Astrophysics (Index)About

Cherenkov radiation

(radiation from the shock of a charged particle passing through a medium)

Cherenkov radiation is electromagnetic radiation (EMR) emitted when a charged particle, e.g., electron, passes through a dielectric medium at a speed faster than the speed of light within that medium. The electromagnetic disturbance at the point where the particle travels moves faster than light and causes EMR in an expanding cone shape (Cherenkov cone), with an emphasis on shorter wavelengths. A well-known example is the blue glow in pictures of cooling water pools within nuclear-reactor facilities.

Spaceborne gamma rays can trigger showers of particles (such as electron-positron pairs) traveling at high speeds in the atmosphere, in turn, generating Cherenkov radiation in the air that can be detected by Earth-bound detectors, enabling them to indirectly detect the gamma rays (Cherenkov detectors).


(physics,EMR)
Further reading:
https://en.wikipedia.org/wiki/Cherenkov_radiation
https://en.wikipedia.org/wiki/Gamma-ray_astronomy
https://www.webexhibits.org/causesofcolor/4BA.html
https://www.iaea.org/newscenter/news/what-is-cherenkov-radiation
https://math.ucr.edu/home/baez/physics/Relativity/SpeedOfLight/cherenkov.html
http://large.stanford.edu/courses/2014/ph241/alaeian2/
https://ui.adsabs.harvard.edu/abs/1937PhRv...52..378C/abstract
https://www.douglas-scott-mcgregor.com/uploads/1/3/3/5/133545016/frank_and_tamm.pdf

Referenced by pages:
Cherenkov detector
Cherenkov Telescope Array (CTA)
GRAPES-3
High Energy Stereoscopic System (HESS)
High-altitude Water Cherenkov Observatory (HAWC)
IceCube
imaging atmospheric Cherenkov telescope (IACT)
KM3NeT (Cubic Kilometre Neutrino Telescope)
LHAASO
MAGIC
Milagro
Orbiting Wide-angle Light Collectors (OWL)
POEMMA
tau neutrino (ντ)
very-high-energy gamma rays (VHEGR)

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