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Lepton

In particle physics, a lepton is an elementary particle of half-integer spin (spin 1/2) that does not undergo strong interactions.[1] Two main classes of leptons exist: charged leptons (also known as the electron-like leptons or muons), including the electron, muon, and tauon, and neutral leptons, better known as neutrinos. Charged leptons can combine with other particles to form various composite particles such as atoms and positronium, while neutrinos rarely interact with anything, and are consequently rarely observed. The best known of all leptons is the electron.

Not to be confused with leptin or Lipton.

There are six types of leptons, known as flavours, grouped in three generations.[2] The first-generation leptons, also called electronic leptons, comprise the electron (
e
) and the electron neutrino (
ν
e
); the second are the muonic leptons, comprising the muon (
μ
) and the muon neutrino (
ν
μ
); and the third are the tauonic leptons, comprising the tau (
τ
) and the tau neutrino (
ν
τ
). Electrons have the least mass of all the charged leptons. The heavier muons and taus will rapidly change into electrons and neutrinos through a process of particle decay: the transformation from a higher mass state to a lower mass state. Thus electrons are stable and the most common charged lepton in the universe, whereas muons and taus can only be produced in high-energy collisions (such as those involving cosmic rays and those carried out in particle accelerators).


Leptons have various intrinsic properties, including electric charge, spin, and mass. Unlike quarks, however, leptons are not subject to the strong interaction, but they are subject to the other three fundamental interactions: gravitation, the weak interaction, and to electromagnetism, of which the latter is proportional to charge, and is thus zero for the electrically neutral neutrinos.


For every lepton flavor, there is a corresponding type of antiparticle, known as an antilepton, that differs from the lepton only in that some of its properties have equal magnitude but opposite sign. According to certain theories, neutrinos may be their own antiparticle. It is not currently known whether this is the case.


The first charged lepton, the electron, was theorized in the mid-19th century by several scientists[3][4][5] and was discovered in 1897 by J. J. Thomson.[6] The next lepton to be observed was the muon, discovered by Carl D. Anderson in 1936, which was classified as a meson at the time.[7] After investigation, it was realized that the muon did not have the expected properties of a meson, but rather behaved like an electron, only with higher mass. It took until 1947 for the concept of "leptons" as a family of particles to be proposed.[8] The first neutrino, the electron neutrino, was proposed by Wolfgang Pauli in 1930 to explain certain characteristics of beta decay.[8] It was first observed in the Cowan–Reines neutrino experiment conducted by Clyde Cowan and Frederick Reines in 1956.[8][9] The muon neutrino was discovered in 1962 by Leon M. Lederman, Melvin Schwartz, and Jack Steinberger,[10] and the tau discovered between 1974 and 1977 by Martin Lewis Perl and his colleagues from the Stanford Linear Accelerator Center and Lawrence Berkeley National Laboratory.[11] The tau neutrino remained elusive until July 2000, when the DONUT collaboration from Fermilab announced its discovery.[12][13]


Leptons are an important part of the Standard Model. Electrons are one of the components of atoms, alongside protons and neutrons. Exotic atoms with muons and taus instead of electrons can also be synthesized, as well as lepton–antilepton particles such as positronium.

Koide formula

List of particles

– hypothetical particles that were once postulated to be subcomponents of quarks and leptons

Preons

Anicin, I. V. (2005). "The Neutrino: Its Past, Present and Future". :physics/0503172.

arXiv

Fukuda, Y.; et al. (1998). "Evidence for Oscillation of Atmospheric Neutrinos". Physical Review Letters. 81 (8): 1562–1567. :hep-ex/9807003. Bibcode:1998PhRvL..81.1562F. doi:10.1103/PhysRevLett.81.1562. S2CID 7102535.

arXiv

Kodama, K.; et al. (2001). "Observation of tau neutrino interactions". Physics Letters B. 504 (3): 218–224. :hep-ex/0012035. Bibcode:2001PhLB..504..218D. doi:10.1016/S0370-2693(01)00307-0. S2CID 119335798.

arXiv

B. R. Martin; G. Shaw (1992). . Particle Physics. John Wiley & Sons. pp. 23–47. ISBN 978-0-471-92358-9.

"Chapter 2: Leptons, quarks and hadrons"

Neddermeyer, S. H.; Anderson, C. D. (1937). (PDF). Physical Review. 51 (10): 884–886. Bibcode:1937PhRv...51..884N. doi:10.1103/PhysRev.51.884.

"Note on the Nature of Cosmic-Ray Particles"

Perl, M. L.; et al. (1975). "Evidence for Anomalous Lepton Production in e+–e Annihilation". . 35 (22): 1489–1492. Bibcode:1975PhRvL..35.1489P. doi:10.1103/PhysRevLett.35.1489.

Physical Review Letters

Peskin, M. E.; Schroeder, D. V. (1995). . Westview Press. ISBN 978-0-201-50397-5.

Introduction to Quantum Field Theory

Riesselmann, K. (2007). . Symmetry Magazine. 4 (2). Archived from the original on 31 May 2009.

"Logbook: Neutrino Invention"

Rosenfeld, L. (1948). Nuclear Forces. . p. xvii.

Interscience Publishers

Shankar, R. (1994). "Chapter 2: Rotational Invariance and Angular Momentum". Principles of Quantum Mechanics (2nd ed.). . pp. 305–352. ISBN 978-0-306-44790-7.

Springer

Weinberg, S. (2003). . Cambridge University Press. ISBN 978-0-521-82351-7.

The Discovery of Subatomic Particles

Wilson, R. (1997). Astronomy Through the Ages: The Story of the Human Attempt to Understand the Universe. . p. 138. ISBN 978-0-7484-0748-4.

CRC Press

. – The PDG compiles authoritative information on particle properties.

"Particle Data Group homepage"

. Physics & Astronomy. Georgia State University. Hyperphysics. – a summary of leptons.

"Leptons"