated. The reason given is: With the Higgs boson now empirically confirmed, the paragraphs on the mass should be rephrased to make it clear that they are about what could be predicted before that observation. Please help update this article to reflect recent events or newly available information. (July 2018)

Since the Higgs field is scalar, the Higgs boson has no spin. The Higgs boson is also its own antiparticle, is CP-even, and has zero electric and colour charge.

The Standard Model does not predict the mass of the Higgs boson. If that mass is between 115 and 180 GeV/c (consistent with empirical observations of 125 GeV/c), then the Standard Model can be valid at energy scales all the way up to the Planck scale (10 GeV). It should be the only particle in the Standard Model that remains massive even at high energies. Many theorists expect new physics beyond the Standard Model to emerge at the TeV-scale, based on unsatisfactory properties of the Standard Model. The highest possible mass scale allowed for the Higgs boson (or some other electroweak symmetry breaking mechanism) is 1.4 TeV; beyond this point, the Standard Model becomes inconsistent without such a mechanism, because unitarity is violated in certain scattering processes.

It is also possible, although experimentally difficult, to estimate the mass of the Higgs boson indirectly. In the Standard Model, the Higgs boson has a number of indirect effects; most notably, Higgs loops result in tiny corrections to masses of the W and Z bosons. Precision measurements of electroweak parameters, such as the Fermi constant and masses of the W and Z bosons, can be used to calculate constraints on the mass of the Higgs. As of July 2011, the precision electroweak measurements tell us that the mass of the Higgs boson is likely to be less than about 161 GeV/c at 95% confidence level. These indirect constraints rely on the assumption that the Standard Model is correct. It may still be possible to discover a Higgs boson above these masses, if it is accompanied by other particles beyond those accommodated by the Standard Model.

The LHC cannot directly measure the Higgs boson's lifetime, due to its extreme brevity. It is predicted as 1.56×10 s based on the predicted decay width of 4.07×10 GeV. However it can be measured indirectly, based upon comparing masses measured from quantum phenomena known as "on shelf" and extremely rare "off shelf" production pathways, derived from Dalitz decay via a virtual photon (H→γ*γ→ℓℓγ). Using this technique, the lifetime of the Higgs boson was tentatively measured in 2021 as 1.2 - 4.6 x 10 s, at sigma 3.2 (1 in 1000) significance.

Production

Feynman diagrams for Higgs production

Gluon fusion	Higgs Strahlung
Vector boson fusion	Top fusion

If Higgs particle theories are valid, then a Higgs particle can be produced much like other particles that are studied, in a particle collider. This involves accelerating a large number of particles to extremely high energies and extremely close to the speed of light, then allowing them to smash together. Protons and lead ions (the bare nuclei of lead atoms) are used at the LHC. In the extreme energies of these collisions, the desired esoteric particles will occasionally be produced and this can be detected and studied; any absence or difference from theoretical expectations can also be used to improve the theory. The relevant particle theory (in this case the Standard Model) will determine the necessary kinds of collisions and detectors. The Standard Model predicts that Higgs bosons could be formed in a number of ways, although the probability of producing a Higgs boson in any collision is always expected to be very small – for example, only one Higgs boson per 10 billion collisions in the Large Hadron Collider. The most common expected processes for Higgs boson production are:

Gluon fusion

If the collided particles are hadrons such as the proton or antiproton – as is the case in the LHC and Tevatron – then it is most likely that two of the gluons binding the hadron together collide. The easiest way to produce a Higgs particle is if the two gluons combine to form a loop of virtual quarks. Since the coupling of particles to the Higgs boson is proportional to their mass, this process is more likely for heavy particles. In practice it is enough to consider the contributions of virtual top and bottom quarks (the heaviest quarks). This process is the dominant contribution at the LHC and Tevatron being about ten times more likely than any of the other processes.

Higgs Strahlung

If an elementary fermion collides with an anti-fermion – e.g., a quark with an anti-quark or an electron with a positron – the two can merge to form a virtual W or Z boson which, if it carries sufficient energy, can then emit a Higgs boson. This process was the dominant production mode at the LEP, where an electron and a positron collided to form a virtual Z boson, and it was the second largest contribution for Higgs production at the Tevatron. At the LHC this process is only the third largest, because the LHC collides protons with protons, making a quark-antiquark collision less likely than at the Tevatron. Higgs Strahlung is also known as associated production.

Weak boson fusion

Another possibility when two (anti-)fermions collide is that the two exchange a virtual W or Z boson, which emits a Higgs boson. The colliding fermions do not need to be the same type. So, for example, an up quark may exchange a Z boson with an anti-down quark. This process is the second most important for the production of Higgs particle at the LHC and LEP.

Top fusion

The final process that is commonly considered is by far the least likely (by two orders of magnitude). This process involves two colliding gluons, which each decay into a heavy quark–antiquark pair. A quark and antiquark from each pair can then combine to form a Higgs particle.

Decay

Quantum mechanics predicts that if it is possible for a particle to decay into a set of lighter particles, then it will eventually do so. This is also true for the Higgs boson. The likelihood with which this happens depends on a variety of factors including: the difference in mass, the strength of the interactions, etc. Most of these factors are fixed by the Standard Model, except for the mass of the Higgs boson itself. For a Higgs boson with a mass of 125 GeV/c the SM predicts a mean life time of about 1.6×10 s.

Since it interacts with all the massive elementary particles of the SM, the Higgs boson has many different processes through which it can decay. Each of these possible processes has its own probability, expressed as the branching ratio; the fraction of the total number decays that follows that process. The SM predicts these branching ratios as a function of the Higgs mass (see plot).

One way that the Higgs can decay is by splitting into a fermion–antifermion pair. As general rule, the Higgs is more likely to decay into heavy fermions than light fermions, because the mass of a fermion is proportional to the strength of its interaction with the Higgs. By this logic the most common decay should be into a top–antitop quark pair. However, such a decay would only be possible if the Higgs were heavier than ~346 GeV/c, twice the mass of the top quark. For a Higgs mass of 125 GeV/c the SM predicts that the most common decay is into a bottom–antibottom quark pair, which happens 57.7% of the time. The second most common fermion decay at that mass is a tau–antitau pair, which happens only about 6.3% of the time.

Another possibility is for the Higgs to split into a pair of massive gauge bosons. The most likely possibility is for the Higgs to decay into a pair of W bosons (the light blue line in the plot), which happens about 21.5% of the time for a Higgs boson with a mass of 125 GeV/c. The W bosons can subsequently decay either into a quark and an antiquark or into a charged lepton and a neutrino. The decays of W bosons into quarks are difficult to distinguish from the background, and the decays into leptons cannot be fully reconstructed (because neutrinos are impossible to detect in particle collision experiments). A cleaner signal is given by decay into a pair of Z-bosons (which happens about 2.6% of the time for a Higgs with a mass of 125 GeV/c), if each of the bosons subsequently decays into a pair of easy-to-detect charged leptons (electrons or muons).

Decay into massless gauge bosons (i.e., gluons or photons) is also possible, but requires intermediate loop of virtual heavy quarks (top or bottom) or massive gauge bosons. The most common such process is the decay into a pair of gluons through a loop of virtual heavy quarks. This process, which is the reverse of the gluon fusion process mentioned above, happens approximately 8.6% of the time for a Higgs boson with a mass of 125 GeV/c. Much rarer is the decay into a pair of photons mediated by a loop of W bosons or heavy quarks, which happens only twice for every thousand decays. However, this process is very relevant for experimental searches for the Higgs boson, because the energy and momentum of the photons can be measured very precisely, giving an accurate reconstruction of the mass of the decaying particle.

In 2021 the extremely rare Dalitz decay was tentatively observed, into two leptons (electrons or muons) and a photon (ℓℓγ), via virtual photon decay. This can happen in three ways; Higgs to virtual photon to ℓℓγ in which the virtual photon (γ*) has very small but nonzero mass, Higgs to Z boson to ℓℓγ, or Higgs to two leptons, one of which emits a final-state photon leading to ℓℓγ. ATLAS searched for evidence of the first of these (H→γ*γ→ℓℓγ) at low di-lepton mass (≤ 30 GeV), where this process should dominate. The observation is at sigma 3.2 (1 in 1000) significance. This decay path is important because it facilitates measuring the on- and off-shelf mass of the Higgs boson (allowing indirect measurement of decay time), and the decay into two charged particles allows exploration of charge conjugation and charge parity (CP) violation.

Public discussion

Naming

Names used by physicists

The name most strongly associated with the particle and field is the Higgs boson and Higgs field. For some time the particle was known by a combination of its PRL author names (including at times Anderson), for example the Brout–Englert–Higgs particle, the Anderson-Higgs particle, or the Englert–Brout–Higgs–Guralnik–Hagen–Kibble mechanism, and these are still used at times. Fuelled in part by the issue of recognition and a potential shared Nobel Prize, the most appropriate name was still occasionally a topic of debate until 2013. Higgs himself prefers to call the particle either by an acronym of all those involved, or "the scalar boson", or "the so-called Higgs particle".

A considerable amount has been written on how Higgs' name came to be exclusively used. Two main explanations are offered. The first is that Higgs undertook a step which was either unique, clearer or more explicit in his paper in formally predicting and examining the particle. Of the PRL papers' authors, only the paper by Higgs explicitly offered as a prediction that a massive particle would exist and calculated some of its properties; he was therefore "the first to postulate the existence of a massive particle" according to Nature. Physicist and author Frank Close and physicist-blogger Peter Woit both comment that the paper by GHK was also completed after Higgs and Brout–Englert were submitted to Physical Review Letters, and that Higgs alone had drawn attention to a predicted massive scalar boson, while all others had focused on the massive vector bosons. In this way, Higgs' contribution also provided experimentalists with a crucial "concrete target" needed to test the theory.

However, in Higgs' view, Brout and Englert did not explicitly mention the boson since its existence is plainly obvious in their work, while according to Guralnik the GHK paper was a complete analysis of the entire symmetry breaking mechanism whose mathematical rigour is absent from the other two papers, and a massive particle may exist in some solutions. Higgs' paper also provided an "especially sharp" statement of the challenge and its solution according to science historian David Kaiser.

The alternative explanation is that the name was popularised in the 1970s due to its use as a convenient shorthand or because of a mistake in citing. Many accounts (including Higgs' own) credit the "Higgs" name to physicist Benjamin Lee. Lee was a significant popularizer of the theory in its early days, and habitually attached the name "Higgs" as a "convenient shorthand" for its components from 1972. and in at least one instance from as early as 1966. Although Lee clarified in his footnotes that "'Higgs' is an abbreviation for Higgs, Kibble, Guralnik, Hagen, Brout, Englert", his use of the term (and perhaps also Steven Weinberg's mistaken cite of Higgs' paper as the first in his seminal 1967 paper) meant that by around 1975–1976 others had also begun to use the name 'Higgs' exclusively as a shorthand. In 2012, physicist Frank Wilczek, who was credited for naming the elementary particle, the axion (over an alternative proposal "Higglet", by Weinberg), endorsed the "Higgs boson" name, stating "History is complicated, and wherever you draw the line, there will be somebody just below it."

Nickname

The Higgs boson is often referred to as the "God particle" in popular media outside the scientific community. The nickname comes from the title of the 1993 book on the Higgs boson and particle physics, The God Particle: If the Universe Is the Answer, What Is the Question? by Physics Nobel Prize winner and Fermilab director Leon Lederman. Lederman wrote it in the context of failing US government support for the Superconducting Super Collider, a partially constructed titanic competitor to the Large Hadron Collider with planned collision energies of 2 × 20 TeV that was championed by Lederman since its 1983 inception and shut down in 1993. The book sought in part to promote awareness of the significance and need for such a project in the face of its possible loss of funding. Lederman, a leading researcher in the field, writes that he wanted to title his book The Goddamn Particle: If the Universe is the Answer, What is the Question? Lederman's editor decided that the title was too controversial and convinced him to change the title to The God Particle: If the Universe is the Answer, What is the Question?

While media use of this term may have contributed to wider awareness and interest, many scientists feel the name is inappropriate since it is sensational hyperbole and misleads readers; the particle also has nothing to do with any God, leaves open numerous questions in fundamental physics, and does not explain the ultimate origin of the universe. Higgs, an atheist, was reported to be displeased and stated in a 2008 interview that he found it "embarrassing" because it was "the kind of misuse ... which I think might offend some people". The nickname has been satirised in mainstream media as well. Science writer Ian Sample stated in his 2010 book on the search that the nickname is "universally hate" by physicists and perhaps the "worst derided" in the history of physics, but that (according to Lederman) the publisher rejected all titles mentioning "Higgs" as unimaginative and too unknown.

Lederman begins with a review of the long human search for knowledge, and explains that his tongue-in-cheek title draws an analogy between the impact of the Higgs field on the fundamental symmetries at the Big Bang, and the apparent chaos of structures, particles, forces and interactions that resulted and shaped our present universe, with the biblical story of Babel in which the primordial single language of early Genesis was fragmented into many disparate languages and cultures.

