The Cherenkov effect occurs when a particle carrying an electric charge travels through a transparent medium like water or air. If the particle travels faster than light in this medium, its passage causes a brief flash of light, a Cherenkov light.
The effect is named after the Soviet physicist Pavel Alekseyevich Cherenkov (1904-1990) who discovered the phenomenon and obtained the Nobel Prize in Physics for his discovery in 1958.
In the field of radioactivity, the particles concerned by the Cherenkov effect are electrons and positrons. Very light, they reach very high speeds. In water, the speed of light is 200,000 km / sec. An electron must have an energy greater than 175 keV to go faster than light in water. This condition is often fulfilled by beta electrons of radioactivity, but never with the heavy and too slow alpha particles.
During their journey, the corpuscles ionize and rattle the many atoms and molecules they encounter. The restoration of the medium is accompanied by the emission of de-excitation photons, for instance in water of visible photons of blue light. The emission of these photons does not cost much in energy: 2.5 electronvolts (eV) for a photon in the blue!
A 500 keV (500,000 eV ) electron that would spend all its energy in emitting blue photons would produce 200,000 of them! The path of the beta electrons in water is of the order of a few millimeters. On this very short course, the emitted photons are therefore very numerous. Photons are also elementary waves. These blue waves combine along the trajectory to form spherical light waves. If the electron goes faster than light in water, these spherical waves combine in turn into a conical wave front that accompanies the particle.
An electron that exceeds the speed of light resembles a fighter plane that crosses the sound barrier. As long as the plane has not exceeded the speed of sound, the sound waves announce its arrival. When it reaches a supersonic speed, the plane passes over our heads before the sound wavefront shakes the windows and vibrates our eardrums. The Cherenkov effect derives from an analogous principle: the electron plays the role of the airplane, the waves of light that of the sound waves.
In the atmosphere, the speed of light is very close to 300,000 km / sec, the speed of light in a vacuum. An electron must have an energy greater than 21 MeV (21 million electronvolts!) to generate a flash of Cherenkov light. This condition is never fulfilled for the electrons of radioactivity.
Cosmic radiation, on the other hand, contains electrons, positrons and also very high energy muons that can produce Cherenkov light flashes. This Cherenkov light is used to detect cosmic showers.
The Cherenkov effect is used as a tool in many modern experiments: in nuclear physics (for instance to detect solar neutrinos); in high energy experiments such as the ones performed at CERN to identify the nature of particles; in the astrophysical experiments that study cosmic showers.
Access to page in french