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  2. Pion - Wikipedia

    en.wikipedia.org/wiki/Pion

    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 π 0 was identified definitively at the University of California's cyclotron in 1949 by observing its decay into two photons. [7]

  3. Proton decay - Wikipedia

    en.wikipedia.org/wiki/Proton_decay

    Here, a proton, consisting of two up quarks and a down, decays into a pion, consisting of an up and anti-up, and a positron, via an X boson with electric charge − ⁠ 4 / 3 ⁠ e. In particle physics, proton decay is a hypothetical form of particle decay in which the proton decays into lighter subatomic particles, such as a neutral pion and a ...

  4. Pair production - Wikipedia

    en.wikipedia.org/wiki/Pair_production

    The photon's energy is converted to particle mass in accordance with Einstein's equation, E = mc 2; where E is energy, m is mass and c is the speed of light. The photon must have higher energy than the sum of the rest mass energies of an electron and positron (2 × 511 keV = 1.022 MeV, resulting in a photon wavelength of 1.2132 pm ) for the ...

  5. Primakoff effect - Wikipedia

    en.wikipedia.org/wiki/Primakoff_effect

    In particle physics, the Primakoff effect, named after Henry Primakoff, is the resonant production of neutral pseudoscalar mesons by high-energy photons interacting with an atomic nucleus. It can be viewed as the reverse process of the decay of the meson into two photons and has been used for the measurement of the decay width of neutral mesons ...

  6. Annihilation - Wikipedia

    en.wikipedia.org/wiki/Annihilation

    When a low-energy electron annihilates a low-energy positron (antielectron), the most probable result is the creation of two or more photons, since the only other final-state Standard Model particles that electrons and positrons carry enough mass–energy to produce are neutrinos, which are approximately 10,000 times less likely to produce, and ...

  7. Pion decay constant - Wikipedia

    en.wikipedia.org/wiki/Pion_decay_constant

    According to Brown–Rho scaling, the masses of nucleons and most light mesons decrease at finite density as the ratio of the in-medium pion decay rate to the free-space pion decay constant. The pion mass is an exception to Brown-Rho scaling because the pion's mass is protected by its Goldstone boson nature. [1]

  8. Chiral anomaly - Wikipedia

    en.wikipedia.org/wiki/Chiral_anomaly

    The Adler–Bell–Jackiw anomaly is seen experimentally, in the sense that it describes the decay of the neutral pion, and specifically, the width of the decay of the neutral pion into two photons. The neutral pion itself was discovered in the 1940s; its decay rate (width) was correctly estimated by J. Steinberger in 1949. [6]

  9. CPLEAR experiment - Wikipedia

    en.wikipedia.org/wiki/CPLEAR_experiment

    This means that for every decay of K 2 into three pions, there are (2.0±0.4)×10-3 decays into two pions. Because of this, neutral K mesons violate CP. [ 2 ] The study of the ratio of neutral kaon and neutral anti-kaons production is thus an efficient tool to understand what happened in the early Universe that promoted the production of matter.

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