}}| statistics = | group = | interaction = Strong, Weak interaction, electromagnetic, and gravity | antiparticle=
| theorized = Hideki Yukawa (1935) | discovered =
| symbol = , , and | mass =
| mean_lifetime =
| decay_particle = | electric_charge =
| charge_radius = :
| color_charge= 0
| spin = 0 ħ
| strangeness =
| charm =
| bottomness =
| topness =
| isospin =
| hypercharge = 0
| parity = −1
| c_parity = +1
In particle physics, a pion (, ) or pi meson, denoted with the Greek alphabet letter pi (), is any of three subatomic particles: , , and . Each pion consists of a quark and an antiquark and is therefore a meson. Pions are the lightest mesons and, more generally, the lightest . They are unstable, with the charged pions and decaying after a mean lifetime of 26.033 ( seconds), and the neutral pion decaying after a much shorter lifetime of 85 ( seconds). Charged pions most often particle decay into and , while neutral pions generally decay into .
The exchange of virtual particle pions, along with vector meson, rho meson and , provides an explanation for the nuclear force between . Pions are not produced in radioactive decay, but commonly are in high-energy collisions between . Pions also result from some matter–antimatter annihilation events. All types of pions are also produced in natural processes when high-energy cosmic-ray protons and other hadronic cosmic-ray components interact with matter in Earth's atmosphere. In 2013, the detection of characteristic gamma rays originating from the decay of neutral pions in two supernova remnants has shown that pions are produced copiously after supernovas, most probably in conjunction with production of high-energy protons that are detected on Earth as cosmic rays.
The pion also plays a crucial role in cosmology, by imposing an upper limit on the energies of cosmic rays surviving collisions with the cosmic microwave background, through the Greisen–Zatsepin–Kuzmin limit.
In 1947, the first true mesons, the charged pions, were found by the collaboration led by Cecil Powell at the University of Bristol, in England. The discovery article had four authors: César Lattes, Giuseppe Occhialini, Hugh Muirhead and Powell. Since the advent of particle accelerators had not yet come, high-energy subatomic particles were only obtainable from atmospheric . Photographic emulsions based on the gelatin-silver process were placed for long periods of time in sites located at high-altitude mountains, first at Pic du Midi de Bigorre in the Pyrenees, and later at Chacaltaya in the Andes Mountains, where the plates were struck by cosmic rays.
After development, the photographic plates were inspected under a microscope by a team of about a dozen women. Marietta Kurz was the first person to detect the unusual "double meson" tracks, characteristic for a pion decaying into a muon, but they were too close to the edge of the photographic emulsion and deemed incomplete. A few days later, Irene Roberts observed the tracks left by pion decay that appeared in the discovery paper. Both women are credited in the figure captions in the article.
In 1948, Lattes, Eugene Gardner, and their team first artificially produced pions at the University of California's cyclotron in Berkeley, California, by bombarding carbon atoms with high-speed . Further advanced theoretical work was carried out by Riazuddin, who in 1959 used the dispersion relation for Compton scattering of on pions to analyze their charge radius.
Since the neutral pion is not electric charge, it is more difficult to detect and observe than the charged pions are. Neutral pions do not leave tracks in photographic emulsions or Wilson . The existence of the neutral pion was inferred from observing its decay products from , a so-called "soft component" of slow electrons with photons. The was identified definitively at the University of California's cyclotron in 1949 by observing its decay into two photons. Later in the same year, they were also observed in cosmic-ray balloon experiments at Bristol University.
In fact, it was shown by Gell-Mann, Oakes and Renner (GMOR) that the square of the pion mass is proportional to the sum of the quark masses times the quark condensate:
with the quark condensate:
This is often known as the GMOR relation and it explicitly shows that in the massless quark limit. The same result also follows from light-front holography.
Empirically, since the light quarks actually have minuscule nonzero masses, the pions also have nonzero . However, those masses are almost an order of magnitude smaller than that of the nucleons, roughly 45 MeV, where are the relevant current quark masses, around .
The pion is one of the particles that mediate the residual strong interaction between a pair of nucleons. This interaction is attractive: it pulls the nucleons together. Written in a non-relativistic form, it is called the Yukawa potential. The pion, being spinless, has kinematics described by the Klein–Gordon equation. In the terms of quantum field theory, the effective field theory Lagrangian describing the pion-nucleon interaction is called the Yukawa interaction.
