Fusion Reaction Dynamics

Fusion reaction dynamics involve combining light atomic nuclei, like hydrogen isotopes, at extremely high temperatures and pressures so they fuse into a heavier nucleus, releasing a large amount of energy. When nuclei are heated to millions of degrees, they move fast enough to overcome their natural repulsion due to positive charges (protons). Once fused, the resulting nucleus and energy are produced, similar to processes powering the sun. Controlling these reactions on Earth requires precise conditions to sustain the fusion process efficiently, making it a promising, clean energy source if mastered.