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Vavilov-Cherenkov and Synchrotron Radiation: Foundations and Applications

The theory of the Vavilov-Cherenkov radiation observed by Cherenkov in 1934 was created by Tamm, Frank and Ginsburg who associated the observed blue light with the uniform charge motion of a charge at a velocity greater than the velocity of light in the medium. On the other hand, Vavilov, Cherenkov&...

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Autor principal: Afanasiev, G. N
Lenguaje:eng
Publicado: Springer 2005
Materias:
Acceso en línea:https://dx.doi.org/10.1007/1-4020-2411-8
http://cds.cern.ch/record/1338854
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author Afanasiev, G. N
author_facet Afanasiev, G. N
author_sort Afanasiev, G. N
collection CERN
description The theory of the Vavilov-Cherenkov radiation observed by Cherenkov in 1934 was created by Tamm, Frank and Ginsburg who associated the observed blue light with the uniform charge motion of a charge at a velocity greater than the velocity of light in the medium. On the other hand, Vavilov, Cherenkov's teacher, attributed the observed blue light to the deceleration of electrons. This has given rise to the appearance of papers in which the radiation of a charge uniformly moving in a finite space interval was related to the Bremsstrahlung arising at the end points of the motion interval. This monograph is intended for students of the third year and higher, for postgraduates, for professional scientists (both experimentalists and theoreticians) dealing with Vavilov-Cherenkov and synchrotron radiation. An acquaintance with the three volumes of the Landau and Lifshitz course (Quantum Mechanics, Classical Field Theory and Macroscopic Electrodynamics) is sufficient for understanding the text.
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spelling cern-13388542021-04-22T01:03:40Zdoi:10.1007/1-4020-2411-8http://cds.cern.ch/record/1338854engAfanasiev, G. NVavilov-Cherenkov and Synchrotron Radiation: Foundations and ApplicationsAstrophysics and AstronomyThe theory of the Vavilov-Cherenkov radiation observed by Cherenkov in 1934 was created by Tamm, Frank and Ginsburg who associated the observed blue light with the uniform charge motion of a charge at a velocity greater than the velocity of light in the medium. On the other hand, Vavilov, Cherenkov's teacher, attributed the observed blue light to the deceleration of electrons. This has given rise to the appearance of papers in which the radiation of a charge uniformly moving in a finite space interval was related to the Bremsstrahlung arising at the end points of the motion interval. This monograph is intended for students of the third year and higher, for postgraduates, for professional scientists (both experimentalists and theoreticians) dealing with Vavilov-Cherenkov and synchrotron radiation. An acquaintance with the three volumes of the Landau and Lifshitz course (Quantum Mechanics, Classical Field Theory and Macroscopic Electrodynamics) is sufficient for understanding the text.Springeroai:cds.cern.ch:13388542005
spellingShingle Astrophysics and Astronomy
Afanasiev, G. N
Vavilov-Cherenkov and Synchrotron Radiation: Foundations and Applications
title Vavilov-Cherenkov and Synchrotron Radiation: Foundations and Applications
title_full Vavilov-Cherenkov and Synchrotron Radiation: Foundations and Applications
title_fullStr Vavilov-Cherenkov and Synchrotron Radiation: Foundations and Applications
title_full_unstemmed Vavilov-Cherenkov and Synchrotron Radiation: Foundations and Applications
title_short Vavilov-Cherenkov and Synchrotron Radiation: Foundations and Applications
title_sort vavilov-cherenkov and synchrotron radiation: foundations and applications
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1007/1-4020-2411-8
http://cds.cern.ch/record/1338854
work_keys_str_mv AT afanasievgn vavilovcherenkovandsynchrotronradiationfoundationsandapplications