thermonuclear reaction

(nuclear physics) A nuclear fusion reaction which occurs between various nuclei of light elements when they are constituents of a gas at very high temperature.

A nuclear fusion reaction which occurs between various nuclei of the light elements when they are constituents of a gas at very high temperatures. Thermonuclear reactions, the source of energy generation in the Sun and the stable stars, are utilized in the fusion bomb. See also Hydrogen bomb; Nuclear fusion; Stellar evolution; Sun.

Thermonuclear reactions occur most readily between isotopes of hydrogen (deuterium and tritium) and less readily among a few other nuclei of higher atomic number. At the temperatures and densities required to produce an appreciable rate of thermonuclear reactions, all matter is completely ionized; that is, it exists only in the plasma state. Thermonuclearer fusion reactions may then occur within such an ionized gas when the agitation energy of the stripped nuclei is sufficient to overcome their mutual electrostatic repulsions, allowing the colliding nuclei to approach each other closely enough to react. For this reason, reactions tend to occur much more readily between energy-rich nuclei of low atomic number (small charge) and particularly between those nuclei of the hot gas which have the greatest relative kinetic energy. This latter fact leads to the result that, at the lower fringe of temperatures where thermonuclear reactions may take place, the rate of reactions varies exceedingly rapidly with temperature. See also Carbon-nitrogen-oxygen cycles; Kinetic theory of matter; Magnetohydrodynamics; Nuclear reaction; Pinch effect; Proton-proton chain.

A reaction between nuclei, usually fusion, which releases very large amounts of energy.

The noun has one meaning:

Meaning #1: a nuclear fusion reaction taking place at very high temperatures (as in the sun)