Today ... we have the standard model, which reduces all of reality to a dozen or so particles and four forces ... It's a hard-won simplicity remarkably accurate. But it is also incomplete and, in fact, internally inconsistent ... This boson is so central to the state of physics today, so crucial to our final understanding of the structure of matter, yet so elusive, that I have given it a nickname: the God Particle. Why God Particle? Two reasons. One, the publisher wouldn't let us call it the Goddamn Particle, though that might be a more appropriate title, given its villainous nature and the expense it is causing. And two, there is a connection, of sorts, to another book, a much older one ...

— Lederman & Teresi The God Particle: If the Universe is the Answer, What is the Question

Lederman asks whether the Higgs boson was added just to perplex and confound those seeking knowledge of the universe, and whether physicists will be confounded by it as recounted in that story, or ultimately surmount the challenge and understand "how beautiful is the universe made".

Other proposals

A renaming competition by British newspaper The Guardian in 2009 resulted in their science correspondent choosing the name "the champagne bottle boson" as the best submission: "The bottom of a champagne bottle is in the shape of the Higgs potential and is often used as an illustration in physics lectures. So it's not an embarrassingly grandiose name, it is memorable, and has some physics connection too." The name Higgson was suggested as well, in an opinion piece in the Institute of Physics' online publication physicsworld.com.

Educational explanations and analogies

There has been considerable public discussion of analogies and explanations for the Higgs particle and how the field creates mass, including coverage of explanatory attempts in their own right and a competition in 1993 for the best popular explanation by then-UK Minister for Science Sir William Waldegrave and articles in newspapers worldwide.

An educational collaboration involving an LHC physicist and a High School Teachers at CERN educator suggests that dispersion of light – responsible for the rainbow and dispersive prism – is a useful analogy for the Higgs field's symmetry breaking and mass-causing effect.

Matt Strassler uses electric fields as an analogy:

Some particles interact with the Higgs field while others don't. Those particles that feel the Higgs field act as if they have mass. Something similar happens in an electric field – charged objects are pulled around and neutral objects can sail through unaffected. So you can think of the Higgs search as an attempt to make waves in the Higgs field to prove it's really there.

A similar explanation was offered by The Guardian:

The Higgs boson is essentially a ripple in a field said to have emerged at the birth of the universe and to span the cosmos to this day... The particle is crucial however: It is the smoking gun, the evidence required to show the theory is right.

The Higgs field's effect on particles was famously described by physicist David Miller as akin to a room full of political party workers spread evenly throughout a room: The crowd gravitates to and slows down famous people but does not slow down others. He also drew attention to well-known effects in solid state physics where an electron's effective mass can be much greater than usual in the presence of a crystal lattice.

Analogies based on drag effects, including analogies of "syrup" or "molasses" are also well known, but can be somewhat misleading since they may be understood (incorrectly) as saying that the Higgs field simply resists some particles' motion but not others' – a simple resistive effect could also conflict with Newton's third law.

Recognition and awards

There was considerable discussion prior to late 2013 of how to allocate the credit if the Higgs boson is proven, made more pointed as a Nobel prize had been expected, and the very wide basis of people entitled to consideration. These include a range of theoreticians who made the Higgs mechanism theory possible, the theoreticians of the 1964 PRL papers (including Higgs himself), the theoreticians who derived from these a working electroweak theory and the Standard Model itself, and also the experimentalists at CERN and other institutions who made possible the proof of the Higgs field and boson in reality. The Nobel prize has a limit of three persons to share an award, and some possible winners are already prize holders for other work, or are deceased (the prize is only awarded to persons in their lifetime). Existing prizes for works relating to the Higgs field, boson, or mechanism include:

• Nobel Prize in Physics (1979) – Glashow, Salam, and Weinberg, for contributions to the theory of the unified weak and electromagnetic interaction between elementary particles
• Nobel Prize in Physics (1999) – 't Hooft and Veltman, for elucidating the quantum structure of electroweak interactions in physics
• J. J. Sakurai Prize for Theoretical Particle Physics (2010) – Hagen, Englert, Guralnik, Higgs, Brout, and Kibble, for elucidation of the properties of spontaneous symmetry breaking in four-dimensional relativistic gauge theory and of the mechanism for the consistent generation of vector boson masses (for the 1964 papers described above)
• Wolf Prize (2004) – Englert, Brout, and Higgs
• Special Breakthrough Prize in Fundamental Physics (2013) – Fabiola Gianotti and Peter Jenni, spokespersons of the ATLAS Collaboration and Michel Della Negra, Tejinder Singh Virdee, Guido Tonelli, and Joseph Incandela spokespersons, past and present, of the CMS collaboration, "For leadership role in the scientific endeavour that led to the discovery of the new Higgs-like particle by the ATLAS and CMS collaborations at CERN's Large Hadron Collider".
• Nobel Prize in Physics (2013) – Peter Higgs and François Englert, for the theoretical discovery of a mechanism that contributes to our understanding of the origin of mass of subatomic particles, and which recently was confirmed through the discovery of the predicted fundamental particle, by the ATLAS and CMS experiments at CERN's Large Hadron Collider

Englert's co-researcher Robert Brout had died in 2011 and the Nobel Prize is not ordinarily given posthumously.

Additionally Physical Review Letters' 50-year review (2008) recognised the 1964 PRL symmetry breaking papers and Weinberg's 1967 paper A model of Leptons (the most cited paper in particle physics, as of 2012) "milestone Letters".

Following reported observation of the Higgs-like particle in July 2012, several Indian media outlets reported on the supposed neglect of credit to Indian physicist Satyendra Nath Bose after whose work in the 1920s the class of particles "bosons" is named (although physicists have described Bose's connection to the discovery as tenuous).

Technical aspects and mathematical formulation

In the Standard Model, the Higgs field is a four-component scalar field that forms a complex doublet of the weak isospin SU(2) symmetry:

${\displaystyle \phi ={\frac {1}{\sqrt {2}}}\left({\begin{array}{c}\phi ^{1}+i\phi ^{2}\\\phi ^{0}+i\phi ^{3}\end{array}}\right)\ ,}$

while the field has charge +⁠1/2⁠ under the weak hypercharge U(1) symmetry.

Note: This article uses the scaling convention where the electric charge, Q, the weak isospin, T₃, and the weak hypercharge, Y_W, are related by Q = T₃ + Y_W. A different convention used in most other Misplaced Pages articles is Q = T₃ + ⁠1/2⁠Y_W.

The Higgs part of the Lagrangian is

${\displaystyle {\mathcal {L}}_{\text{H}}=\left|\left(\partial _{\mu }-igW_{\mu \,a}{\tfrac {1}{2}}\sigma ^{a}-i{\tfrac {1}{2}}g'B_{\mu }\right)\phi \right|^{2}+\mu _{\text{H}}^{2}\phi ^{\dagger }\phi -\lambda \left(\phi ^{\dagger }\phi \right)^{2}\ ,}$

where ${\displaystyle W_{\mu \,a}}$ and ${\displaystyle B_{\mu }}$ are the gauge bosons of the SU(2) and U(1) symmetries, ${\displaystyle g}$ and ${\displaystyle g'}$ their respective coupling constants, ${\displaystyle \sigma ^{a}}$ are the Pauli matrices (a complete set generators of the SU(2) symmetry), and ${\displaystyle \lambda >0}$ and ${\displaystyle \mu _{\text{H}}^{2}>0}$, so that the ground state breaks the SU(2) symmetry (see figure).

The ground state of the Higgs field (the bottom of the potential) is degenerate with different ground states related to each other by a SU(2) gauge transformation. It is always possible to pick a gauge such that in the ground state ${\displaystyle \phi ^{1}=\phi ^{2}=\phi ^{3}=0}$. The expectation value of ${\displaystyle \phi ^{0}}$ in the ground state (the vacuum expectation value or VEV) is then ${\displaystyle \left\langle \phi ^{0}\right\rangle ={\tfrac {1}{\sqrt {2\,}}}v}$, where ${\displaystyle v={\tfrac {1}{\sqrt {\lambda \,}}}\left|\mu _{\text{H}}\right|}$. The measured value of this parameter is ~246 GeV/c. It has units of mass, and is the only free parameter of the Standard Model that is not a dimensionless number. Quadratic terms in ${\displaystyle W_{\mu }}$ and ${\displaystyle B_{\mu }}$ arise, which give masses to the W and Z bosons:

${\displaystyle {\begin{aligned}m_{\text{W}}&={\tfrac {1}{2}}v\left|\,g\,\right|\ ,\\m_{\text{Z}}&={\tfrac {1}{2}}v{\sqrt {g^{2}+{g'}^{2}\ }}\ ,\end{aligned}}}$

with their ratio determining the Weinberg angle, ${\textstyle \cos \theta _{\text{W}}={\frac {m_{\text{W}}}{\ m_{\text{Z}}\ }}={\frac {\left|\,g\,\right|}{\ {\sqrt {g^{2}+{g'}^{2}\ }}\ }}}$, and leave a massless U(1) photon, ${\displaystyle \gamma }$. The mass of the Higgs boson itself is given by

${\displaystyle m_{\text{H}}={\sqrt {2\mu _{\text{H}}^{2}\ }}\equiv {\sqrt {2\lambda v^{2}\ }}.}$

The quarks and the leptons interact with the Higgs field through Yukawa interaction terms:

${\displaystyle {\begin{aligned}{\mathcal {L}}_{\text{Y}}=&-\lambda _{u}^{i\,j}{\frac {\ \phi ^{0}-i\phi ^{3}\ }{\sqrt {2\ }}}{\overline {u}}_{\text{L}}^{i}u_{\text{R}}^{j}+\lambda _{u}^{i\,j}{\frac {\ \phi ^{1}-i\phi ^{2}\ }{\sqrt {2\ }}}{\overline {d}}_{\text{L}}^{i}u_{\text{R}}^{j}\\&-\lambda _{d}^{i\,j}{\frac {\ \phi ^{0}+i\phi ^{3}\ }{\sqrt {2\ }}}{\overline {d}}_{\text{L}}^{i}d_{\text{R}}^{j}-\lambda _{d}^{i\,j}{\frac {\ \phi ^{1}+i\phi ^{2}\ }{\sqrt {2\ }}}{\overline {u}}_{\text{L}}^{i}d_{\text{R}}^{j}\\&-\lambda _{e}^{i\,j}{\frac {\ \phi ^{0}+i\phi ^{3}\ }{\sqrt {2\ }}}{\overline {e}}_{\text{L}}^{i}e_{\text{R}}^{j}-\lambda _{e}^{i\,j}{\frac {\ \phi ^{1}+i\phi ^{2}\ }{\sqrt {2\ }}}{\overline {\nu }}_{\text{L}}^{i}e_{\text{R}}^{j}+{\textrm {h.c.}}\ ,\end{aligned}}}$

where ${\displaystyle (d,u,e,\nu )_{\text{L,R}}^{i}}$ are left-handed and right-handed quarks and leptons of the ith generation, ${\displaystyle \lambda _{\text{u,d,e}}^{i\,j}}$ are matrices of Yukawa couplings where h.c. denotes the hermitian conjugate of all the preceding terms. In the symmetry breaking ground state, only the terms containing ${\displaystyle \phi ^{0}}$ remain, giving rise to mass terms for the fermions. Rotating the quark and lepton fields to the basis where the matrices of Yukawa couplings are diagonal, one gets

${\displaystyle {\mathcal {L}}_{\text{m}}=-m_{\text{u}}^{i}{\overline {u}}_{\text{L}}^{i}u_{\text{R}}^{i}-m_{\text{d}}^{i}{\overline {d}}_{\text{L}}^{i}d_{\text{R}}^{i}-m_{\text{e}}^{i}{\overline {e}}_{\text{L}}^{i}e_{\text{R}}^{i}+{\textrm {h.c.}},}$

where the masses of the fermions are ${\displaystyle m_{\text{u,d,e}}^{i}={\tfrac {1}{\sqrt {2\ }}}\lambda _{\text{u,d,e}}^{i}v}$, and ${\displaystyle \lambda _{\text{u,d,e}}^{i}}$ denote the eigenvalues of the Yukawa matrices.

