Preon

In

have six preons, and quarks and leptons have only three.

In the

elements.

When the term "preon" was coined, it was primarily to explain the two families of spin-1/2 fermions: quarks and leptons. More recent preon models also account for spin-1 bosons, and are still called "preons". Each of the preon models postulates a set of fewer fundamental particles than those of the Standard Model, together with the rules governing how those fundamental particles combine and interact. Based on these rules, the preon models try to explain the Standard Model, often predicting small discrepancies with this model and generating new particles and certain phenomena which do not belong to the Standard Model.

Goals of preon models

Preon research is motivated by the desire to:

• Reduce the large number of particles, many that differ only in charge, to a smaller number of more fundamental particles. For example, the
  periodic table of elements and the quark model
  of mesons and baryons.
• Explain the reason for there being exactly three
  fermions
  .
• Calculate parameters that are currently unexplained by the Standard Model, such as the masses of S.M. fundamental fermions, their electric charges, and color charges; in effect, reduce the number of model-required experimental input parameters from the number required by the Standard Model.
• Provide reasons for the very large range of mass-energy observed in supposedly fundamental particles, from the electron neutrino to the top quark.
• Provide alternative explanations for the
  which?
  ]).
• Account for neutrino oscillation and apparently unique mass mechanism.
• Make new, non-repetitive predictions, such as providing cold dark matter candidates.
• Explain why there exists only the observed variety of particle species, and give a model with reasons for producing only these observed particles (since the prediction of non-observed particles is a problem with many current models, such as supersymmetry).

Background

Before the Standard Model was developed in the 1970s (the key elements of the Standard Model known as quarks were proposed by Murray Gell-Mann and George Zweig in 1964), physicists observed hundreds of different kinds of particles in particle accelerators. These were organized into relationships on their physical properties in a largely ad-hoc system of hierarchies, not entirely unlike the way taxonomy grouped animals based on their physical features. Not surprisingly, the huge number of particles was referred to as the "particle zoo".

The Standard Model, which is now the prevailing model of particle physics, dramatically simplified this picture by showing that most of the observed particles were mesons, which are combinations of two quarks, or baryons which are combinations of three quarks, plus a handful of other particles. The particles being seen in the ever-more-powerful accelerators were, according to the theory, typically nothing more than combinations of these quarks.

Comparisons of quarks, leptons, and bosons

Within the Standard Model, there are several classes of particles. One of these, the quarks, has six types, of which there are three varieties in each (dubbed "colors", red, green, and blue, giving rise to quantum chromodynamics).

Additionally, there are six different types of what are known as leptons. Of these six leptons, there are three charged particles: the electron, muon, and tau. The neutrinos comprise the other three leptons, and each neutrino pairs with one the three charged leptons.

In the Standard Model, there are also bosons, including the photons and gluons; W⁺, W⁻, and Z bosons; and the Higgs boson; and an open space left for the graviton. Almost all of these particles come in "left-handed" and "right-handed" versions (see chirality). The quarks, leptons, and W boson all have antiparticles with opposite electric charge (or in the case of the neutrinos, opposite weak isospin).

Unresolved problems with the Standard Model

The Standard Model also has a number of problems which have not been entirely solved. In particular, no successful theory of

based on a particle theory has yet been proposed. Although the Model assumes the existence of a graviton, all attempts to produce a consistent theory based on them have failed.

Kalman

The Standard Model also has problems predicting the large scale structure of the universe. For instance, the SM generally predicts equal amounts of matter and antimatter in the universe. A number of attempts have been made to "fix" this through a variety of mechanisms, but to date none have won widespread support. Likewise, basic adaptations of the Model suggest the presence of proton decay, which has not yet been observed.

Motivation for preon models

Several models have been proposed in an attempt to provide a more fundamental explanation of the results in experimental and theoretical particle physics, using names such as "parton" or "preon" for the hypothetical basic particle constituents.

Preon theory is motivated by a desire to replicate in particle physics the achievements of the

.

However, the particular preon model discussed below has attracted comparatively little interest among the particle physics community to date, in part because no evidence has been obtained so far in collider experiments to show that the fermions of the Standard Model are composite.

