Electron-impact excitation of Sc ii: collision strengths and effective collision strengths for fine-structure transitions
Article first published online: 23 JUL 2012
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 424, Issue 4, pages 2461–2467, 21 August 2012
How to Cite
Grieve, M. F. R. and Ramsbottom, C. A. (2012), Electron-impact excitation of Sc ii: collision strengths and effective collision strengths for fine-structure transitions. Monthly Notices of the Royal Astronomical Society, 424: 2461–2467. doi: 10.1111/j.1365-2966.2012.21021.x
- Issue published online: 8 AUG 2012
- Article first published online: 23 JUL 2012
- Manuscript Accepted: 30 MAR 2012
- Manuscript Received: 29 MAR 2012
- DEL studentship
- atomic data;
- atomic processes;
Accurate fine-structure atomic data for the Fe-peak elements are essential for interpreting astronomical spectra. There is a severe paucity of data available for Sc ii, highlighted by the fact that no collision strengths are readily available for this ion. We present electron-impact excitation collision strengths and Maxwellian averaged effective collision strengths for Sc ii. The collision strengths were calculated for all 3916 transitions amongst 89 jj levels (arising from the 3d4s, 3d2, 4s2, 3d4p, 4s4p, 3d5s, 3d4d, 3d5p, 4p2 and 3d4f configurations), resulting in a 944 coupled channel problem. The R-matrix package rmatrxii was utilized, along with the transformation code fine and the external region code pstgf, to calculate the collision strengths for a range of incident electron energies in the 0 to 8.3 Rydberg region. Maxwellian averaged effective collision strengths were then produced for 27 temperatures lying within the astrophysically significant range of 30 to 105 K.
The collision strengths and effective collision strengths were produced for two different target models. The purpose was to systematically examine the effect of including open 3p correlation terms into the configuration interaction expansion for the wavefunction. The first model consisted of all 36 CI terms that could be generated with the 3p core closed. The second model incorporated an additional six configurations which allowed for single-electron excitations from within the 3p core. Comparisons are made between the two models and the results of Bautista et al., obtained by private communication. It is concluded that the first model produced the most reliable set of collision and effective collision strengths for use in astrophysical and plasma applications.