See also

Standard Model

• Higgs mechanism – Mechanism that explains the generation of mass for gauge bosons
• History of quantum field theory
• Introduction to quantum mechanics – Non-mathematical introduction
• Noncommutative standard model

  and noncommutative geometry – Branch of mathematics

• Mathematical formulation of the Standard Model – Mathematics of a particle physics model
  • Standard Model fields overview
  • mass terms and the Higgs mechanism
• Quantum gauge theory – Physical theory with fields invariant under the action of local "gauge" Lie groupsPages displaying short descriptions of redirect targets
• W and Z bosons – Bosons that mediate the weak interaction

Other

• Bose–Einstein statistics – Description of the behavior of bosons
• Dalitz plot – particle physics plotPages displaying wikidata descriptions as a fallback
• Particle Fever, a 2013 American documentary film following various LHC experiments and concluding with the identification of the Higgs boson
• Quantum triviality – Possible outcome of renormalization in physics
• Scalar boson – Boson with spin equal to zero
• Stueckelberg action – Special case of the abelian Higgs mechanism
• Tachyonic field – Field with an imaginary mass* ZZ diboson – subatomic particlesPages displaying wikidata descriptions as a fallback

Explanatory notes

1. Note that such events also occur due to other processes. Detection involves a statistically significant excess of such events at specific energies.
2. ^ In the Standard Model, the total decay width of a Higgs boson with a mass of 125 GeV/c is predicted to be 4.07×10 GeV. The mean lifetime is given by ${\displaystyle \tau =\hbar /\Gamma }$.
3. In Higgs based theories, the Higgs boson itself should be an exception, being massive even at high energies
4. In physics, it is possible for a law to hold true only if certain assumptions hold true, or when certain conditions are met. For example, Newton's laws of motion only apply at speeds where relativistic effects are negligible; and laws related to conductivity, gases, and classical physics (as opposed to quantum mechanics) may apply only within certain ranges of size, temperature, pressure, or other conditions.
5. ^ The success of the Higgs-based electroweak theory and Standard Model is illustrated by their predictions of the mass of two particles later detected: the W boson (predicted mass: 80.390 ± 0.018 GeV, experimental measurement: 80.387 ± 0.019 GeV), and the Z boson (predicted mass: 91.1874 ± 0.0021, experimental measurement: 91.1876 ± 0.0021 GeV). Other accurate predictions included the weak neutral current, the gluon, and the top and charm quarks, all later proven to exist as the theory said.
6. Electroweak symmetry is broken by the Higgs field in its lowest energy state, called its ground state. At high energy levels this does not happen, and the gauge bosons of the weak force would be expected to become massless above those energy levels.
7. The range of a force is inversely proportional to the mass of the particles transmitting it. In the Standard Model, forces are carried by virtual particles. The movement and interactions of these particles with each other are limited by the energy–time uncertainty principle. As a result, the more massive a single virtual particle is, the greater its energy, and therefore the shorter the distance it can travel. A particle's mass therefore, determines the maximum distance at which it can interact with other particles and on any force it mediates. By the same token, the reverse is also true: massless and near-massless particles can carry long distance forces. (See also: Compton wavelength and static forces and virtual-particle exchange) Since experiments have shown that the weak force acts over only a very short range, this implies that massive gauge bosons must exist, and indeed, their masses have since been confirmed by measurement.
8. By the 1960s, many had already started to see gauge theories as failing to explain particle physics, because theorists had been unable to solve the mass problem or even explain how gauge theory could provide a solution. So the idea that the Standard Model – which relied on a Higgs field, not yet proved to exist – could be fundamentally incorrect, was not unreasonable. Against this, once the model was developed around 1972, no better theory existed, and its predictions and solutions were so accurate, that it became the preferred theory anyway. It then became crucial to science, to know whether it was correct.
9. For example: The Huffington Post / Reuters, and others.
10. The bubble's effects would be expected to propagate across the universe at the speed of light from wherever it occurred. However space is vast – with even the nearest galaxy being over 2 million light years from us, and others being many billions of light years distant, so the effect of such an event would be unlikely to arise here for billions of years after first occurring.
11. If the Standard Model is valid, then the particles and forces we observe in our universe exist as they do, because of underlying quantum fields. Quantum fields can have states of differing stability, including 'stable', 'unstable' and 'metastable' states (the latter remain stable unless sufficiently perturbed). If a more stable vacuum state were able to arise, then existing particles and forces would no longer arise as they presently do. Different particles or forces would arise from (and be shaped by) whatever new quantum states arose. The world we know depends upon these particles and forces, so if this happened, everything around us, from subatomic particles to galaxies, and all fundamental forces, would be reconstituted into new fundamental particles and forces and structures. The universe would potentially lose all of its present structures and become inhabited by new ones (depending upon the exact states involved) based upon the same quantum fields.
12. ^ Goldstone's theorem only applies to gauges having manifest Lorentz covariance, a condition that took time to become questioned. But the process of quantisation requires a gauge to be fixed and at this point it becomes possible to choose a gauge such as the 'radiation' gauge which is not invariant over time, so that these problems can be avoided. According to Bernstein (1974), p. 8:

    the "radiation gauge" condition ∇⋅A(x) = 0 is clearly not covariant, which means that if we wish to maintain transversality of the photon in all Lorentz frames, the photon field A_μ(x) cannot transform like a four-vector. This is no catastrophe, since the photon field is not an observable, and one can readily show that the S-matrix elements, which are observable have covariant structures. ... in gauge theories one might arrange things so that one had a symmetry breakdown because of the noninvariance of the vacuum; but, because the Goldstone et al. proof breaks down, the zero mass Goldstone mesons need not appear.

    Bernstein (1974) contains an accessible and comprehensive background and review of this area, see external links.
13. A field with the "Mexican hat" potential ${\displaystyle V(\phi )=\mu ^{2}\phi ^{2}+\lambda \phi ^{4}}$ and ${\displaystyle \mu ^{2}<0}$ has a minimum not at zero but at some non-zero value ${\displaystyle \phi _{0}}$. By expressing the action in terms of the field ${\displaystyle {\tilde {\phi }}=\phi -\phi _{0}}$ (where ${\displaystyle \phi _{0}}$ is a constant independent of position), we find the Yukawa term has a component ${\displaystyle g\phi _{0}{\bar {\psi }}\psi }$. Since both g and ${\displaystyle \phi _{0}}$ are constants, this looks exactly like the mass term for a fermion of mass ${\displaystyle g\phi _{0}}$. The field ${\displaystyle {\tilde {\phi }}}$ is then the Higgs field.
14. ^ The example is based on the production rate at the LHC operating at 7 TeV. The total cross-section for producing a Higgs boson at the LHC is about 10 picobarn, while the total cross-section for a proton–proton collision is 110 millibarn.
15. Just before LEP's shut down, some events that hinted at a Higgs were observed, but it was not judged significant enough to extend its run and delay construction of the LHC.
16. ^ ATLAS and CMS only just co-discovered this particle in July... We will not know after today whether it is a Higgs at all, whether it is a Standard Model Higgs or not, or whether any particular speculative idea... is now excluded... Knowledge about nature does not come easy. We discovered the top quark in 1995, and we are still learning about its properties today... we will still be learning important things about the Higgs during the coming few decades. We've no choice but to be patient. — M. Strassler (2012)
17. Announced in articles in Time, Forbes, Slate, NPR, and others.
18. In the Standard Model, the mass term arising from the Dirac Lagrangian for any fermion ${\displaystyle \psi }$ is ${\displaystyle -m{\bar {\psi }}\psi }$. This is not invariant under the electroweak symmetry, as can be seen by writing ${\displaystyle \psi }$ in terms of left and right handed components:

    ${\displaystyle -m{\bar {\psi }}\psi \,=\,-m\left({\bar {\psi }}_{L}\psi _{R}+{\bar {\psi }}_{R}\psi _{L}\right)}$

    i.e., contributions from ${\displaystyle {\bar {\psi }}_{L}\psi _{L}}$ and ${\displaystyle {\bar {\psi }}_{R}\psi _{R}}$ terms do not appear. We see that the mass-generating interaction is achieved by constant flipping of particle chirality. Since the spin-half particles have no right/left helicity pair with the same SU(2) and SU(3) representation and the same weak hypercharge, then assuming these gauge charges are conserved in the vacuum, none of the spin-half particles could ever swap helicity. Therefore, in the absence of some other cause, all fermions must be massless.
19. This upper limit would increase to 185 GeV/c if the lower bound of 114.4 GeV/c from the LEP-2 direct search is allowed for.
20. Other names have included:
    • The "Anderson–Higgs" mechanism,
    • "Higgs–Kibble" mechanism (by Abdus Salam) and
    • "A-B-E-G-H-H-K-'tH" mechanism (by Peter Higgs).
21. Benjamin W. Lee also uses the Korean language name Lee Whi-soh.
22. Examples of early papers using the term "Higgs boson" include
    • Ellis, Gaillard, & Nanopoulos (1976) "A phenomenological profile of the Higgs boson".
    • Bjorken (1977) "Weak interaction theory and neutral currents".
    • Wienberg (received, 1975) "Mass of the Higgs boson".
23. Global financial partnerships could be the only way to salvage such a project. Some feel that Congress delivered a fatal blow.
    'We have to keep the momentum and optimism and start thinking about international collaboration,' said Leon M. Lederman, the Nobel Prize-winning physicist who was the architect of the super collider plan.
24. In Miller's analogy, the Higgs field is compared to political party workers spread evenly throughout a room. There will be some people (in Miller's example an anonymous person) who pass through the crowd with ease, paralleling the interaction between the field and particles that do not interact with it, such as massless photons. There will be other people (in Miller's example the British prime minister) who would find their progress being continually slowed by the swarm of admirers crowding around, paralleling the interaction for particles that do interact with the field and by doing so, acquire a finite mass.

References

Citations

1. P.A. Zyla; et al. (Particle Data Group) (2020). "Higgs Boson" (PDF). Progress of Theoretical and Experimental Physics: 1. Archived (PDF) from the original on 23 March 2021. Retrieved 13 January 2021.
2. ^ LHC Higgs Cross Section Working Group; Dittmaier; Mariotti; Passarino; Tanaka; Alekhin; Alwall; Bagnaschi; Banfi (2012). "Handbook of LHC Higgs Cross Sections: 2. Differential Distributions". CERN Report 2 (Tables A.1 – A.20). 1201: 3084. arXiv:1201.3084. Bibcode:2012arXiv1201.3084L. doi:10.5170/CERN-2012-002. S2CID 119287417.
3. ^ "Life of the Higgs boson". CMS Collaboration. Archived from the original on 2 December 2021. Retrieved 21 January 2021.
4. ^ "ATLAS finds evidence of a rare Higgs boson decay". CERN. 8 February 2021. Archived from the original on 19 January 2022. Retrieved 21 January 2022.
5. ATLAS collaboration (2018). "Observation of H→bb decays and VH production with the ATLAS detector". Physics Letters B. 786: 59–86. arXiv:1808.08238. doi:10.1016/j.physletb.2018.09.013. S2CID 53658301.
6. CMS collaboration (2018). "Observation of Higgs Boson Decay to Bottom Quarks". Physical Review Letters. 121 (12): 121801. arXiv:1808.08242. Bibcode:2018PhRvL.121l1801S. doi:10.1103/PhysRevLett.121.121801. PMID 30296133. S2CID 118901756.
7. ^ O'Luanaigh, C. (14 March 2013). "New results indicate that new particle is a Higgs boson". CERN. Archived from the original on 20 October 2015. Retrieved 9 October 2013.
8. ^ CMS Collaboration (2017). "Constraints on anomalous Higgs boson couplings using production and decay information in the four-lepton final state". Physics Letters B. 775 (2017): 1–24. arXiv:1707.00541. Bibcode:2017PhLB..775....1S. doi:10.1016/j.physletb.2017.10.021. S2CID 3221363.
9. Goulette, Marc (15 August 2012). "What should we know about the Higgs particle?". Atlas Experiment/CERN. Archived from the original on 13 January 2022. Retrieved 21 January 2022.
10. "Getting to know the Higgs particle: new discoveries!". Institute of Physics. Archived from the original on 13 January 2022. Retrieved 21 January 2022.
11. ^ Onyisi, P. (23 October 2012). "Higgs boson FAQ". University of Texas ATLAS group. Archived from the original on 12 October 2013. Retrieved 8 January 2013.
12. ^ Strassler, M. (12 October 2012). "The Higgs FAQ 2.0". ProfMattStrassler.com. Archived from the original on 12 October 2013. Retrieved 8 January 2013. Why do particle physicists care so much about the Higgs particle?
    Well, actually, they don't. What they really care about is the Higgs field, because it is so important.
13. ^ Adam Falkowski (writing as 'Jester') (27 February 2013). "When shall we call it Higgs?". Résonaances particle physics blog. Archived from the original on 29 June 2017. Retrieved 7 March 2013.
14. Lederman, Leon M. (1993). The God Particle. Bantam Doubleday Dell. ISBN 0-385-31211-3.
15. ^ Sample, Ian (29 May 2009). "Anything but the God particle". The Guardian. Archived from the original on 25 July 2018. Retrieved 24 June 2009.
16. ^ Evans, R. (14 December 2011). "The Higgs boson: Why scientists hate that you call it the 'God particle'". National Post. Archived from the original on 23 February 2015. Retrieved 3 November 2013.
17. Griffiths 2008, pp. 49–52
18. Tipler & Llewellyn 2003, pp. 603–604
19. From P.W. Anderson, "More is different", Science, 1972.
20. Griffiths 2008, pp. 372–373
21. ^ Woit, Peter (13 November 2010). "The Anderson–Higgs Mechanism". Dr. Peter Woit (Senior Lecturer in Mathematics Columbia University and Ph.D. particle physics). Archived from the original on 23 November 2012. Retrieved 12 November 2012.
22. Shu, F. H. (1982). The Physical Universe: An Introduction to Astronomy. University Science Books. pp. 107–108. ISBN 978-0-935702-05-7. Archived from the original on 29 June 2016. Retrieved 27 June 2015.
23. ^ José Luis Lucio; Arnulfo Zepeda (1987). Proceedings of the II Mexican School of Particles and Fields, Cuernavaca-Morelos, 1986. World Scientific. p. 29. ISBN 978-9971504342. Archived from the original on 25 January 2022. Retrieved 5 September 2020.
24. ^ Gunion; Dawson; Kane; Haber (1990). The Higgs Hunter's Guide (1st ed.). p. 11. ISBN 978-0-2015-0935-9. Archived from the original on 25 January 2022. Retrieved 5 September 2020. Cited by Peter Higgs in his talk "My Life as a Boson", 2001, ref#25.
25. ^ Lederman, Leon M.; Teresi, Dick (1993). The God Particle: If the Universe is the Answer, What is the Question. Houghton Mifflin Company. ISBN 9780395558492.
26. Strassler, M. (8 October 2011). "The Known Particles – If The Higgs Field Were Zero". ProfMattStrassler.com. Archived from the original on 17 March 2021. Retrieved 13 November 2012. The Higgs field: so important it merited an entire experimental facility, the Large Hadron Collider, dedicated to understanding it.
27. ^ Biever, C. (6 July 2012). "It's a boson! But we need to know if it's the Higgs". New Scientist. Retrieved 9 January 2013. 'As a layman, I would say, I think we have it,' said Rolf-Dieter Heuer, director general of CERN at Wednesday's seminar announcing the results of the search for the Higgs boson. But when pressed by journalists afterwards on what exactly 'it' was, things got more complicated. 'We have discovered a boson – now we have to find out what boson it is'
    Q: 'If we don't know the new particle is a Higgs, what do we know about it?' We know it is some kind of boson, says Vivek Sharma of CMS
    Q: 'are the CERN scientists just being too cautious? What would be enough evidence to call it a Higgs boson?' As there could be many different kinds of Higgs bosons, there's no straight answer.
    
