Abstract
The form of the profile for spectral lines of radiation is found using the relativistic distribution function (DF) of fluxons on velocities and exact relativistic Doppler formula for frequencies. It is shown that the spectral line of radiation has finite width contrary to the results of classical theory in the limit of strong fluctuations.
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© 2001 Springer Science+Business Media Dordrecht
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Djumaev, M.R. (2001). The Doppler Effect and Form of the Profile of Radiation Spectral Lines. In: Abdullaev, F., Bang, O., Sørensen, M.P. (eds) Nonlinearity and Disorder: Theory and Applications. NATO Science Series, vol 45. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0542-5_34
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DOI: https://doi.org/10.1007/978-94-010-0542-5_34
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-0192-5
Online ISBN: 978-94-010-0542-5
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