Fusion21

What is nuclear fusion?



The goal of fusion research is to derive energy from fusion of atomic nuclei. Nuclear fusion is an important natural process: Many chemical elements originate from hydrogen through fusion; fusion is the energy source of the sun and stars. Under terrestrial conditions it is the two hydrogen isotopes, deuterium and tritium, that fuse most readily. In the process a helium nucleus is produced, this being accompanied by release of a neutron and large quantities of useful energy: One gram of fuel could generate 90,000 kilowatt-hours of energy in a power plant – the combustion heat of 11 tonnes of coal.

Fusion fuels are cheap and uniformly distributed on earth. Seawater contains deuterium in almost inexhaustible quantities. Tritium, a radioactive gas with a short half-life of 12.3 years, hardly occurs in nature. It can, however, be formed in a power plant from lithium, which is likewise abundantly available. Since, moreover, a fusion power plant will have ecologically favourable properties, fusion could make an enduring contribution to future energy supply.





Fusion reaction of deuterium and tritium