Neutron Production

Neutron production in nuclear fusion occurs when light atomic nuclei, like those of hydrogen, collide and fuse together under extremely high temperatures and pressures, such as those found in stars. During this process, the energy released can sometimes cause the combined nucleus to emit neutrons. These neutrons can then participate in further reactions, contributing to the overall energy output. This mechanism is crucial for powering stars, including our Sun, and is a key area of research for developing sustainable fusion energy on Earth. Understanding neutron production helps scientists harness fusion as a clean energy source.