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Pion

Subatomic particle; lightest meson

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Through Pi (letter), Subatomic particle and Gamma ray

The exchange of virtual pions, along with vector, rho and omega mesons, provides an explanation for the residual strong force between nucleons. Pions are not produced in radioactive decay, but commonly are in high-energy collisions between hadrons. 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.

History

Theoretical work by Hideki Yukawa in 1935 had predicted the existence of mesons as the carrier particles of the strong nuclear force. From the range of the strong nuclear force (inferred from the radius of the atomic nucleus), Yukawa predicted the existence of a particle having a mass of about 100 MeV/c2. Initially after its discovery in 1936, the muon (initially called the "mesotron" or the "mu meson") was thought to be this particle, since it has a mass of 106 MeV/c2. However, later experiments showed that the muon did not participate in the strong nuclear interaction. In modern terminology, this makes the muon a lepton, and not a meson. The pions, which were later identified as the mesons predicted by Yukawa, were confirmed afterward: charged pions in 1947 and neutral pions in 1950.

In 1941–42, Bibha Chowdhuri and Debendra Mohan Bose reported cosmic-ray meson tracks at the Bose Institute that later historians have regarded as early evidence of pions. Although particle accelerators had already been developed by the early 1930s, atmospheric cosmic rays remained the principal source of high-energy subatomic particles until high-energy accelerators became available in the early 1950s. Photographic emulsions were placed for long periods of time in sites located atop Mount Sandakphu in present-day West Bengal and in the higher town of Pharijong in Tibet. The particles recorded at Sandakphu (about 221 me [113 MeV/c2]) were lighter than those observed at Pharijong (about 278 me [142 MeV/c2]), which led to a tentative conclusion that the lighter ones (the muons) were the decay product of the heavier ones (the pions). However, follow-up studies could not be conducted because only halftone plates were available during World War II. A study in 1947 by the collaboration led by Cecil Powell at the University of Bristol in England obtained more conclusive results with fulltone plates at Pic du Midi de Bigorre in the Pyrenees, and later at Chacaltaya in the Andes Mountains, for which Powell won the 1950 Nobel Prize in Physics. Marietta Kurz was the first person to detect the unusual "double meson" tracks upon inspecting the Powell team's plates, 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, and the previous study by Chowdhuri and Bose was credited as well.

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 alpha particles. Further advanced theoretical work was carried out by Riazuddin, who in 1959 used the dispersion relation for Compton scattering of virtual photons on pions to analyze their charge radius.

Since the neutral pion is not electrically charged, it is more difficult to detect and observe than the charged pions are. Neutral pions do not leave tracks in photographic emulsions or Wilson cloud chambers. The existence of the neutral pion was inferred from observing its decay products from cosmic rays, a so-called "soft component" of slow electrons with photons. The π0
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.

... Yukawa choose the letter π because of its resemblance to the Kanji character for 介 [kai], which means "to mediate", based on the idea that the meson works as a strong force mediator particle between hadrons.

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Source and licence. Adapted from the Wikipedia article “Pion” (this version, 2026-07-15) by its contributors, shared under CC BY-SA 4.0. Lablypedia has left out its tables, references and most pictures, and linked it to other Lablypedia articles.