28. Siegfried, T. (20 July 2012). "Higgs Hysteria". Science News. Archived from the original on 31 October 2012. Retrieved 9 December 2012. In terms usually reserved for athletic achievements, news reports described the finding as a monumental milestone in the history of science.
29. ^ Del Rosso, A. (19 November 2012). "Higgs: The beginning of the exploration". CERN. Archived from the original on 19 April 2019. Retrieved 9 January 2013. Even in the most specialized circles, the new particle discovered in July is not yet being called the "Higgs boson". Physicists still hesitate to call it that before they have determined that its properties fit with those the Higgs theory predicts the Higgs boson has.
30. ^ Naik, G. (14 March 2013). "New Data Boosts Case for Higgs Boson Find". The Wall Street Journal. Archived from the original on 4 January 2018. Retrieved 15 March 2013. 'We've never seen an elementary particle with spin zero,' said Tony Weidberg, a particle physicist at the University of Oxford who is also involved in the CERN experiments.
31. Heilprin, J. (14 March 2013). "Higgs Boson Discovery Confirmed After Physicists Review Large Hadron Collider Data at CERN". The Huffington Post. Archived from the original on 17 March 2013. Retrieved 14 March 2013.
32. ^ "LHC experiments delve deeper into precision". Media and Press relations (Press release). CERN. 11 July 2017. Archived from the original on 22 November 2018. Retrieved 23 July 2017.
33. "CMS precisely measures the mass of the Higgs boson". CMS Collaboration/CERN. Archived from the original on 23 December 2021. Retrieved 21 January 2022.
34. D'Onofrio, Michela; Rummukainen, Kari (15 January 2016). "Standard model cross-over on the lattice". Physical Review D. 93 (2): 025003. arXiv:1508.07161. Bibcode:2016PhRvD..93b5003D. doi:10.1103/PhysRevD.93.025003. S2CID 119261776.
35. Demystifying the Higgs Boson with Leonard Susskind Archived 1 April 2019 at the Wayback Machine, Leonard Susskind presents an explanation of what the Higgs mechanism is, and what it means to "give mass to particles." He also explains what's at stake for the future of physics and cosmology. 30 July 2012.
36. D'Onofrio, Michela; Rummukainen, Kari (2016). "Standard model cross-over on the lattice". Phys. Rev. D93 (2): 025003. arXiv:1508.07161. Bibcode:2016PhRvD..93b5003D. doi:10.1103/PhysRevD.93.025003. S2CID 119261776.
37. Rao, Achintya (2 July 2012). "Why would I care about the Higgs boson?". CMS Public Website. CERN. Archived from the original on 9 July 2012. Retrieved 18 July 2012.
38. Jammer, Max (2000). Concepts of Mass in Contemporary Physics and Philosophy. Princeton, NJ: Princeton University Press. pp. 162–163. ISBN 9780691010175., who provides many references in support of this statement.
39. Dvorsky, George (2013). "Is there a link between the Higgs boson and dark energy?". io9. Archived from the original on 1 March 2018. Retrieved 1 March 2018.
40. "What Universe Is This, Anyway?". NPR.org. 2014. Archived from the original on 1 March 2018. Retrieved 1 March 2018.
41. ^ Alekhin, S.; Djouadi, A.; Moch, S. (13 August 2012). "The top quark and Higgs boson masses and the stability of the electroweak vacuum". Physics Letters B. 716 (1): 214–219. arXiv:1207.0980. Bibcode:2012PhLB..716..214A. doi:10.1016/j.physletb.2012.08.024. S2CID 28216028.
42. Turner, M.S.; Wilczek, F. (1982). "Is our vacuum metastable?". Nature. 298 (5875): 633–634. Bibcode:1982Natur.298..633T. doi:10.1038/298633a0. S2CID 4274444.
43. Coleman, S.; de Luccia, F. (1980). "Gravitational effects on and of vacuum decay". Physical Review. D21 (12): 3305–3315. Bibcode:1980PhRvD..21.3305C. doi:10.1103/PhysRevD.21.3305. OSTI 1445512.
44. Stone, M. (1976). "Lifetime and decay of excited vacuum states". Phys. Rev. D. 14 (12): 3568–3573. Bibcode:1976PhRvD..14.3568S. doi:10.1103/PhysRevD.14.3568.
45. Frampton, P.H. (1976). "Vacuum Instability and Higgs Scalar Mass". Physical Review Letters. 37 (21): 1378–1380. Bibcode:1976PhRvL..37.1378F. doi:10.1103/PhysRevLett.37.1378.
46. Frampton, P.H. (1977). "Consequences of Vacuum Instability in Quantum Field Theory". Phys. Rev. D. 15 (10): 2922–2928. Bibcode:1977PhRvD..15.2922F. doi:10.1103/PhysRevD.15.2922.
47. Klotz, Irene (18 February 2013). Adams, David; Eastham, Todd (eds.). "Universe has finite lifespan, Higgs boson calculations suggest". Huffington Post. Reuters. Archived from the original on 20 February 2013. Retrieved 21 February 2013. Earth will likely be long gone before any Higgs boson particles set off an apocalyptic assault on the universe
48. Hoffman, Mark (19 February 2013). "Higgs boson will destroy the universe, eventually". Science World Report. Archived from the original on 11 June 2019. Retrieved 21 February 2013.
49. Ellis, J.; Espinosa, J.R.; Giudice, G.F.; Hoecker, A.; Riotto, A. (2009). "The Probable Fate of the Standard Model". Physics Letters B. 679 (4): 369–375. arXiv:0906.0954. Bibcode:2009PhLB..679..369E. doi:10.1016/j.physletb.2009.07.054. S2CID 17422678.
50. Masina, Isabella (12 February 2013). "Higgs boson and top quark masses as tests of electroweak vacuum stability". Phys. Rev. D. 87 (5): 53001. arXiv:1209.0393. Bibcode:2013PhRvD..87e3001M. doi:10.1103/PhysRevD.87.053001. S2CID 118451972.
51. Buttazzo, Dario; Degrassi, Giuseppe; Giardino, Pier Paolo; Giudice, Gian F.; Sala, Filippo; Salvio, Alberto; Strumia, Alessandro (2013). "Investigating the near-criticality of the Higgs boson". JHEP. 2013 (12): 089. arXiv:1307.3536. Bibcode:2013JHEP...12..089B. doi:10.1007/JHEP12(2013)089. S2CID 54021743. Archived from the original on 28 August 2014. Retrieved 25 June 2014.
52. Salvio, Alberto (9 April 2015). "A simple, motivated completion of the Standard Model below the Planck scale: Axions and right-handed neutrinos". Physics Letters B. 743: 428–434. arXiv:1501.03781. Bibcode:2015PhLB..743..428S. doi:10.1016/j.physletb.2015.03.015. S2CID 119279576.
53. ^ Boyle, Alan (19 February 2013). "Will our universe end in a 'big slurp'? Higgs-like particle suggests it might". NBC News' Cosmic blog. Archived from the original on 21 February 2013. Retrieved 21 February 2013. he bad news is that its mass suggests the universe will end in a fast-spreading bubble of doom. The good news? It'll probably be tens of billions of years. The article quotes Fermilab's Joseph Lykken: "he parameters for our universe, including the Higgs suggest that we're just at the edge of stability, in a "metastable" state. Physicists have been contemplating such a possibility for more than 30 years. Back in 1982, physicists Michael Turner and Frank Wilczek wrote in Nature that "without warning, a bubble of true vacuum could nucleate somewhere in the universe and move outwards ..."
54. Peralta, Eyder (19 February 2013). "If Higgs boson calculations are right, a catastrophic 'bubble' could end universe". The Two-Way. NPR News. Archived from the original on 21 February 2013. Retrieved 21 February 2013. Article cites Fermilab's Joseph Lykken: "The bubble forms through an unlikely quantum fluctuation, at a random time and place," Lykken tells us. "So in principle it could happen tomorrow, but then most likely in a very distant galaxy, so we are still safe for billions of years before it gets to us."
55. Bezrukov, F.; Shaposhnikov, M. (24 January 2008). "The Standard Model Higgs boson as the inflaton". Physics Letters B. 659 (3): 703–706. arXiv:0710.3755. Bibcode:2008PhLB..659..703B. doi:10.1016/j.physletb.2007.11.072. S2CID 14818281.
56. Salvio, Alberto (9 August 2013). "Higgs Inflation at NNLO after the Boson Discovery". Physics Letters B. 727 (1–3): 234–239. arXiv:1308.2244. Bibcode:2013PhLB..727..234S. doi:10.1016/j.physletb.2013.10.042. S2CID 56544999. Archived from the original on 26 January 2016. Retrieved 25 June 2014.
57. Cole, K.C. (14 December 2000). "One Thing Is Perfectly Clear: Nothingness Is Perfect". Los Angeles Times. Archived from the original on 25 January 2022. Retrieved 17 January 2013. he Higgs' influence (or the influence of something like it) could reach much further. For example, something like the Higgs—if not exactly the Higgs itself—may be behind many other unexplained "broken symmetries" in the universe as well ... In fact, something very much like the Higgs may have been behind the collapse of the symmetry that led to the Big Bang, which created the universe. When the forces first began to separate from their primordial sameness—taking on the distinct characters they have today—they released energy in the same way as water releases energy when it turns to ice. Except in this case, the freezing packed enough energy to blow up the universe. ... However it happened, the moral is clear: Only when the perfection shatters can everything else be born.
58. Sean Carroll (2012). The Particle at the End of the Universe: How the Hunt for the Higgs Boson Leads Us to the Edge of a New World. Penguin Group US. ISBN 978-1-101-60970-5.
59. Goldstone, J.; Salam, Abdus; Weinberg, Steven (1962). "Broken Symmetries". Physical Review. 127 (3): 965–970. Bibcode:1962PhRv..127..965G. doi:10.1103/PhysRev.127.965.
60. ^ Guralnik, G. S. (2011). "The Beginnings of Spontaneous Symmetry Breaking in Particle Physics". arXiv:1110.2253 .
61. ^ Kibble, T.W.B. (2009). "Englert–Brout–Higgs–Guralnik–Hagen–Kibble Mechanism". Scholarpedia. 4 (1): 6441. Bibcode:2009SchpJ...4.6441K. doi:10.4249/scholarpedia.6441.
62. ^ Kibble, T.W.B. (2009). "History of Englert–Brout–Higgs–Guralnik–Hagen–Kibble Mechanism (history)". Scholarpedia. 4 (1): 8741. Bibcode:2009SchpJ...4.8741K. doi:10.4249/scholarpedia.8741.
63. "The Nobel Prize in Physics 2008". Nobelprize.org. Archived from the original on 13 January 2009.
64. Ruegg, Henri; Ruiz-Altaba, Martí (2004). "The Stueckelberg Field". International Journal of Modern Physics A. 19 (20): 3265–3347. arXiv:hep-th/0304245. Bibcode:2004IJMPA..19.3265R. doi:10.1142/S0217751X04019755. S2CID 7017354. Archived from the original on 10 December 2021. Retrieved 15 January 2022.
65. List of Anderson 1958–1959 papers referencing 'symmetry', at APS Journals
66. ^ Higgs, Peter (24 November 2010). "My Life as a Boson" (PDF). London: Kings College. pp. 4–5. Archived from the original (PDF) on 4 November 2013. Retrieved 17 January 2013. – Talk given by Peter Higgs at Kings College, London, expanding on a paper originally presented in 2001. The original 2001 paper may be found in: Higgs, Peter (25 May 2001). "My Life as a Boson: The Story of 'The Higgs'". In Michael J. Duff & James T. Liu (eds.). 2001 A Spacetime Odyssey: Proceedings of the Inaugural Conference of the Michigan Center for Theoretical Physics. Ann Arbor, Michigan: World Scientific. pp. 86–88. ISBN 978-9-8123-8231-3. Archived from the original on 25 January 2022. Retrieved 17 January 2013.
67. Anderson, P. (1963). "Plasmons, gauge invariance and mass". Physical Review. 130 (1): 439–442. Bibcode:1963PhRv..130..439A. doi:10.1103/PhysRev.130.439.
68. Klein, A.; Lee, B. (1964). "Does Spontaneous Breakdown of Symmetry Imply Zero-Mass Particles?". Physical Review Letters. 12 (10): 266–268. Bibcode:1964PhRvL..12..266K. doi:10.1103/PhysRevLett.12.266.
69. Englert, François; Brout, Robert (1964). "Broken Symmetry and the Mass of Gauge Vector Mesons". Physical Review Letters. 13 (9): 321–323. Bibcode:1964PhRvL..13..321E. doi:10.1103/PhysRevLett.13.321.
70. ^ Higgs, Peter (1964). "Broken Symmetries and the Masses of Gauge Bosons". Physical Review Letters. 13 (16): 508–509. Bibcode:1964PhRvL..13..508H. doi:10.1103/PhysRevLett.13.508.
71. ^ Guralnik, Gerald; Hagen, C. R.; Kibble, T. W. B. (1964). "Global Conservation Laws and Massless Particles". Physical Review Letters. 13 (20): 585–587. Bibcode:1964PhRvL..13..585G. doi:10.1103/PhysRevLett.13.585.
72. Higgs, Peter (1964). "Broken symmetries, massless particles, and gauge fields". Physics Letters. 12 (2): 132–133. Bibcode:1964PhL....12..132H. doi:10.1016/0031-9163(64)91136-9.
73. Higgs, Peter (24 November 2010). "My Life as a Boson" (PDF). Talk given by Peter Higgs at Kings College, London, 24 November 2010. Archived from the original (PDF) on 4 November 2013. Retrieved 17 January 2013. Gilbert ... wrote a response to saying 'No, you cannot do that in a relativistic theory. You cannot have a preferred unit time-like vector like that.' This is where I came in, because the next month was when I responded to Gilbert's paper by saying 'Yes, you can have such a thing' but only in a gauge theory with a gauge field coupled to the current.
74. G.S. Guralnik (2011). "Gauge invariance and the Goldstone theorem – 1965 Feldafing talk". Modern Physics Letters A. 26 (19): 1381–1392. arXiv:1107.4592. Bibcode:2011MPLA...26.1381G. doi:10.1142/S0217732311036188. S2CID 118500709.
75. Higgs, Peter (1966). "Spontaneous Symmetry Breakdown without Massless Bosons". Physical Review. 145 (4): 1156–1163. Bibcode:1966PhRv..145.1156H. doi:10.1103/PhysRev.145.1156.
76. Kibble, Tom (1967). "Symmetry Breaking in Non-Abelian Gauge Theories". Physical Review. 155 (5): 1554–1561. Bibcode:1967PhRv..155.1554K. doi:10.1103/PhysRev.155.1554.
77. "Guralnik, G S; Hagen, C R and Kibble, T W B (1967). Broken Symmetries and the Goldstone Theorem. Advances in Physics, vol. 2" (PDF). Archived from the original (PDF) on 24 September 2015. Retrieved 16 September 2014.
78. ^ "Letters from the Past – A PRL Retrospective". Physical Review Letters. 12 February 2014. Archived from the original on 10 January 2010. Retrieved 7 May 2008.
79. S. Weinberg (1967). "A Model of Leptons". Physical Review Letters. 19 (21): 1264–1266. Bibcode:1967PhRvL..19.1264W. doi:10.1103/PhysRevLett.19.1264.
80. A. Salam (1968). N. Svartholm (ed.). Elementary Particle Physics: Relativistic Groups and Analyticity. Eighth Nobel Symposium. Stockholm: Almquvist and Wiksell. p. 367.
81. S.L. Glashow (1961). "Partial-symmetries of weak interactions". Nuclear Physics. 22 (4): 579–588. Bibcode:1961NucPh..22..579G. doi:10.1016/0029-5582(61)90469-2.
82. ^ Ellis, John; Gaillard, Mary K.; Nanopoulos, Dimitri V. (2012). "A Historical Profile of the Higgs Boson". arXiv:1201.6045 .
83. Martin Veltman (8 December 1999). "From Weak Interactions to Gravitation" (PDF). The Nobel Prize. p. 391. Archived from the original (PDF) on 25 July 2018. Retrieved 9 October 2013.
