“One example of the close connection between particle physics and cosmology is an experiment that was performed in 1965 using the particle accelerator at Brookhaven National Laboratory on Long Island, New York. According to prevailing theories, a certain symmetry in the early universe created equal amounts of matter and its opposite, antimatter. We can see something like this at Fermilab when collisions produce equal numbers of protons and their opposite, antiprotons. But when matter and antimatter collide, they annihilate each other in bursts of radiation. So if the early universe produced equal amounts of matter and antimatter, then either all the matter and antimatter should have consumed each other, leaving a universe of nothing but radiation, or the matter and antimatter may have in some way separated. If so, where is the antimatter?
From careful searches for the radiation that results from matter-antimatter annihilations, scientists learned that the density of antimatter in the observable universe was very small. The Brookhaven experiment helped solve the puzzle of the missing antimatter by revealing a violation of a certain symmetry in the decay of neutral kaons (a type of meson, which in turn is a subatomic particle that is made up of quarks and antiquarks). As a result of this tiny violation of symmetry, a slight excess of matter survived annihilation by antimatter. This surviving matter now forms the galaxies, stars, and planets.”
(From Encarta, Leon M. Lederman’s article.)