Oscillator strengths and transition probabilities for transitions among the fine-structure levels of the terms belonging to the 3s 2 3p 2 , 3s3p 3 , 3s 2 3p3d, 3s 2 3p4s, 3s 2 3p4p, and 3s 2 3p4d configurations of S III are calculated using extensive configuration-interaction wave functions. The rel
Oscillator Strengths for IR Rovibrational Transitions of CO
β Scribed by J.M. Hure; E. Roueff
- Publisher
- Elsevier Science
- Year
- 1993
- Tongue
- English
- Weight
- 597 KB
- Volume
- 160
- Category
- Article
- ISSN
- 0022-2852
No coin nor oath required. For personal study only.
β¦ Synopsis
We have solved the nuclear SchrΓΆdinger radial equation to derive wavefunctions and rovibrational energy levels of the carbon monoxide molecule ({ }^{12} \mathrm{C}^{16} \mathrm{O}) in its ground electronic state (X^{\prime} \Sigma^{+}) at a spectroscopic accuracy. We then calculated the dipole matrix elements for transitions involving vibrational quantum numbers up to (v=15) and rotational quantum numbers up to (J=200). Calculations were carried out for the fundamental ((\Delta v=1)) and the three first overtone ((\Delta v=) (2,3,4) ) bands. For the transition matrix elements there is typically a (10 %) difference from previous results due to recent values of the dipole moment function. This gives a significant (20 %) difference for the absorption oscillator strengths which are computed for this set of 21600 lines. C 1993 Academic Press, Inc.
π SIMILAR VOLUMES
An extensive dataset of oscillator strengths, line strengths, and Einstein A-coefficients has been calculated for a large number of dipole-allowed (DS Γ 0) fine-structure transitions in Si II. The line strengths in LS coupling are obtained in an ab initio manner in the close-coupling approximation e