84. ^ Politzer, David (8 December 2004). "The Dilemma of Attribution". The Nobel Prize. Archived from the original on 21 March 2013. Retrieved 22 January 2013. Sidney Coleman published in Science magazine in 1979 a citation search he did documenting that essentially no one paid any attention to Weinberg's Nobel Prize winning paper until the work of 't Hooft (as explicated by Ben Lee). In 1971 interest in Weinberg's paper exploded. I had a parallel personal experience: I took a one-year course on weak interactions from Shelly Glashow in 1970, and he never even mentioned the Weinberg–Salam model or his own contributions.
85. Coleman, Sidney (14 December 1979). "The 1979 Nobel Prize in Physics". Science. 206 (4424): 1290–1292. Bibcode:1979Sci...206.1290C. doi:10.1126/science.206.4424.1290. PMID 17799637.
86. ^ (50 year celebration, 2008)
87. Bernstein 1974, p. 9
88. Bernstein 1974, pp. 9, 36 (footnote), 43–44, 47
89. ^ American Physical Society – "J. J. Sakurai Prize for Theoretical Particle Physics". Archived from the original on 12 February 2010. Retrieved 2 October 2009.
90. Merali, Zeeya (4 August 2010). "Physicists get political over Higgs". Nature. doi:10.1038/news.2010.390. Archived from the original on 25 January 2022. Retrieved 28 December 2011.
91. ^ Close, Frank (2011). The Infinity Puzzle: Quantum Field Theory and the Hunt for an Orderly Universe. Oxford: Oxford University Press. ISBN 978-0-19-959350-7.
92. ^ G.S. Guralnik (2009). "The History of the Guralnik, Hagen and Kibble development of the Theory of Spontaneous Symmetry Breaking and Gauge Particles". International Journal of Modern Physics A. 24 (14): 2601–2627. arXiv:0907.3466. Bibcode:2009IJMPA..24.2601G. doi:10.1142/S0217751X09045431. S2CID 16298371.
93. ^ Baglio, Julien; Djouadi, Abdelhak (2011). "Higgs production at the lHC". Journal of High Energy Physics. 1103 (3): 055. arXiv:1012.0530. Bibcode:2011JHEP...03..055B. doi:10.1007/JHEP03(2011)055. S2CID 119295294.
94. "Collisions". LHC Machine Outreach. CERN. Archived from the original on 26 March 2020. Retrieved 26 July 2012.
95. ^ "Hunt for Higgs boson hits key decision point". NBC News. 6 December 2012. Archived from the original on 18 May 2020. Retrieved 19 January 2013.
96. "Welcome to the Worldwide LHC Computing Grid". WLCG – Worldwide LHC Computing Grid. CERN. Archived from the original on 25 July 2018. Retrieved 14 November 2012. global collaboration of more than 170 computing centres in 36 countries ... to store, distribute and analyse the ~25 Petabytes (25 million Gigabytes) of data annually generated by the Large Hadron Collider
97. "The Worldwide LHC Computing Grid". The Worldwide LHC Computing Grid. CERN. November 2017. Archived from the original on 7 November 2017. Retrieved 5 November 2017. It now links thousands of computers and storage systems in over 170 centres across 41 countries. ... The WLCG is the world's largest computing grid
98. W.-M. Yao; et al. (2006). "Review of Particle Physics" (PDF). Journal of Physics G. 33 (1): 1–1232. arXiv:astro-ph/0601168. Bibcode:2006JPhG...33....1Y. doi:10.1088/0954-3899/33/1/001. Archived (PDF) from the original on 27 January 2017. Retrieved 25 October 2006.
99. The CDF Collaboration; The D0 Collaboration; The Tevatron New Physics, Higgs Working Group (2012). "Updated Combination of CDF and D0 Searches for Standard Model Higgs Boson Production with up to 10.0 fb of Data". arXiv:1207.0449 .{{cite arXiv}}: CS1 maint: numeric names: authors list (link)
100. "Interim Summary Report on the Analysis of the 19 September 2008 Incident at the LHC" (PDF). CERN. 15 October 2008. EDMS 973073. Archived (PDF) from the original on 20 August 2013. Retrieved 28 September 2009.
101. "CERN releases analysis of LHC incident". Media and Press relations (Press release). CERN. 16 October 2008. Archived from the original on 12 November 2016. Retrieved 12 November 2016.
102. "LHC to restart in 2009". Media and Press relations (Press release). CERN. 5 December 2008. Archived from the original on 12 November 2016. Retrieved 12 November 2016.
103. "LHC progress report". CERN Bulletin (18). 3 May 2010. Archived from the original on 26 May 2018. Retrieved 7 December 2011.
104. "ATLAS experiment presents latest Higgs search status". ATLAS homepage. CERN. 13 December 2011. Archived from the original on 23 November 2016. Retrieved 13 December 2011.
105. Taylor, Lucas (13 December 2011). "CMS search for the Standard Model Higgs Boson in LHC data from 2010 and 2011". CMS public website. CERN. Archived from the original on 7 January 2012. Retrieved 13 December 2011.
106. ^ Overbye, D. (5 March 2013). "Chasing The Higgs Boson". The New York Times. Archived from the original on 5 March 2013. Retrieved 5 March 2013.
107. ^ "ATLAS and CMS experiments present Higgs search status" (Press release). CERN Press Office. 13 December 2011. Archived from the original on 13 December 2012. Retrieved 14 September 2012. the statistical significance is not large enough to say anything conclusive. As of today what we see is consistent either with a background fluctuation or with the presence of the boson. Refined analyses and additional data delivered in 2012 by this magnificent machine will definitely give an answer
108. "Welcome". WLCG – Worldwide LHC Computing Grid. CERN. Archived from the original on 10 November 2012. Retrieved 29 October 2012.
109. CMS collaboration (2015). "Precise determination of the mass of the Higgs boson and tests of compatibility of its couplings with the standard model predictions using proton collisions at 7 and 8 TeV". The European Physical Journal C. 75 (5): 212. arXiv:1412.8662. Bibcode:2015EPJC...75..212K. doi:10.1140/epjc/s10052-015-3351-7. PMC 4433454. PMID 25999783.
110. ATLAS collaboration (2015). "Measurements of Higgs boson production and couplings in the four-lepton channel in pp collisions at center-of-mass energies of 7 and 8 TeV with the ATLAS detector". Physical Review D. 91 (1): 012006. arXiv:1408.5191. Bibcode:2015PhRvD..91a2006A. doi:10.1103/PhysRevD.91.012006.
111. ATLAS collaboration (2014). "Measurement of Higgs boson production in the diphoton decay channel in pp collisions at center-of-mass energies of 7 and 8 TeV with the ATLAS detector". Physical Review D. 90 (11): 112015. arXiv:1408.7084. Bibcode:2014PhRvD..90k2015A. doi:10.1103/PhysRevD.90.112015.
112. "Press Conference: Update on the search for the Higgs boson at CERN on 4 July 2012". Indico.cern.ch. 22 June 2012. Archived from the original on 21 July 2012. Retrieved 4 July 2012.
113. "CERN to give update on Higgs search as curtain raiser to ICHEP conference". Media and Press relations (Press release). CERN. 22 June 2012. Archived from the original on 12 November 2016. Retrieved 12 November 2016.
114. "Scientists analyse global Twitter gossip around Higgs boson discovery". Phys.org. 23 January 2013. Archived from the original on 29 October 2013. Retrieved 6 February 2013. For the first time scientists have been able to analyse the dynamics of social media on a global scale before, during and after the announcement of a major scientific discovery.
     De Domenico, M.; Lima, A.; Mougel, P.; Musolesi, M. (2013). "The Anatomy of a Scientific Gossip". Scientific Reports. 3 (2013): 2980. arXiv:1301.2952. Bibcode:2013NatSR...3E2980D. doi:10.1038/srep02980. PMC 3798885. PMID 24135961.
115. "Higgs boson particle results could be a quantum leap". Times LIVE. 28 June 2012. Archived from the original on 4 July 2012. Retrieved 4 July 2012.
116. CERN prepares to deliver Higgs particle findings Archived 17 March 2021 at the Wayback Machine, Australian Broadcasting Corporation. Retrieved 4 July 2012.
117. "God Particle Finally Discovered? Higgs Boson News At Cern Will Even Feature Scientist It's Named After". Huffingtonpost.co.uk. 3 July 2012. Archived from the original on 11 March 2013. Retrieved 19 January 2013.
118. Our Bureau (4 July 2012). "Higgs on way, theories thicken – Wait for news on God particle". The Telegraph – India. Archived from the original on 7 July 2012. Retrieved 19 January 2013.
119. Thornhill, Ted (3 July 2013). "God Particle Finally Discovered? Higgs Boson News At Cern Will Even Feature Scientist It's Named After". Huffington Post. Archived from the original on 11 September 2013. Retrieved 23 July 2013.
120. Adrian Cho (13 July 2012). "Higgs Boson Makes Its Debut After Decades-Long Search". Science. 337 (6091): 141–143. Bibcode:2012Sci...337..141C. doi:10.1126/science.337.6091.141. PMID 22798574.
121. ^ CMS collaboration (2012). "Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC". Physics Letters B. 716 (1): 30–61. arXiv:1207.7235. Bibcode:2012PhLB..716...30C. doi:10.1016/j.physletb.2012.08.021.
122. ^ Taylor, Lucas (4 July 2012). "Observation of a New Particle with a Mass of 125 GeV". CMS Public Website. CERN. Archived from the original on 5 July 2012. Retrieved 4 July 2012.
123. "Latest Results from ATLAS Higgs Search". ATLAS News. CERN. 4 July 2012. Archived from the original on 23 November 2016. Retrieved 4 July 2012.
124. ^ ATLAS collaboration (2012). "Observation of a New Particle in the Search for the Standard Model Higgs Boson with the ATLAS Detector at the LHC". Physics Letters B. 716 (1): 1–29. arXiv:1207.7214. Bibcode:2012PhLB..716....1A. doi:10.1016/j.physletb.2012.08.020. S2CID 119169617.
125. ^ "Higgs bosons: theory and searches" (PDF). PDGLive. Particle Data Group. 12 July 2012. Archived (PDF) from the original on 8 March 2021. Retrieved 15 August 2012.
126. Gillies, James (23 July 2012). "LHC 2012 proton run extended by seven weeks". CERN Bulletin (30). Archived from the original on 26 May 2018. Retrieved 29 August 2012.
127. ^ "Higgs boson behaving as expected". 3 News NZ. 15 November 2012. Archived from the original on 1 May 2014. Retrieved 15 November 2012.
128. Strassler, Matt (14 November 2012). "Higgs Results at Kyoto". Of Particular Significance: Conversations about science with theoretical physicist Matt Strassler (personal website). Archived from the original on 8 March 2021. Retrieved 10 January 2013.
129. Sample, Ian (14 November 2012). "Higgs particle looks like a bog Standard Model boson, say scientists". The Guardian. London, UK. Archived from the original on 26 January 2016. Retrieved 15 November 2012.
130. "CERN experiments observe particle consistent with long-sought Higgs boson". Media and Press relations (Press release). CERN. 4 July 2012. Archived from the original on 21 November 2017. Retrieved 12 November 2016.
131. "Person Of The Year 2012". Time. 19 December 2012. Archived from the original on 12 February 2013. Retrieved 13 February 2013.
132. "Higgs Boson Discovery Has Been Confirmed". Forbes. Archived from the original on 25 October 2013. Retrieved 9 October 2013.
133. Slate Video Staff (11 September 2012). "Higgs Boson Confirmed; CERN Discovery Passes Test". Slate.com. Archived from the original on 9 July 2013. Retrieved 9 October 2013.
134. "The Year Of The Higgs, And Other Tiny Advances In Science". NPR.org. NPR. 1 January 2013. Archived from the original on 5 March 2014. Retrieved 9 October 2013.
135. "Confirmed: the Higgs boson does exist". The Sydney Morning Herald. 4 July 2012. Archived from the original on 25 January 2022. Retrieved 21 February 2020.
136. John Heilprin (27 January 2013). "CERN chief: Higgs boson quest could wrap up by midyear". NBCNews.com. AP. Archived from the original on 21 February 2013. Retrieved 20 February 2013. Rolf Heuer, director of , said he is confident that "towards the middle of the year, we will be there." – Interview by AP, at the World Economic Forum, 26 January 2013.
137. Boyle, Alan (16 February 2013). "Will our universe end in a 'big slurp'? Higgs-like particle suggests it might". NBCNews.com. Archived from the original on 21 February 2013. Retrieved 20 February 2013. 'it's going to take another few years' after the collider is restarted to confirm definitively that the newfound particle is the Higgs boson.
138. Gillies, James (6 March 2013). "A question of spin for the new boson". CERN. Archived from the original on 8 March 2013. Retrieved 7 March 2013.
139. ^ Chatrchyan, S.; et al. (CMS Collaboration) (February 2013). "Study of the mass and spin-parity of the Higgs boson candidate via its decays to Z boson pairs". Physical Review Letters. 110 (8): 081803. arXiv:1212.6639. Bibcode:2013PhRvL.110h1803C. doi:10.1103/PhysRevLett.110.081803. PMID 23473131. S2CID 2621524.
140. ^ Aad, G.; et al. (ATLAS Collaboration) (7 October 2013). "Evidence for the spin-0 nature of the Higgs boson using ATLAS data". Phys. Lett. B. 726 (1–3): 120–144. arXiv:1307.1432. Bibcode:2013PhLB..726..120A. doi:10.1016/j.physletb.2013.08.026.
141. Chatrchyan, S.; et al. (CMS collaboration) (2013). "Higgs-like Particle in a Mirror". Physical Review Letters. 110 (8): 081803. arXiv:1212.6639. Bibcode:2013PhRvL.110h1803C. doi:10.1103/PhysRevLett.110.081803. PMID 23473131. S2CID 2621524.
142. ATLAS; CMS Collaborations (2016). "Measurements of the Higgs boson production and decay rates and constraints on its couplings from a combined ATLAS and CMS analysis of the LHC pp collision data at √s = 7 and 8 TeV". Journal of High Energy Physics. 2016 (8): 45. arXiv:1606.02266. Bibcode:2016JHEP...08..045A. doi:10.1007/JHEP08(2016)045. S2CID 118523967.
143. "Highlights from the 2019 Moriond conference (electroweak physics)". 29 March 2019. Archived from the original on 21 April 2019. Retrieved 24 April 2019.
144. "All together now: adding more pieces to the Higgs boson puzzle". ATLAS collaboration. 18 March 2019. Archived from the original on 16 April 2019. Retrieved 24 April 2019.
145. "Long-sought decay of Higgs boson observed". Media and Press relations (Press release). CERN. 28 August 2018. Archived from the original on 22 November 2018. Retrieved 30 August 2018.
146. Atlas Collaboration (28 August 2018). "ATLAS observes elusive Higgs boson decay to a pair of bottom quarks". Atlas (Press release). CERN. Archived from the original on 28 August 2018. Retrieved 28 August 2018.
147. CMS Collaboration (August 2018). "Observation of Higgs boson decay to bottom quarks". CMS. Archived from the original on 30 August 2018. Retrieved 30 August 2018.