Attempts

A number of physicists have attempted to develop a theory of "pre-quarks" (from which the name preon derives) in an effort to justify theoretically the many parts of the Standard Model that are known only through experimental data. Other names which have been used for these proposed fundamental particles (or particles intermediate between the most fundamental particles and those observed in the Standard Model) include prequarks, subquarks, maons,[6] alphons, quinks, rishons, tweedles, helons, haplons, Y-particles,^[7] and primons.^[8] Preon is the leading name in the physics community.

Efforts to develop a substructure date at least as far back as 1974 with a paper by Pati and Salam in Physical Review.^[9] Other attempts include a 1977 paper by Terazawa, Chikashige, and Akama,^[10] similar, but independent, 1979 papers by Ne'eman,^[11] Harari,^[12] and Shupe,^[13] a 1981 paper by Fritzsch and Mandelbaum,^[14] and a 1992 book by D'Souza and Kalman.^[1] None of these have gained wide acceptance in the physics world. However, in a recent work^[15] de Souza has shown that his model describes well all weak decays of hadrons according to selection rules dictated by a quantum number derived from his compositeness model. In his model leptons are elementary particles and each quark is composed of two primons, and thus, all quarks are described by four primons. Therefore, there is no need for the Standard Model Higgs boson and each quark mass is derived from the interaction between each pair of primons by means of three Higgs-like bosons.

In his 1989 Nobel Prize acceptance lecture, Hans Dehmelt described a most fundamental elementary particle, with definable properties, which he called the cosmon, as the likely result of a long but finite chain of increasingly more elementary particles.^[16]

Composite Higgs

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Many preon models either do not account for the Higgs boson or rule it out, and propose that electro-weak symmetry is broken not by a scalar Higgs field but by composite preons.^[17] For example, Fredriksson preon theory does not need the Higgs boson, and explains the electro-weak breaking as the rearrangement of preons, rather than a Higgs-mediated field. In fact, the Fredriksson preon model and the de Souza model predict that the Standard Model Higgs boson does not exist.

Rishon model

The rishon model (RM) is the earliest effort (1979) to develop a preon model to explain the phenomenon appearing in the Standard Model (SM) of particle physics. It was first developed by Haim Harari and Michael A. Shupe (independently of each other), and later expanded by Harari and his then-student Nathan Seiberg.^[18]

The model has two kinds of fundamental particles called rishons (ראשונים) (which means "First" in

.

The Rishon model illustrates some of the typical efforts in the field. Many of the preon models theorize that the apparent imbalance of matter and antimatter in the universe is in fact illusory, with large quantities of preon-level antimatter confined within more complex structures.

Criticisms

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The mass paradox

One preon model started as an internal paper at the Collider Detector at

of an up-quark, and 400,000 times larger than the rest mass of an electron.

Heisenberg's uncertainty principle states that ${\displaystyle \operatorname {\Delta } x\cdot \operatorname {\Delta } p\geq {\tfrac {1}{2}}\hbar }$ and thus anything confined to a box smaller than ${\displaystyle \operatorname {\Delta } x}$ would have a momentum uncertainty proportionally greater. Thus, the preon model proposed particles smaller than the elementary particles they make up, since the momentum uncertainty ${\displaystyle \operatorname {\Delta } p}$ should be greater than the particles themselves.

So the preon model represents a mass paradox: How could quarks or electrons be made of smaller particles that would have many orders of magnitude greater mass-energies arising from their enormous momenta? One way of resolving this paradox is to postulate a large binding force between preons that cancels their mass-energies.^{[citation needed]}

Conflicts with observed physics

Preon models propose additional unobserved forces or dynamics to account for the observed properties of elementary particles, which may have implications in conflict with observation. For example, now that the LHC's observation of a Higgs boson is confirmed, the observation contradicts the predictions of many preon models that excluded it.^{[citation needed]}

Preon theories require quarks and leptons to have a finite size. It is possible that the Large Hadron Collider will observe this after it is upgraded to higher energies.^{[citation needed]}

