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English: Cherenkov radiation, also known as Vavilov-Cherenkov radiation, (also spelled Čerenkov) is electromagnetic radiation emitted when a charged particle (such as an electron) passes through a dielectric medium at a speed greater than the phase velocity of light in that medium. The charged particles polarize the molecules of that medium, which then turn back rapidly to their ground state, emitting radiation in the process. The characteristic blue glow of nuclear reactors is due to Cherenkov radiation. It is named after Russian scientist Pavel Alekseyevich Cherenkov, the 1958 Nobel Prize winner who was the first to detect it experimentally. A theory of this effect was later developed within the framework of Einstein's special relativity theory by Igor Tamm and Ilya Frank, who also shared the Nobel Prize. Cherenkov radiation has been theoretically predicted by the English polymath Oliver Heaviside in papers published in 1888–1889.
This category has only the following subcategory.
- ► Air Cherenkov Telescopes (1 C, 1 F)
Media in category "Cherenkov radiation"
The following 27 files are in this category, out of 27 total.
- 2011 Advanced Science...
- Advanced Test Reactor.jpg
- Cerenkov Effect.jpg
- Cherenkov radiation-an...