The nearly identical masses of and indicate that there must be a symmetry at play: this symmetry is called the SU(2) flavour symmetry or isospin. The reason that there are three pions, , and , is that these are understood to belong to the triplet representation or the adjoint representation 3 of SU(2). By contrast, the up and down quarks transform according to the fundamental representation 2 of SU(2), whereas the anti-quarks transform according to the conjugate representation 2*.
With the addition of the strange quark, the pions participate in a larger, SU(3), flavour symmetry, in the adjoint representation, 8, of SU(3). The other members of this octet are the four and the eta meson.
Pions are pseudoscalars under a parity transformation. Pion currents thus couple to the axial vector current and so participate in the chiral anomaly.
The second most common decay mode of a pion, with a branching fraction of 0.000123, is also a leptonic decay into an electron and the corresponding electron antineutrino. This "electronic mode" was discovered at CERN in 1958:
The suppression of the electronic decay mode with respect to the muonic one is given approximately (up to a few percent effect of the radiative corrections) by the ratio of the half-widths of the pion–electron and the pion–muon decay reactions,
and is a spin effect known as helicity suppression.
Its mechanism is as follows: The negative pion has spin zero; therefore the lepton and the antineutrino must be emitted with opposite spins (and opposite linear momenta) to preserve net zero spin (and conserve linear momentum). However, because the weak interaction is sensitive only to the left chirality component of fields, the antineutrino has always left chirality, which means it is right-handed, since for massless anti-particles the helicity is opposite to the chirality. This implies that the lepton must be emitted with spin in the direction of its linear momentum (i.e., also right-handed). If, however, leptons were massless, they would only interact with the pion in the left-handed form (because for massless particles helicity is the same as chirality) and this decay mode would be prohibited. Therefore, suppression of the electron decay channel comes from the fact that the electron's mass is much smaller than the muon's. The electron is relatively massless compared with the muon, and thus the electronic mode is greatly suppressed relative to the muonic one, virtually prohibited.
Although this explanation suggests that parity violation is causing the helicity suppression, the fundamental reason lies in the vector-nature of the interaction which dictates a different handedness for the neutrino and the charged lepton. Thus, even a parity conserving interaction would yield the same suppression.
Measurements of the above ratio have been considered for decades to be a test of lepton universality. Experimentally, this ratio is .
Beyond the purely leptonic decays of pions, some structure-dependent radiative leptonic decays (that is, decay to the usual leptons plus a gamma ray) have also been observed.
Also observed, for charged pions only, is the very rare "pion beta decay" (with branching fraction of about ) into a neutral pion, an electron and an electron antineutrino (or for positive pions, a neutral pion, a positron, and electron neutrino).
The rate at which pions decay is a prominent quantity in many sub-fields of particle physics, such as chiral perturbation theory. This rate is parametrized by the pion decay constant (), related to the wave function overlap of the quark and antiquark, which is about .
The decay (as well as decays into any odd number of photons) is forbidden by the C-symmetry of the electromagnetic interaction: The intrinsic C-parity of the is +1, while the C-parity of a system of photons is .
The second largest decay mode () is the Dalitz decay (named after Richard Dalitz), which is a two-photon decay with an internal photon conversion resulting in a photon and an electron-positron pair in the final state:
The third largest established decay mode () is the double-Dalitz decay, with both photons undergoing internal conversion which leads to further suppression of the rate:
The fourth largest established decay mode is the Feynman diagram and therefore suppressed (and additionally helicity-suppressed) leptonic decay mode ():
The neutral pion has also been observed to decay into positronium with a branching fraction on the order of . No other decay modes have been established experimentally. The branching fractions above are the PDG central values, and their uncertainties are omitted, but available in the cited publication.
History
Possible applications
Theoretical overview
Basic properties
Charged pion decays
Neutral pion decays
a The quark composition of the is not exactly divided between up and down quarks, due to complications from non-zero quark masses.
+ Pions Pion 1− 0− 0 0 0 + Pion Self 1− 0−+ 0 0 0
See also
Further reading
External links
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