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・ PAIR
・ Pair
・ Pair (parliamentary convention)
・ PAIR (puncture-aspiration-injection-reaspiration)
・ Pair a Dice Found
・ Pair bond
・ Pair by association
・ Pair Dadeni
・ Pair distribution function
・ Pair gain
・ Pair Of Dice Paradise
・ Pair of Kings
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・ Pair of spaces
・ Pair potential
Pair production
・ Pair programming
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・ Pair trawling
・ Pair-conversion
・ Pair-et-Grandrupt
・ Pair-instability supernova
・ Pair-rule gene
・ Paira
・ Pairagachha
・ Pairan
・ Pairat Decharin
・ Pairatahi River
・ Pairc nan Laoch


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Pair production : ウィキペディア英語版
Pair production

Pair production is the creation of an elementary particle and its antiparticle, for example creating an electron and positron, a muon and antimuon, or a proton and antiproton. Pair production often refers specifically to a photon creating an electron-positron pair near a nucleus but can more generally refer to any neutral boson creating a particle-antiparticle pair. In order for pair production to occur, the incoming energy of the interaction must be above a threshold in order to create the pair at least the total rest mass energy of the two particles and that the situation allows both energy and momentum to be conserved. However, all other conserved quantum numbers (angular momentum, electric charge, lepton number) of the produced particles must sum to zero thus the created particles shall have opposite values of each other. For instance, if one particle has electric charge of +1 the other must have electric charge of −1, or if one particle has strangeness of +1 then another one must have strangeness of −1. The probability of pair production in photon-matter interactions increases with photon energy and also increases approximately as the square of atomic number.
== Photon to electron and positron ==

For photons at high-energy, (MeV scale and higher) pair production is the dominant mode of photon interaction with matter. These interactions were first observed in Patrick Blackett's counter-controlled cloud chamber, leading to the 1948 Nobel Prize in Physics. If the photon is near an atomic nucleus, the energy of a photon can be converted into an electron-positron pair:
→  + 
The photon's energy is converted to particle's mass through ; where is energy, is mass and 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
* 0.511 MeV = 1.022 MeV) for the production to occur. The photon must be near a nucleus in order to satisfy conservation of momentum, as an electron-positron pair producing in free space cannot both satisfy conservation of energy and momentum. Because of this, when pair production occurs, the atomic nucleus receives some recoil. The reverse of this process is electron positron annihilation.

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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