     CMS Collaboration (24 August 2018). "Observation of Higgs boson decay to bottom quarks". CERN Document Server. CERN. Archived from the original on 25 January 2022. Retrieved 30 August 2018.
     CMS Collaboration (24 August 2018). "Observation of Higgs boson decay to bottom quarks". Physical Review Letters. 121 (12): 121801. arXiv:1808.08242. Bibcode:2018PhRvL.121l1801S. doi:10.1103/PhysRevLett.121.121801. PMID 30296133. S2CID 118901756.
148. Peskin & Schroeder 1995, pp. 717–719, 787–791
149. Peskin & Schroeder 1995, pp. 715–716
150. Branco, G. C.; Ferreira, P.M.; Lavoura, L.; Rebelo, M.N.; Sher, Marc; Silva, João P. (July 2012). "Theory and phenomenology of two-Higgs-doublet models". Physics Reports. 516 (1): 1–102. arXiv:1106.0034. Bibcode:2012PhR...516....1B. doi:10.1016/j.physrep.2012.02.002. S2CID 119214990.
151. Csaki, C.; Grojean, C.; Pilo, L.; Terning, J. (2004). "Towards a realistic model of Higgsless electroweak symmetry breaking". Physical Review Letters. 92 (10): 101802. arXiv:hep-ph/0308038. Bibcode:2004PhRvL..92j1802C. doi:10.1103/PhysRevLett.92.101802. PMID 15089195. S2CID 6521798.
152. Csaki, C.; Grojean, C.; Pilo, L.; Terning, J.; Terning, John (2004). "Gauge theories on an interval: Unitarity without a Higgs". Physical Review D. 69 (5): 055006. arXiv:hep-ph/0305237. Bibcode:2004PhRvD..69e5006C. doi:10.1103/PhysRevD.69.055006. S2CID 119094852.
153. ^ "The Hierarchy Problem: why the Higgs has a snowball's chance in hell". Quantum Diaries. 1 July 2012. Archived from the original on 29 March 2013. Retrieved 19 March 2013.
154. "The Hierarchy Problem | Of Particular Significance". Profmattstrassler.com. 16 August 2011. Archived from the original on 7 March 2013. Retrieved 9 October 2013.
155. D. J. E. Callaway (1988). "Triviality Pursuit: Can Elementary Scalar Particles Exist?". Physics Reports. 167 (5): 241–320. Bibcode:1988PhR...167..241C. doi:10.1016/0370-1573(88)90008-7.
156. Gunion, John (2000). The Higgs Hunter's Guide (illustrated, reprint ed.). Westview Press. pp. 1–3. ISBN 978-0-7382-0305-8.
157. Randall, Lisa. Warped Passages: Unraveling the Mysteries of the Universe's Hidden Dimensions. p. 286. People initially thought of tachyons as particles travelling faster than the speed of light ... But we now know that a tachyon indicates an instability in a theory that contains it. Regrettably for science fiction fans, tachyons are not real physical particles that appear in nature.
158. Sen, Ashoke (May 2002). "Rolling Tachyon". J. High Energy Phys. 2002 (204): 48. arXiv:hep-th/0203211. Bibcode:2002JHEP...04..048S. doi:10.1088/1126-6708/2002/04/048. S2CID 12023565.
159. Kutasov, David; Marino, Marcos & Moore, Gregory W. (2000). "Some exact results on tachyon condensation in string field theory". JHEP. 2000 (10): 045. arXiv:hep-th/0009148. Bibcode:2000JHEP...10..045K. doi:10.1088/1126-6708/2000/10/045. S2CID 15664546.
160. Aharonov, Y.; Komar, A.; Susskind, L. (1969). "Superluminal Behavior, Causality, and Instability". Phys. Rev. 182 (5): 1400–1403. Bibcode:1969PhRv..182.1400A. doi:10.1103/PhysRev.182.1400.
161. Feinberg, Gerald (1967). "Possibility of faster-than-light particles". Physical Review. 159 (5): 1089–1105. Bibcode:1967PhRv..159.1089F. doi:10.1103/PhysRev.159.1089.
162. Peskin & Schroeder 1995
163. Flatow, Ira (6 July 2012). "At Long Last, The Higgs Particle... Maybe". NPR. Archived from the original on 10 July 2012. Retrieved 10 July 2012.
164. "Explanatory Figures for the Higgs Boson Exclusion Plots". ATLAS News. CERN. Archived from the original on 16 September 2017. Retrieved 6 July 2012.
165. Carena, M.; Grojean, C.; Kado, M.; Sharma, V. (2013). "Status of Higgs boson physics" (PDF). p. 192. Archived (PDF) from the original on 10 December 2017. Retrieved 5 November 2017.
166. Lykken, Joseph D. (27 June 2009). "Beyond the Standard Model". Proceedings of the 2009 European School of High-Energy Physics. Bautzen, Germany. arXiv:1005.1676. Bibcode:2010arXiv1005.1676L.
167. Plehn, Tilman (2012). Lectures on LHC Physics. Lecture Notes in Physics. Vol. 844. Springer. §1.2.2. arXiv:0910.4182. Bibcode:2012LNP...844.....P. doi:10.1007/978-3-642-24040-9. ISBN 978-3-642-24039-3. S2CID 118019449.
168. "LEP Electroweak Working Group". Archived from the original on 3 April 2008. Retrieved 4 April 2006.
169. Peskin, Michael E.; Wells, James D. (2001). "How can a heavy Higgs boson be consistent with the precision electroweak measurements?". Physical Review D. 64 (9): 093003. arXiv:hep-ph/0101342. Bibcode:2001PhRvD..64i3003P. doi:10.1103/PhysRevD.64.093003. S2CID 5932066.
170. ^ Baglio, Julien; Djouadi, Abdelhak (2010). "Predictions for Higgs production at the Tevatron and the associated uncertainties". Journal of High Energy Physics. 1010 (10): 063. arXiv:1003.4266. Bibcode:2010JHEP...10..064B. doi:10.1007/JHEP10(2010)064. S2CID 119199894.
171. ^ Teixeira-Dias (LEP Higgs working group), P. (2008). "Higgs boson searches at LEP". Journal of Physics: Conference Series. 110 (4): 042030. arXiv:0804.4146. Bibcode:2008JPhCS.110d2030T. doi:10.1088/1742-6596/110/4/042030. S2CID 16443715.
172. Asquith, Lily (22 June 2012). "Why does the Higgs decay?". Life and Physics. London: The Guardian. Archived from the original on 1 November 2013. Retrieved 14 August 2012.
173. Liu, G.Z.; Cheng, G. (2002). "Extension of the Anderson-Higgs mechanism". Physical Review B. 65 (13): 132513. arXiv:cond-mat/0106070. Bibcode:2002PhRvB..65m2513L. CiteSeerX 10.1.1.242.3601. doi:10.1103/PhysRevB.65.132513. S2CID 118551025.
174. ^ "Mass appeal: As physicists close in on the Higgs boson, they should resist calls to change its name". Nature (editorial). 483, 374 (7390): 374. 21 March 2012. Bibcode:2012Natur.483..374.. doi:10.1038/483374a. PMID 22437571.
175. ^ Becker, Kate (29 March 2012). "A Higgs by any other name". "NOVA" (PBS) physics. Archived from the original on 17 December 2012. Retrieved 21 January 2013.
176. "Frequently asked questions: The Higgs!". CERN Bulletin (28). Archived from the original on 5 July 2012. Retrieved 18 July 2012.
177. ^ Woit, Peter (13 April 2013). ""Not Even Wrong": Anderson on Anderson-Higgs". Mathematics. Woit's physics blog (blog). New York, NY: Columbia University. Archived from the original on 19 October 2013. Retrieved 6 August 2013.
178. Sample, Ian (4 July 2012). "Higgs boson's many great minds cause a Nobel prize headache". The Guardian. London, UK. Archived from the original on 17 October 2013. Retrieved 23 July 2013.
179. ^ Peskin, M. (July 2012). "40 years of the Higgs boson" (PDF). 2012 SLAC Summer Institute Conferences. Presentation at SSI 2012. Stanford University. pp. 3–5. Archived (PDF) from the original on 1 May 2014. Retrieved 21 January 2013. quoting Lee's ICHEP 1972 presentation at Fermilab: "... which is known as the Higgs mechanism ..." and "Lee's locution" – his footnoted explanation of this shorthand.
180. U.R. Phys. & Astro. press office (8 October 2007). "Nobelist Steven Weinberg praises professor Carl Hagen and collaborators for Higgs Boson theory". Department of Physics and Astronomy (Press release). Rochester, NY: University of Rochester. Archived from the original on 16 April 2008. — Rochester's Hagen Sakurai Prize announcement
181. Hagen, C.R. (2010). Sakurai Prize Talk (video) – via YouTube.
182. ^ Cho, A. (14 September 2012). "Why the 'Higgs'?" (PDF). Particle physics. Science. 337 (6100): 1287. doi:10.1126/science.337.6100.1287. PMID 22984044. Archived from the original (PDF) on 4 July 2013. Retrieved 12 February 2013. Lee ... apparently used the term 'Higgs Boson' as early as 1966 ... but what may have made the term stick is a seminal paper Steven Weinberg ... published in 1967 ... Weinberg acknowledged the mix-up in an essay in the New York Review of Books in May 2012. (See also original article in
     • New York Review of Books (2012)
     • Close, Frank (2011). "[see book extract]". The Infinity Puzzle. Oxford University Press. p. 372 – via Google Books.)
     which identified the error).
183. ^ Weinberg, Steven (10 May 2012). "The Crisis of Big Science". The New York Review of Books. footnote 1. Archived from the original on 21 January 2013. Retrieved 12 February 2013.
184. Lederman, Leon; Teresi, Dick (2006). The God Particle: If the Universe Is the Answer, What Is the Question?. Houghton Mifflin Harcourt. ISBN 978-0-547-52462-7. Archived from the original on 13 May 2016. Retrieved 27 June 2015.
185. Dickerson, Kelly (8 September 2014). "Stephen Hawking says 'god particle' could wipe out the universe". livescience.com. Archived from the original on 28 January 2015. Retrieved 23 February 2015.
186. Baggott, Jim (2012). Higgs: The invention and discovery of the 'God Particle'. Oxford University Press. ISBN 978-0-19-165003-1. Archived from the original on 20 May 2016. Retrieved 27 June 2015.
187. Scientific American, ed. (2012). The Higgs Boson: Searching for the God Particle. Macmillan. ISBN 978-1-4668-2413-3. Archived from the original on 9 June 2016. Retrieved 27 June 2015.
188. Ted Jaeckel (2007). The God Particle: The Discovery and Modeling of the Ultimate Prime Particle. Universal-Publishers. ISBN 978-1-58112-959-5. Archived from the original on 29 April 2016. Retrieved 27 June 2015.
189. ^ Aschenbach, Joy (5 December 1993). "No resurrection in sight for moribund super collider". Science. Los Angeles Times. Archived from the original on 6 November 2013. Retrieved 16 January 2013.
190. "A supercompetition for Illinois". Chicago Tribune. 31 October 1986. Archived from the original on 15 May 2013. Retrieved 16 January 2013. The SSC, proposed by the U.S. Department of Energy in 1983, is a mind-bending project... this gigantic laboratory ... this titanic project
191. Diaz, Jesus (15 December 2012). "This Is [The] World's Largest Super Collider That Never Was". Gizmodo. Archived from the original on 18 January 2013. Retrieved 16 January 2013. ...this titanic complex ...
192. Abbott, Charles (June 1987). "[no title cited]". Illinois Issues Journal. p. 18. Archived from the original on 1 November 2013. Retrieved 16 January 2013. Lederman, who considers himself an unofficial propagandist for the super collider, said the SSC could reverse the physics brain drain in which bright young physicists have left America to work in Europe and elsewhere.
193. Kevles, Dan. "Good-bye to the SSC: On the life and death of the superconducting super collider" (PDF). California Institute of Technology: "Engineering & Science". 58 no. 2 (Winter 1995): 16–25. Archived (PDF) from the original on 11 May 2013. Retrieved 16 January 2013. Lederman, one of the principal spokesmen for the SSC, was an accomplished high-energy experimentalist who had made Nobel Prize-winning contributions to the development of the Standard Model during the 1960s (although the prize itself did not come until 1988). He was a fixture at congressional hearings on the collider, an unbridled advocate of its merits.
194. Calder, Nigel (2005). Magic Universe: A grand tour of modern science. pp. 369–370. ISBN 978-0-19-162235-9. Archived from the original on 25 January 2022. Retrieved 5 September 2020. The possibility that the next big machine would create the Higgs became a carrot to dangle in front of funding agencies and politicians. A prominent American physicist, Leon lederman , advertised the Higgs as The God Particle in the title of a book published in 1993 ... Lederman was involved in a campaign to persuade the US government to continue funding the Superconducting Super Collider ... the ink was not dry on Lederman's book before the US Congress decided to write off the billions of dollars already spent
195. Lederman, Leon (1993). The God Particle: If the universe is the answer, what is the question?. Dell Publishing. chapter 2, p. 2. ISBN 978-0-385-31211-0. Retrieved 30 July 2015.
196. Alister McGrath (15 December 2011). "[The] Higgs boson: The particle of faith". The Daily Telegraph. Archived from the original on 15 December 2011. Retrieved 15 December 2011.
197. Sample, Ian (3 March 2009). "Father of the god particle: Portrait of Peter Higgs unveiled". The Guardian. London, UK. Archived from the original on 12 September 2014. Retrieved 24 June 2009.
198. ^ Chivers, Tom (13 December 2011). "How the 'god particle' got its name". The Telegraph. London, UK. Archived from the original on 9 January 2012. Retrieved 3 December 2012.
199. "Key scientist sure "God particle" will be found soon". Reuters. 7 April 2008. Archived from the original on 23 February 2021. Retrieved 2 July 2017.
200. "The man behind the 'god particle'". New Scientist (interview). 13 September 2008. pp. 44–45. Archived from the original on 13 September 2008. Retrieved 29 August 2017.
     ORIGINAL INTERVIEW
     "Father of the 'god particle'". The Guardian. 30 June 2008. Archived from the original on 1 December 2016. Retrieved 14 December 2016.
201. Borowitz, Andy (13 July 2012). "5 questions for the Higgs boson". The New Yorker. Archived from the original on 12 November 2020. Retrieved 12 December 2019.
202. Sample, Ian (2010). Massive: The hunt for the god particle. pp. 148–149, & 278–279. ISBN 978-1-905264-95-7. Archived from the original on 25 January 2022. Retrieved 5 September 2020.
203. Cole, K. (14 December 2000). "One thing is perfectly clear: Nothingness is perfect". Science File. Los Angeles Times. Archived from the original on 5 October 2015. Retrieved 17 January 2013. Consider the early universe–a state of pure, perfect nothingness; a formless fog of undifferentiated stuff ... 'perfect symmetry' ... What shattered this primordial perfection? One likely culprit is the so-called Higgs field ... Physicist Leon Lederman compares the way the Higgs operates to the biblical story of Babel all spoke the same language ... Like God, says Lederman, the Higgs differentiated the perfect sameness, confusing everyone (physicists included) ... Feynman wondered why the universe we live in was so obviously askew... Perhaps, he speculated, total perfection would have been unacceptable to God. And so, just as God shattered the perfection of Babel, 'God made the laws only nearly symmetrical'
204. Lederman, p. 22 et seq.:

