Fusion physics: hydrogen to helium
Fusion is the joining of light nuclei into a heavier nucleus, releasing energy. Like fission, the energy comes from the binding-energy curve — but from the light end, where lighter nuclei have less binding energy per nucleon than heavier ones (up to iron). The Sun's core fuses hydrogen to helium through the proton-proton chain.
The terrestrial reaction of greatest engineering interest is deuterium-tritium (D-T) fusion:
The products are an alpha particle (He-4, 3.5 MeV) and a fast neutron (14.1 MeV). The He-4 carries 20% of the energy and stays in the plasma (heating it); the neutron carries 80% and escapes the plasma, depositing its energy in surrounding structure as heat for power generation.
Why D-T rather than D-D or other reactions: D-T has the highest reaction cross-section at the lowest temperatures of any fusion reaction. D-D fusion is possible but requires higher temperatures (closer to 500 million K vs ~100 million K for D-T). At any temperature achievable in current systems, D-T is the easiest reaction.
The trade-off: D-T requires tritium, which does not occur naturally in usable quantities (tritium has a 12.3-year half-life). Tritium must be bred from lithium-6 in a blanket surrounding the plasma, using the 14.1 MeV neutron from the fusion reaction itself. The breeding loop is a critical part of any commercial D-T fusion design.
