Content, Cosmology

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11.3 Antimatter and antiparticles:
In particle physics and quantum chemistry, antimatter is composed of antiparticles in the same way that normal matter is composed of particles. For example an antielectron (a positron, an electron with a positive charge) and an antiproton (a proton with a negative charge) could form an antihydrogen atom in the same way that an electron and a proton form a normal matter hydrogen atom. Mixing of matter and antimatter would lead to the annihilation of both as mixing of antiparticles and particles does, thus giving rise to high-energy photons (gamma rays) or other particle-antiparticle pairs. The particles resulting from matter-antimatter annihilation are endowed with energy equal to the difference between the rest mass of the products of the annihilation and the rest mass of the original matter-antimatter pair, which is often quite large. Antimatter is not found naturally on Earth, except very briefly and in vanishingly small quantities (as the result of radioactive decay or cosmic rays). This is because antimatter which came to exist on Earth outside the confines of a suitable physics laboratory would almost instantly meet the ordinary matter that Earth is made of, and be annihilated. Antiparticles and some stable antimatter (such as antihydrogen) can be made in tiny amounts, but not in enough quantity to do more than test a few of its theoretical properties.

- Antineutrinos: Antiparticles of neutrinos are neutral particles produced in nuclear beta decay where a neutron turns into a proton. They have a spin of 1/2, and they are part of the lepton family of particles. The antineutrinos observed so far all have right-handed helicity, while the neutrinos are left-handed. Antineutrinos interact with other matter only through the gravitational and weak forces, making them very difficult to detect experimentally. Antineutrinos have very small mass.

- Electron-positron annihilation: This occurs when an electron and a positron (the electron's anti-particle) collide. The result of the collision is the creation of gamma ray photons or, less often, other particles. The process must satisfy a number of conservation laws, including:
- Conservation of charge. The net charge before and after is zero.
- Conservation of linear momentum and total energy. This forbids the creation of a single gamma ray.
- Conservation of angular momentum.

As with any two charged objects, electrons and positrons may also interact with each other without annihilating, in general by elastic scattering.