4.7 Article

ELECTRON-IMPACT EXCITATION OF Ni II: EFFECTIVE COLLISION STRENGTHS FOR OPTICALLY ALLOWED FINE-STRUCTURE TRANSITIONS

Journal

ASTROPHYSICAL JOURNAL
Volume 738, Issue 1, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/738/1/5

Keywords

atomic data; atomic processes; methods: numerical; plasmas; scattering

Funding

  1. STFC
  2. DEL Studentship
  3. Science and Technology Facilities Council [ST/H001778/1, PP/D00103X/1] Funding Source: researchfish
  4. Division Of Astronomical Sciences
  5. Direct For Mathematical & Physical Scien [0802292] Funding Source: National Science Foundation
  6. Division Of Astronomical Sciences
  7. Direct For Mathematical & Physical Scien [0808398] Funding Source: National Science Foundation
  8. STFC [PP/D00103X/1, ST/H001778/1] Funding Source: UKRI

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In this paper, we present collision strengths and Maxwellian averaged effective collision strengths for the electron-impact excitation of Ni II. Attention is expressly concentrated on the optically allowed fine-structure transitions between the 3d(9), 3d(8)4s, and 3d(7)4s(2) even parity levels and the 3d(8)4p and 3d(7)4s 4p odd parity levels. The parallel RMATRXII R-matrix package has been recently extended to allow for the inclusion of relativistic fine-structure effects. This suite of codes has been utilized in conjunction with the parallel PSTGF and PSTGICF programs in order to compute converged total collision strengths for the allowed transitions with which this study is concerned. All 113 LS terms identified with the 3d(9), 3d(8)4s, 3d(7)4s(2), 3d(8)4p, and 3d(7)4s 4p basis configurations were included in the target wavefunction representation, giving rise to a sophisticated 295 jj-level, 1930 coupled channel scattering complex. Maxwellian averaged effective collision strengths have been computed at 30 individual electron temperatures ranging from 30 to 1,000,000 K. This range comfortably encompasses all temperatures significant to astrophysical and plasma applications. The convergence of the collision strengths is exhaustively investigated and comparisons are made with previous theoretical works, where significant discrepancies exist for the majority of transitions. We conclude that intrinsic in achieving converged collision strengths and thus effective collision strengths for the allowed transitions is the combined inclusion of contributions from the (N + 1) partial waves extending to a total angular momentum value of L = 50 and further contributions from even higher partial waves accomplished by employing a top-up procedure.

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