Pair production

Pair production refers to the creation of an elementary particle and its antiparticle. This is allowed, provided there is enough energy and momentum available to create their mass and motion, because they have opposite quantum numbers (which are therefore conserved in the process).

Related Topics:
Elementary particle - Antiparticle - Energy - Momentum - Quantum numbers

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In nuclear physics, this occurs when a high-energy photon interacts with an atomic nucleus, allowing it to decay into an electron and a positron without violating conservation of momentum. It is the chief method by which energy from gamma rays is observed in condensed matter. The photon need only have a total energy of twice the electron mass (i.e. 1.02 MeV) for this to occur; if it is much more energetic, heavier particles may also be produced. These interactions were first observed in Patrick Maynard Stuart Blackett's counter-controlled bubble chamber, leading to the 1948 Nobel prize for physics.

Related Topics:
Nuclear physics - Photon - Electron - Positron - Conservation of momentum - Gamma rays - Matter - MeV - Patrick Maynard Stuart Blackett - Bubble chamber - 1948 - Nobel prize

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In semiclassical general relativity, pair production is also invoked to explain the Hawking radiation effect. According to quantum mechanics, at short scales short-lived particle-pairs are constantly appearing and disappearing (see quantum foam); in a region of strong gravitational tidal forces, the two particles in a pair may sometimes be wrenched apart before they have a chance to mutually annihilate. When this happens in the region around a black hole, one particle may escape, with its antiparticle being captured by the hole.

Related Topics:
Semiclassical - General relativity - Hawking radiation - Quantum mechanics - Quantum foam - Tidal forces - Annihilate - Black hole

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