The synchrotron radiation from the Volkov solution of the Dirac equation

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dc.creatorPardy, Miroslav
dc.date2007-03-09
dc.date.accessioned2026-07-07T07:51:05Z
dc.date.available2026-07-07T07:51:05Z
dc.descriptionThe aim of this article is to show it is possible to get the power spectrum of the synchrotron radiation from the Volkov solution of the Dirac equation and the S-matrix. We also generalize the Bargmann-Michel-Telegdi equation for the spin motion in case it involves the radiative term. This equation can play crucial role for the spin motion of protons in LHC. The axion production in the magnetic field described by the Volkov solution is discussed.
dc.description14 pages
dc.identifierhttps://arxiv.org/abs/hep-ph/0703102
dc.identifierhttp://arxiv.org/abs/hep-ph/0703102
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/125388
dc.subjectHigh Energy Physics - Phenomenology
dc.titleThe synchrotron radiation from the Volkov solution of the Dirac equation
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