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Nuclear fusion

In physics, nuclear fusion is the process by which two nuclei join together to form a heavier nucleus. It is accompanied by the release or absorption of energy depending on the masses of the nuclei involved. Iron and nickel nuclei have the largest binding energies of all nuclei and therefore are the most stable. The fusion of two nuclei to produce a nucleus lighter than iron or nickel generally gives off energy while the fusion of nuclei heavier than them absorbs energy.

The deuterium-tritium (D-T) fusion reaction is considered the most promising for producing fusion power.

The deuterium-tritium (D-T) fusion reaction is considered the most promising for producing fusion power.
 

All text is available under the terms of the GNU Free Documentation License (see Copyrights for details).

 

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