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Baryon
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Baryons are the family of subatomic particles with a baryon number of 1. The term baryon is usually used to refer to triquarks — baryons made of three quarks. "Exotic" baryons made of four quarks and one antiquark, are known as the pentaquarks, but their existence is not generally accepted. Each baryon has a corresponding antiparticle (anti-baryon) where quarks are replaced by their corresponding antiquarks and their corresponding antiquarks replaced by quarks. Amongst the baryons are the protons and neutrons, which make up atomic nuclei, but many other unstable baryons exist as well. The term "baryon" is derived from the Greek (barys), meaning "heavy," because at the time of their naming it was believed that baryons were characterized by having greater mass than other particles.
Baryons are a subset of the hadrons (which are the particles made of quarks) and participate in the strong interaction.
BackgroundBaryons are strongly interacting fermions — that is, they experience the strong nuclear force and are described by Fermi-Dirac statistics, which apply to all particles obeying the Pauli exclusion principle. This is in contrast to the bosons, which do not obey the exclusion principle.
Baryons, along with mesons, are hadrons, meaning they are particles composed of quarks. Quarks have baryon numbers of B = and antiquarks have baryon number of B = -. The term "baryon" usually refer to triquarks—baryons mades of three quarks (B = + + = 1), but there are other "exotic" baryons, such as pentaquarks — baryons made of four quarks and one antiquark (B = + + + - = 1), but their existence is not generally accepted. Theoretically, heptaquarks (5 quarks, 2 antiquarks), nonaquarks (6 quarks, 3 antiquarks), etc. could also exist.
Classification
Baryons are classified into groups according to their isospin values and quark content. There are six groups of triquarks — nucleon , Delta , Lambda , Sigma , Xi , and Omega . The rules for classification are defined by the Particle Data Group. These rules consider the , and quarks to be light and the , , and to be heavy. The rules cover all the particles that can be made from three of each of the six quarks — even though baryons made of top quarks are not expected to exist because of the top quark's short lifetime—but not pentaquarks.:
- Baryons with three and/or quarks are 's or 's (isospin ).
- Baryons with two and/or quarks are 's (isospin 0) or 's (isospin 1). If the third quark is heavy, its identity is given by a subscript.
- Baryons with one or quark are 's (isospin ). One or two subscripts are used if one or both of the remaining quarks are heavy.
- Baryons with no or quarks are 's (isospin 0), and subscripts indicate any heavy quark content.
- Baryons that decay strongly have their masses as part of their names. For example, Sigmas and Omegas do not decay strongly, but Deltas , and charmed Xis do.
Quarks carry charge, so knowing the charge of a particle indirectly gives the quark content. For example, the rules above say that the contains a bottom and some combination of two up and/or down quarks. A must be one up quark (Q=), one down quark (Q=−), and one bottom quark (Q=−) to have the correct charge (Q=0).
The number of baryons within one group (excluding resonances) is given by the number of isospin projections possible (2 × isospin + 1). For example there are four 's, corresponding to the four isospin projections of the isospin value I = : (Iz = ), (Iz = ), (Iz = −), and (Iz = −). Another example would be the three 's, corresponding to the three isospin projections of the isospin value I = 1: (Iz = 1), (Iz = 0), and (Iz = −1).
Baryonic matterBaryonic matter is matter composed mostly of baryons (by mass), which includes atoms of any sort (and thus includes nearly all matter that we may encounter or experience in everyday life, including our bodies). Non-baryonic matter, as implied by the name, is any sort of matter that is not primarily composed of baryons. This might include such ordinary matter as neutrinos or free electrons; however, it may also include exotic species of non-baryonic dark matter, such as supersymmetric particles, axions or black holes. The distinction between baryonic and non-baryonic matter is important in cosmology, because Big Bang nucleosynthesis models set tight constraints on the amount of baryonic matter present in the early universe.
The very existence of baryons is also a significant issue in cosmology because we have assumed that the Big Bang produced a state with equal amounts of baryons and anti-baryons. The process by which baryons come to outnumber their antiparticles is called baryogenesis (in contrast to a process by which leptons account for the predominance of matter over antimatter, leptogenesis).
BaryogenesisExperiments are consistent with the number of quarks in the universe being a constant and, more specifically, the number of baryons being a constant; in technical language, the total baryon number appears to be conserved. Within the prevailing Standard Model of particle physics, the number of baryons may change in multiples of three due to the action of sphalerons, although this is rare and has not been observed experimentally. Some grand unified theories of particle physics also predict that a single proton can decay, changing the baryon number by one; however, this has not yet been observed experimentally. The excess of baryons over antibaryons in the present universe is thought to be due to non-conservation of baryon number in the very early universe, though this is not well understood.
See also
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