The shape of the inner-wing satellites of self-broadened first resonance lines of caesium and rubidium
- 28 September 1980
- journal article
- Published by IOP Publishing in Journal of Physics B: Atomic and Molecular Physics
- Vol. 13 (18) , 3605-3611
- https://doi.org/10.1088/0022-3700/13/18/012
Abstract
Theoretical satellite profiles have been calculated by means of the modified quasi-static approximation. Comparison with the experimental results shows that the shape of the theoretical satellite band depends on precise knowledge of the interatomic potential curves. A simple quadratic approximation of the 0g-(2P32/+2P32/+2S12/) potential curve near the extremum was also tested in the case of the caesium 8565 AA satellite band.Keywords
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