     Something we cannot yet detect and which, one might say, has been put there to test and confuse us... The issue is whether physicists will be confounded by this puzzle or whether, in contrast to the unhappy Babylonians, we will continue to build the tower and, as Einstein put it, "know the mind of God". And the Lord said, Behold the people are un-confounding my confounding. And the Lord sighed and said, Go to, let us go down, and there give them the God Particle so that they may see how beautiful is the universe I have made

205. Sample, Ian (12 June 2009). "Higgs competition: Crack open the bubbly, the God particle is dead". The Guardian. London, UK. Archived from the original on 12 January 2015. Retrieved 4 May 2010.
206. Gordon, Fraser (5 July 2012). "Introducing the higgson". physicsworld.com. Archived from the original on 8 July 2012. Retrieved 25 August 2012.
207. Wolchover, Natalie (3 July 2012). "Higgs Boson Explained: How 'God Particle' Gives Things Mass". Huffington Post. Archived from the original on 20 April 2013. Retrieved 21 January 2013.
208. Oliver, Laura (4 July 2012). "Higgs boson: How would you explain it to a seven-year-old?". The Guardian. London, UK. Archived from the original on 22 October 2014. Retrieved 21 January 2013.
209. Zimmer, Ben (15 July 2012). "Higgs boson metaphors as clear as molasses". The Boston Globe. Archived from the original on 4 February 2013. Retrieved 21 January 2013.
210. "The Higgs particle: an analogy for Physics classroom (section)". www.lhc-closer.es (a collaboration website of LHCb physicist Xabier Vidal and High School Teachers at CERN educator Ramon Manzano). Archived from the original on 5 July 2012. Retrieved 9 January 2013.
211. Flam, Faye (12 July 2012). "Finally – A Higgs Boson Story Anyone Can Understand". The Philadelphia Inquirer (philly.com). Archived from the original on 23 March 2013. Retrieved 21 January 2013.
212. Sample, Ian (28 April 2011). "How will we know when the Higgs particle has been detected?". The Guardian. London, UK. Archived from the original on 26 January 2016. Retrieved 21 January 2013.
213. ^ Miller, David (1993). "A quasi-political explanation of the Higgs boson; for Mr. Waldegrave, UK Science Minister". Archived from the original on 15 March 2010. Retrieved 10 July 2012.
214. Jepsen, Kathryn (1 March 2012). "Ten things you may not know about the Higgs boson". Symmetry Magazine. Archived from the original on 14 August 2012. Retrieved 10 July 2012.
215. Goldberg, David (17 November 2010). "What's the matter with the Higgs boson?". io9. Archived from the original on 21 January 2013. Retrieved 21 January 2013.{{cite web}}: CS1 maint: unfit URL (link)
216. "The Nobel Prize in Physics 1979". official Nobel Prize website. Archived from the original on 17 June 2017. Retrieved 13 June 2017.
217. "The Nobel Prize in Physics 1999". official Nobel Prize website. Archived from the original on 16 June 2017. Retrieved 13 June 2017.
218. "Special Breakthrough Prize Laureates 2013". breakthroughprize.org. Archived from the original on 15 January 2017.
219. "2013 Nobel Prize in Physics". official Nobel Prize website. Archived from the original on 11 June 2017. Retrieved 13 June 2017.
220. Overbye, D. (8 October 2013). "For Nobel, they can thank the 'god particle'". The New York Times. Archived from the original on 30 June 2017. Retrieved 3 November 2013.
221. Daigle, Katy (10 July 2012). "India: Enough about Higgs, let's discuss the boson". AP News. Archived from the original on 23 September 2012. Retrieved 10 July 2012.
222. Bal, Hartosh Singh (19 September 2012). "The Bose in the Boson". The New York Times. Archived from the original on 29 December 2019. Retrieved 21 September 2012.
223. Alikhan, Anvar (16 July 2012). "The spark in a crowded field". Outlook India. Archived from the original on 9 July 2012. Retrieved 10 July 2012.
224. ^ Peskin & Schroeder 1995, Chapter 20
225. Nakano, T.; Nishijima, N. (1953). "Charge independence for V-particles". Progress of Theoretical Physics. 10 (5): 581. Bibcode:1953PThPh..10..581N. doi:10.1143/PTP.10.581.
226. Nishijima, K. (1955). "Charge independence theory of V-particles". Progress of Theoretical Physics. 13 (3): 285–304. Bibcode:1955PThPh..13..285N. doi:10.1143/PTP.13.285.
227. Gell-Mann, M. (1956). "The interpretation of the new particles as displaced charged multiplets". Il Nuovo Cimento. 4 (S2): 848–866. Bibcode:1956NCim....4S.848G. doi:10.1007/BF02748000. S2CID 121017243.

