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・ Weak equivalence (homotopy theory)
・ Weak evolutionarily stable strategy
・ Weak focusing
・ Weak form and strong form
・ Weak formulation
・ Weak generative capacity
・ Weak gravitational lensing
・ Weak Hausdorff space
・ Weak heap
・ Weak Hopf algebra
・ Weak hypercharge
・ Weak in the Presence of Beauty
・ Weak in the Presence of Beauty (album)
・ Weak in the Presence of Beauty (song)
・ Weak inflection
Weak interaction
・ Weak interpretability
・ Weak inverse
・ Weak isospin
・ Weak key
・ Weak localization
・ Weak measurement
・ Weak Moments of the Shadows
・ Weak n-category
・ Weak noun
・ Weak NP-completeness
・ Weak ontology
・ Weak ontology (political concept)
・ Weak operator topology
・ Weak ordering


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Weak interaction : ウィキペディア英語版
Weak interaction

In particle physics, the weak interaction is the mechanism responsible for the weak force or weak nuclear force, one of the four known fundamental interactions of nature, alongside the strong interaction, electromagnetism, and gravitation. The weak interaction is responsible for the radioactive decay of subatomic particles, and it plays an essential role in nuclear fission. The theory of the weak interaction is sometimes called quantum flavordynamics (QFD), in analogy with the terms QCD and QED, but the term is rarely used because the weak force is best understood in terms of electro-weak theory (EWT).
In the Standard Model of particle physics, the weak interaction is caused by the emission or absorption of W and Z bosons. All known fermions interact through the weak interaction. Fermions are particles that have half-integer spin (one of the fundamental properties of particles). A fermion can be an elementary particle, such as the electron, or it can be a composite particle, such as the proton. The masses of W+, W, and Z bosons are each far greater than that of protons or neutrons, consistent with the short range of the weak force. The force is termed ''weak'' because its field strength over a given distance is typically several orders of magnitude less than that of the strong nuclear force and electromagnetic force.
During the quark epoch, the electroweak force split into the electromagnetic and weak forces. Important examples of weak interaction include beta decay, and the production, from hydrogen, of deuterium needed to power the sun's thermonuclear process. Most fermions will decay by a weak interaction over time. Such decay also makes radiocarbon dating possible, as carbon-14 decays through the weak interaction to nitrogen-14. It can also create radioluminescence, commonly used in tritium illumination, and in the related field of betavoltaics.
Quarks, which make up composite particles like neutrons and protons, come in six "flavours" – up, down, strange, charm, top and bottom – which give those composite particles their properties. The weak interaction is unique in that it allows for quarks to swap their flavour for another. For example, during beta minus decay, a down quark decays into an up quark, converting a neutron to a proton. Also the weak interaction is the only fundamental interaction that breaks parity-symmetry, and similarly, the only one to break CP-symmetry.
==History==
In 1933, Enrico Fermi proposed the first theory of the weak interaction, known as Fermi's interaction. He suggested that beta decay could be explained by a four-fermion interaction, involving a contact force with no range.
However, it is better described as a non-contact force field having a finite range, albeit very short. In 1968, Sheldon Glashow, Abdus Salam and Steven Weinberg unified the electromagnetic force and the weak interaction by showing them to be two aspects of a single force, now termed the electro-weak force.
The existence of the W and Z bosons was not directly confirmed until 1983.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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