Antimatter
Overview
Antimatter is the mirror version of normal matter. Antiparticles have some properties identical to their counterparts, such as mass, but opposite values for others, such as charge. All known particles have antimatter counterparts or are their own antiparticles, and some can combine to form composite antimatter particles, such as the antiproton. When a particle collides with its antiparticle, they annihilate, converting their mass into energy or less massive particles.
The concept of antimatter emerged in 1928, when special relativity, which explained the motion of objects traveling near the speed of light, was combined with quantum mechanics. The mathematics suggested the existence of an electron with negative energy, dubbed the antielectron. This particle—a positively charged electron, or positron—was discovered four years later while analyzing collisions between cosmic rays and atmospheric atoms.
Besides cosmic ray interactions, antimatter is commonly produced in high-energy environments, including stars, nuclear power plants, thunderstorms, and particle accelerators. Some radioactive substances emit antimatter, which is harnessed in imaging systems like PET scans. Through pair production, matter-antimatter particle pairs are created from pure energy, but it is unclear why the energy available in the early universe did not produce equal amounts of matter and antimatter across the cosmos.
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