Abstract
Aims. Energy levels, transition probabilities, and oscillator strengths are calculated for the second most abundant iron peak element
Ni II. The difficulty in obtaining an accurate target representation is related to the open d-shell nature of the target, which has a
minimum requirement of single and double promotions from the ground state configuration to the n = 4 shells. Therefore, in order to
achieve an accurate representation of the target ion, we have also included configurations containing the 4d, 5s, and 5p subshells. We
have undertaken a study of the electron impact excitation of Ni II and present here the collision strengths for forbidden and allowed
transitions among the lowest 800 fine-structure levels as well as the corresponding Maxwellian-averaged effective collision strengths
for a range of astrophysically relevant electron temperatures.
Methods. An accurate Ni II target structure was generated using the modified General-purpose Relativistic Atomic Structure Package
(GRASP0) for the lowest lying 1220 jj fine-structure levels, comprising the 11 configurations: 3p63d9
, 3p63d84s, 3p63d84p, 3p63d84d,
3p63d85s, 3p63d85p, 3p63d74s2
, 3p63d75s2
, 3p63d74s4p, 3p63d74s4d, and 3p43d94s4d. The relativistic parallel Dirac atomic R-matrix
codes (DARC) were utilised in the scattering calculations to generate the collision strengths for incident electron energies between 0 and
2 Ryd and, by employing infinite dipole and non-dipole limit points, we also generated the effective collision strengths for temperatures
in the range from 1000 to 400 000 K. Two separate calculations were performed, both comprised of truncated close-coupling expansions
of 800 jj-levels with the first calculation retaining the theoretical ab initio energy levels generated in the GRASP0 evaluations, whereas
in the second calculation these energies were shifted to their predicted National Institute of Standards and Technology (NIST) values
where possible. This should provide a lower estimate on the uncertainty.
Results. Comparisons are made between the radiative data and the collisional cross sections with past theoretical and experimental
studies. The effective collision strengths when compared with the most recent published calculations, are found to agree to within 10%
for the majority of the transitions considered. In addition, the data are used to model the spectrum of Ni II and good agreement is found
with previous investigations and observations.
Original language | English |
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Article number | A67 |
Number of pages | 14 |
Journal | Astronomy and Astrophysics |
Volume | 648 |
DOIs | |
Publication status | Published - 13 Apr 2021 |
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Dive into the research topics of 'Electron-impact excitation of Ni II'. Together they form a unique fingerprint.Student theses
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Dirac R-matrix scattering calculations in support of plasma diagnostics
Dunleavy, N. (Author), Ramsbottom, C. (Supervisor) & Ballance, C. (Supervisor), Dec 2021Student thesis: Doctoral Thesis › Doctor of Philosophy
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