International Workshop on Atomic Interactions in Laser Fields - Abstracts


The pressure broadening and shift of spectral lines produced in an intense monochromatic radiation field

G. Peach1 and F. Schuller2

1Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK
2Laboratoire des Interactions Moleculaires et des Hautes Pressions, C.N.R.S. 93430 Villetaneuse, France

 

The study of the response of an atom to an intense narrow-band radiation field has become important ever since the advent of laser sources. When atoms that are surrounded by a buffer gas are absorbing or emitting radiation, the spectral line profile is both broadened and shifted, and if the radiation field is intense, additional effects are expected to occur. A general theory has been developed [1], to describe the combined effects of collisional and radiative perturbations on absorption and fluorescence profiles, but this theory has not been applied in practice. In [2], a scalarly-additive unified
theory of pressure broadening has been developed for atom-perturber interactions of the form 1/Rp, which reproduces the well-known results of the impact and static approximations in the low-density/high-temperature and high-density/low-temperature limits, and also predicts the shapes of profiles in the crucial intermediate region. The theories given in [1] and [2] have been combined, and the results obtained for the case of Van der Waals interactions (p = 6) show that the effect of an intense radiation field is to produce significant extra broadening and shift of the profile. If the perturber density is decreased while the temperature is held constant, the width of the line decreases monotonically if there is no radiation field, but if there is a radiation field present, the line width at first decreases but eventually reaches a minimum and then starts to increase again. Illustrative profiles and simple criteria for assessing the relative importance of the strength of the radiation field will be presented.

References

  1. F. Schuller and G. Nienhuis, Physica 121C, 281-294 (1983).
  2. G. Peach, J. Phys. B: At. Mol. Phys. 17, 2599-2618 ( 1984).