General references

• Bernstein, Jeremy (January 1974). "Spontaneous symmetry breaking, gauge theories, the Higgs mechanism and all that" (PDF). Reviews of Modern Physics. 46 (1): 7–48. Bibcode:1974RvMP...46....7B. doi:10.1103/RevModPhys.46.7. Archived from the original (PDF) on 21 January 2013. Retrieved 10 December 2012.

• Peskin, Michael E.; Schroeder, Daniel V. (1995). An Introduction to Quantum Field Theory. Reading, MA: Addison-Wesley Publishing Company. ISBN 978-0-201-50397-5.

• Tipler, Paul; Llewellyn, Ralph (2003). Modern Physics. W. H. Freeman. ISBN 978-0-7167-4345-3.

• Griffiths, David (2008). Introduction to Elementary Particles (2nd revised ed.). WILEY-VCH. ISBN 978-3-527-40601-2.

Further reading

• Nambu, Yoichiro; Jona-Lasinio, Giovanni (1961). "Dynamical Model of Elementary Particles Based on an Analogy with Superconductivity". Physical Review. 122 (1): 345–358. Bibcode:1961PhRv..122..345N. doi:10.1103/PhysRev.122.345.
• Anderson, Philip W. (1963). "Plasmons, Gauge Invariance, and Mass". Physical Review. 130 (1): 439–442. Bibcode:1963PhRv..130..439A. doi:10.1103/PhysRev.130.439.
• Klein, Abraham; Lee, Benjamin W. (1964). "Does Spontaneous Breakdown of Symmetry Imply Zero-Mass Particles?". Physical Review Letters. 12 (10): 266–268. Bibcode:1964PhRvL..12..266K. doi:10.1103/PhysRevLett.12.266.
• Gilbert, Walter (1964). "Broken Symmetries and Massless Particles". Physical Review Letters. 12 (25): 713–714. Bibcode:1964PhRvL..12..713G. doi:10.1103/PhysRevLett.12.713.
• Higgs, Peter (1964). "Broken Symmetries, Massless Particles and Gauge Fields". Physics Letters. 12 (2): 132–133. Bibcode:1964PhL....12..132H. doi:10.1016/0031-9163(64)91136-9.
• Guralnik, Gerald S.; Hagen, C.R.; Kibble, Tom W.B. (1968). "Broken Symmetries and the Goldstone Theorem". In R.L. Cool and R.E. Marshak (ed.). Advances in Physics, Vol. 2. Interscience Publishers. pp. 567–708. ISBN 978-0-470-17057-1. Archived from the original on 23 April 2012. Retrieved 18 June 2011.
• Sean Carroll (2013). The Particle at the End of the Universe: How the Hunt for the Higgs Boson Leads Us to the Edge of a New World. Dutton. ISBN 978-0-14-218030-3.
• Jakobs, Karl; Seez, Chris (2015). "The Higgs Boson discovery". Scholarpedia. 10 (9): 32413. doi:10.4249/scholarpedia.32413. Archived from the original on 26 January 2016. Retrieved 17 January 2016.

External links

Popular science, mass media, and general coverage

• Higgs Boson observation at CERN
• Hunting the Higgs Boson at C.M.S. Experiment, at CERN
• The Higgs Boson by the CERN exploratorium.
• Particle Fever, documentary film about the search for the Higgs Boson.
• The Atom Smashers, documentary film about the search for the Higgs Boson at Fermilab.
• Collected Articles at the Guardian
• Video (04:38) – CERN Announcement on 4 July 2012, of the discovery of a particle which is suspected will be a Higgs Boson.
• Video1 (07:44) + Video2 (07:44) – Higgs Boson Explained by CERN Physicist, Dr. Daniel Whiteson (16 June 2011).
• HowStuffWorks: What exactly is the Higgs Boson?
• Carroll, Sean. "Higgs Boson with Sean Carroll". Sixty Symbols. University of Nottingham.
• Overbye, Dennis (5 March 2013). "Chasing the Higgs Boson: How 2 teams of rivals at CERN searched for physics' most elusive particle". New York Times Science pages. Retrieved 22 July 2013. – New York Times "behind the scenes" style article on the Higgs' search at ATLAS and CMS
• The story of the Higgs theory by the authors of the PRL papers and others closely associated:
  • Higgs, Peter (2010). "My Life as a Boson" (PDF). Talk given at Kings College, London, 24 November 2010. Archived from the original (PDF) on 4 November 2013. Retrieved 17 January 2013. (also: Higgs, Peter (24 November 2010). "My Life As a Boson: The Story of "the Higgs"". International Journal of Modern Physics A. 17: 86–88. Bibcode:2002IJMPA..17S..86H. doi:10.1142/S0217751X02013046.)
  • Kibble, Tom (2009). "Englert–Brout–Higgs–Guralnik–Hagen–Kibble mechanism (history)". Scholarpedia. Retrieved 17 January 2013. (also: Kibble, Tom (2009). "Englert-Brout-Higgs-Guralnik-Hagen-Kibble mechanism (history)". Scholarpedia. 4 (1): 8741. Bibcode:2009SchpJ...4.8741K. doi:10.4249/scholarpedia.8741.)
  • Guralnik, Gerald (2009). "The History of the Guralnik, Hagen and Kibble development of the Theory of Spontaneous Symmetry Breaking and Gauge Particles". International Journal of Modern Physics A. 24 (14): 2601–2627. arXiv:0907.3466. Bibcode:2009IJMPA..24.2601G. doi:10.1142/S0217751X09045431. S2CID 16298371., Guralnik, Gerald (2011). "The Beginnings of Spontaneous Symmetry Breaking in Particle Physics. Proceedings of the DPF-2011 Conference, Providence, RI, 8–13 August 2011". arXiv:1110.2253v1 ., and Guralnik, Gerald (2013). "Heretical Ideas that Provided the Cornerstone for the Standard Model of Particle Physics". Archived 15 October 2013 at the Wayback Machine SPG Mitteilungen March 2013, No. 39, (p. 14), and Talk at Brown University about the 1964 PRL papers
  • Philip Anderson (not one of the PRL authors) on symmetry breaking in superconductivity and its migration into particle physics and the PRL papers
• Cartoon about the search
• Cham, Jorge (19 February 2014). "True Tales from the Road: The Higgs Boson Re-Explained". Piled Higher and Deeper. Retrieved 25 February 2014.
• Higgs Boson, BBC Radio 4 discussion with Jim Al-Khalili, David Wark & Roger Cashmore (In Our Time, 18 November 2004)

Significant papers and other

• "Observation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC". Physics Letters B. 716 (2012): 1–29. 2012. arXiv:1207.7214. Bibcode:2012PhLB..716....1A. doi:10.1016/j.physletb.2012.08.020. S2CID 119169617.
• "Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC". Physics Letters B. 716 (2012): 30–61. 2012. arXiv:1207.7235. Bibcode:2012PhLB..716...30C. doi:10.1016/j.physletb.2012.08.021.
• Particle Data Group: Review of searches for Higgs Bosons.
• 2001, a spacetime odyssey: proceedings of the Inaugural Conference of the Michigan Center for Theoretical Physics : Michigan, 21–25 May 2001, (pp. 86–88), ed. Michael J. Duff, James T. Liu, ISBN 978-981-238-231-3, containing Higgs' story of the Higgs Boson.
• Migdal, A. A.; Polyakov, A. M. (1966). "Spontaneous Breakdown of Strong Interaction Symmetry and the Absence of Massless Particles" (PDF). Soviet Physics JETP. 24 (1): 91. Bibcode:1967JETP...24...91M. S2CID 34510322. Archived from the original (PDF) on 21 September 2018. – example of a 1966 Russian paper on the subject.

Introductions to the field

• Electroweak Symmetry Breaking – A pedagogic introduction to electroweak symmetry breaking with step by step derivations of many key relations, by Robert D. Klauber, 15 January 2018 (archived at Wayback Machine)
• Spontaneous symmetry breaking, gauge theories, the Higgs mechanism and all that (Bernstein, Reviews of Modern Physics Jan 1974) – an introduction of 47 pages covering the development, history and mathematics of Higgs theories from around 1950 to 1974.

v t e Particles in physics
Elementary	Fermions Quarks Up (quark antiquark) Down (quark antiquark) Charm (quark antiquark) Strange (quark antiquark) Top (quark antiquark) Bottom (quark antiquark) Leptons Electron Positron Muon Antimuon Tau Antitau Neutrino Electron neutrino Electron antineutrino Muon neutrino Muon antineutrino Tau neutrino Tau antineutrino Bosons Gauge Photon Gluon W and Z bosons Scalar Higgs boson Ghost fields Faddeev–Popov ghosts Hypothetical Superpartners Gauginos Gluino Gravitino Photino Others Axino Chargino Higgsino Neutralino Sfermion (Stop squark) Others Axion Curvaton Dilaton Dual graviton Graviphoton Graviton Inflaton Leptoquark Magnetic monopole Majoron Majorana fermion Dark photon Preon Sterile neutrino Tachyon W′ and Z′ bosons X and Y bosons
Composite	Hadrons Baryons Nucleon Proton Antiproton Neutron Antineutron Delta baryon Lambda baryon Sigma baryon Xi baryon Omega baryon Mesons Pion Rho meson Eta and eta prime mesons Bottom eta meson Phi meson J/psi meson Omega meson Upsilon meson Kaon B meson D meson Quarkonium Exotic hadrons Tetraquark (Double-charm tetraquark) Pentaquark Others Atomic nuclei Atoms Exotic atoms Positronium Muonium Tauonium Onia Pionium Protonium Superatoms Molecules Hypothetical Baryons Hexaquark Heptaquark Skyrmion Mesons Glueball Theta meson T meson Others Mesonic molecule Pomeron Diquark R-hadron
Quasiparticles	Anyon Davydov soliton Dropleton Exciton Fracton Hole Magnon Phonon Plasmaron Plasmon Polariton Polaron Roton Trion
Lists	Baryons Mesons Particles Quasiparticles Timeline of particle discoveries
Related	History of subatomic physics timeline Standard Model mathematical formulation Subatomic particles Particles Antiparticles Nuclear physics Eightfold way Quark model Exotic matter Massless particle Relativistic particle Virtual particle Wave–particle duality Particle chauvinism
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v t e Standard Model
Background	Particle physics Fermions Gauge boson Higgs boson Quantum field theory Gauge theory Strong interaction Color charge Quantum chromodynamics Quark model Electroweak interaction Weak interaction Quantum electrodynamics Fermi's interaction Weak hypercharge Weak isospin
Constituents	CKM matrix Spontaneous symmetry breaking Higgs mechanism Mathematical formulation of the Standard Model
Beyond the Standard Model	Evidence Hierarchy problem Dark matter Cosmological constant problem Strong CP problem Neutrino oscillation Theories Technicolor Kaluza–Klein theory Grand Unified Theory Theory of everything Supersymmetry MSSM NMSSM Split supersymmetry Supergravity Quantum gravity String theory Superstring theory Loop quantum gravity Causal dynamical triangulation Canonical quantum gravity Superfluid vacuum theory Twistor theory
Experiments	Gran Sasso INO LHC SNO Super-K Tevatron
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