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.