In popular culture

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• In the 1948 reprint/edit of his 1930 novel
  Skylark Three, E. E. Smith
  postulated a series of 'subelectrons of the first and second type' with the latter being fundamental particles that were associated with the gravitation force. While this may not have been an element of the original novel (the scientific basis of some of the other novels in the series was revised extensively due to the additional eighteen years of scientific development), even the edited publication may be the first, or one of the first, mentions of the possibility that electrons are not fundamental particles.
• In the novelized version of the 1982 motion picture
  Vonda McIntyre
  , two of Dr. Carol Marcus' Genesis project team, Vance Madison and Delwyn March, have studied sub-elementary particles they've named "boojums" and "snarks", in a field they jokingly call "kindergarten physics" because it is lower than "elementary" (analogy to school levels).
• James P. Hogan's 1982 novel Voyage from Yesteryear discussed preons (called tweedles), the physics of which became central to the plot.
• In the 2020 video game Risk of Rain 2, an item in the game is called the 'preon accumulator', though only a reference in name.

See also

• Technicolor (physics) – Hypothetical model through which W and Z bosons acquire mass
• Preon star
   – Hypothetical compact star made of exotic matterPages displaying short descriptions of redirect targets
• Preon-degenerate matter
   – Type of dense exotic matter in physicsPages displaying short descriptions of redirect targets
• Rishon model – preonic model of sub-quark particle physicsPages displaying wikidata descriptions as a fallback

References

1. ^ ^{a b} D'Souza, I.A.; Kalman, C.S. (1992). Preons: Models of Leptons, Quarks and Gauge Bosons as Composite Objects.
   ISBN 978-981-02-1019-9
   .
2. doi:10.1103/RevModPhys.28.214
   .
3. doi:10.1103/RevModPhys.30.482. Archived
   (PDF) from the original on 2018-02-23.
4. S2CID 119394495
   .
5. doi:10.4279/PIP.030003
   .
6. ^ Overbye, D. (5 December 2006). "China pursues major role in particle physics". The New York Times. Retrieved 2011-09-12.
7. ^ Yershov, V.N. (2005). "Equilibrium configurations of tripolar charges".
   S2CID 119474883
   .
8. ^ de Souza, M.E. (2005). "The ultimate division of matter". Scientia Plena. 1 (4): 83.
9. ^ Pati, J.C.; Salam, A. (1974). "Lepton number as the fourth "color"" (PDF).
   S2CID 17349483. Archived from the original
   (PDF) on 2019-02-20.
   Erratum: Pati, J.C.; Salam, A. (1975). "Erratum: Lepton number as the fourth "color"".
   doi:10.1103/PhysRevD.11.703.2
   .
10. ^ Terazawa, H.; Chikashige, Y.; Akama, K. (1977). "Unified model of the Nambu-Jona-Lasinio type for all elementary particles".
    doi:10.1103/PhysRevD.15.480
    .
11. ^ Ne'eman, Y. (1979). "Irreducible gauge theory of a consolidated Weinberg-Salam model".
    OSTI 6534180
    .
12. ^ Harari, H. (1979). "A schematic model of quarks and leptons" (PDF).
    OSTI 1447265
    .
13. ^ Shupe, M.A. (1979). "A composite model of leptons and quarks".
    doi:10.1016/0370-2693(79)90627-0
    .
14. ^ Fritzsch, H.; Mandelbaum, G. (1981). "Weak interactions as manifestations of the substructure of leptons and quarks".
    doi:10.1016/0370-2693(81)90626-2
    .
15. ^ de Souza, M.E. (2008). "Weak decays of hadrons reveal compositeness of quarks". Scientia Plena. 4 (6): 064801–1.
16. ^ Dehmelt, H.G. (1989). "Experiments with an isolated subatomic particle at rest". Nobel lecture.
    The Nobel Foundation
    . See also references therein.
17. arXiv:hep-ph/9709227
    .
18. doi:10.1016/0550-3213(82)90426-6. Archived from the original
    (PDF) on 2012-10-07. Retrieved 2018-06-02.

Further reading

• Ball, P. (2007). "Splitting the quark".
  doi:10.1038/news.2007.292
  .
• Piccioni, Robert (2013-01-07). "Have we hit bottom yet?". guidetothecosmos.com. newsletter. — an editorial about preons