Cherenkov radiation


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Cherenkov radiation

also Čerenkov radiation
n.
Light emitted in the Čerenkov effect.

[After Pavel Alekseevich Cherenkov (1904-1990), Russian physicist.]
American Heritage® Dictionary of the English Language, Fifth Edition. Copyright © 2016 by Houghton Mifflin Harcourt Publishing Company. Published by Houghton Mifflin Harcourt Publishing Company. All rights reserved.

Cherenkov radiation

(tʃɪˈrɛŋkɒf)
n
(General Physics) the electromagnetic radiation produced when a charged particle moves through a medium at a greater velocity than the velocity of light in that medium
[C20: named after Pavel Alekseyevich Cherenkov (1904–90), Soviet physicist]
Collins English Dictionary – Complete and Unabridged, 12th Edition 2014 © HarperCollins Publishers 1991, 1994, 1998, 2000, 2003, 2006, 2007, 2009, 2011, 2014
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When these gamma rays reach the Earth's atmosphere they are absorbed, producing a short-lived shower of secondary particles that emit weak flashes of bluish light known as Cherenkov radiation, lasting just a few billionths of a second.
This, in turn, creates an optic shock wave called Cherenkov radiation, which resembles something like a cone of light.
Detecting this so-called Cherenkov radiation from muons is particularly revealing: from the data, scientists deduce the travel direction and the energy of the muon and, thus, of the original neutrino.
The features seen can be described in terms of soliton fission and dispersive wave emission in time domain while in terms of self-phase modulation and Cherenkov radiation in spectral domain, respectively.
Metamaterial exhibits some novel electromagnetic and optical properties which are not found in nature media, for example, negative refraction, reversals of both Doppler shift and Cherenkov radiation [2], enhancement of evanescent wave, and subwavelength imaging [6].
Negative refractive index (NRI) metamaterials with simultaneously negative permittivity and negative permeability are currently the focus of a great deal of interest due to their unique electromagnetic properties such as the reversals of both Doppler shift and Cherenkov radiation, enhancement of evanescent wave, and subwavelength resolution imaging, etc.
It was expanded in 2009 to span 1 square kilometer, becoming the world's biggest Cherenkov radiation detector.
Muons from high-energy neutrinos (energy range between [10.sup.11] and [10.sup.16] eV) radiate blue light, which is the so-called Cherenkov radiation. In transparent ice or clear water this light can be detected by optical sensors like photomultiplier tubes.
Those PMTs can sense the blue Cherenkov radiation that is generated during the rare event of a high-energy neutrino entering the planet from the Northern Hemisphere, passing completely through it, then colliding with a water molecule in the ice sheet in the vicinity of the detector.
Cherenkov radiation occurs when electrons move in a medium with a speed greater than the phase speed of electromagnetic waves in the medium.