The Askaryan effect is the phenomenon whereby a particle traveling faster than the phase velocity of light in a dense dielectric (such as salt, ice or the lunar regolith) produces a shower of secondary charged particles which contain a charge anisotropy and thus emits a cone of coherent radiation in the radio or microwave part of the electromagnetic spectrum. It is similar to the Cherenkov effect. It is named after Gurgen Askaryan, a Soviet-Armenian physicist who postulated it in 1962.
The effect was first observed experimentally in 2000, 38 years after its theoretical prediction. So far the effect has been observed in silica sand, rock salt, ice, and Earth's atmosphere.
The effect is of primary interest in using bulk matter to detect ultra-high energy neutrinos. The Antarctic Impulse Transient Antenna (ANITA) experiment uses antennas attached to a balloon flying over Antarctica to detect the Askaryan radiation produced as cosmic neutrinos travel through the ice. Several experiments have also used the Moon as a neutrino detector based on detection of the Askaryan radiation.
- Observation of the Askaryan Effect in Silica Sand
- Observation of the Askaryan Effect in Rock Salt
- Observation of the Askaryan Effect in Ice
- A large light-mass component of cosmic rays at 1017–1017.5 electronvolts from radio observations
- ANITA Project Overview
- ARIANNA collaboration
- GLUE project
- NuMoon project
- LUNASKA project
- RESUN project[permanent dead link]