Fusion: producing clean, emission-free, virtually unlimited energy for the world
Fusion is a nuclear process where two light nuclei are brought within such proximity of one another that the strong force binds them together, fusing them into a heavier element. For fusion applications on earth, the hydrogen isotopes deuterium (one proton and one neutron) and tritium (one proton and two neutrons) will undergo fusion reactions producing a helium atom and a neutron. The products carry a tremendous amount of kinetic energy based on Einstein’s famous mass-equivalence formula E=mc². The stable helium nucleus carries 20% of the energy and is used to sustain the fusion reaction, and the neutron carries the remainder of the energy isotropically to the walls. The neutrons heat the walls which in turn are cooled by water, generating steam that drives a turbine which, in turn, produces electricity.