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	<updated>2026-04-08T12:32:25Z</updated>
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		<updated>2025-03-17T06:47:23Z</updated>

		<summary type="html">&lt;p&gt;CSV import&lt;/p&gt;
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		<updated>2025-02-10T10:06:18Z</updated>

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		<author><name>Prab</name></author>
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		<updated>2024-03-19T09:56:27Z</updated>

		<summary type="html">&lt;p&gt;CSV import&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;&amp;#039;&amp;#039;&amp;#039;Cherenkov radiation&amp;#039;&amp;#039;&amp;#039; (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 phenomenon is named after the Soviet physicist Pavel Alekseyevich Cherenkov, who was the first to rigorously characterize it and attribute its origin correctly, work for which he received the Nobel Prize in Physics in 1958.&lt;br /&gt;
&lt;br /&gt;
==Overview==&lt;br /&gt;
Cherenkov radiation is a consequence of the electromagnetic field produced by a charged particle moving through a medium with a speed greater than the speed of light in that medium. The radiation is emitted in a cone in the direction of the particle&amp;#039;s motion and is characterized by a continuous spectrum of light that ranges from the near ultraviolet to the visible spectrum, giving it a distinct blue glow. This effect is commonly observed in nuclear reactors and in medical imaging devices.&lt;br /&gt;
&lt;br /&gt;
==Physical Principles==&lt;br /&gt;
The condition for the emission of Cherenkov radiation is given by the Cherenkov angle, which is derived from the conservation of energy and momentum. The angle of emission θ_C is given by the formula:&lt;br /&gt;
&lt;br /&gt;
\[ \cos(\theta_C) = \frac{c}{v \cdot n} \]&lt;br /&gt;
&lt;br /&gt;
where &amp;#039;&amp;#039;c&amp;#039;&amp;#039; is the speed of light in vacuum, &amp;#039;&amp;#039;v&amp;#039;&amp;#039; is the velocity of the charged particle, and &amp;#039;&amp;#039;n&amp;#039;&amp;#039; is the refractive index of the medium. The intensity and spectral distribution of Cherenkov radiation depend on the velocity of the particle, the charge of the particle, and the optical properties of the medium.&lt;br /&gt;
&lt;br /&gt;
==Applications==&lt;br /&gt;
Cherenkov radiation has several important applications in various fields:&lt;br /&gt;
&lt;br /&gt;
* In [[nuclear physics]], it is used for the detection of high-speed particles.&lt;br /&gt;
* In [[medical physics]], Cherenkov radiation is utilized in certain types of radiation therapy and diagnostic techniques.&lt;br /&gt;
* In [[astrophysics]], it aids in the detection of cosmic rays through Cherenkov telescopes.&lt;br /&gt;
* It also finds applications in particle physics experiments, where Cherenkov detectors are used to identify particles.&lt;br /&gt;
&lt;br /&gt;
==Detection and Measurement==&lt;br /&gt;
Cherenkov detectors, including water Cherenkov detectors and gas Cherenkov detectors, are designed to measure the presence and properties of Cherenkov radiation. These detectors play a crucial role in experimental physics by allowing the identification and characterization of high-speed charged particles.&lt;br /&gt;
&lt;br /&gt;
==Historical Background==&lt;br /&gt;
Pavel Cherenkov, along with his colleagues Igor Tamm and Ilya Frank, developed the theoretical explanation for the radiation he observed, linking it to the motion of charged particles at speeds greater than the speed of light in a medium. This work laid the foundation for the field of Cherenkov radiation and its applications in various scientific disciplines.&lt;br /&gt;
&lt;br /&gt;
==See Also==&lt;br /&gt;
* [[Electromagnetic radiation]]&lt;br /&gt;
* [[Speed of light]]&lt;br /&gt;
* [[Nuclear reactor]]&lt;br /&gt;
* [[Particle physics]]&lt;br /&gt;
&lt;br /&gt;
[[Category:Physics]]&lt;br /&gt;
[[Category:Electromagnetic radiation]]&lt;br /&gt;
[[Category:Nuclear physics]]&lt;br /&gt;
{{Physics-stub}}&lt;/div&gt;</summary>
		<author><name>Prab</name></author>
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