Abstract
By using the classical Fourier integral theory, an expression is given for the shape of a spectral line, broadened by phase changes due to collisions and by the actual changes in velocity of the emitting particles resulting from collisions. The result is not a simple Voigt-type folding of an exponential into a dispersion distribution; it exhibits the contraction noted by Dicke and leads to the usual formulas when the time interval between path-deflecting or phase-disturbing collisions becomes very great.
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Publication Info
- Year
- 1961
- Type
- article
- Volume
- 122
- Issue
- 4
- Pages
- 1218-1223
- Citations
- 727
- Access
- Closed
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Identifiers
- DOI
- 10.1103/physrev.122.1218