There have been discussions in the recent literature regarding the accuracy of the available electron impact excitation rates (equivalently effective collision strengths γ) for transitions in Be-like ions. In the present paper we demonstrate, once again, that earlier results for γ are indeed overestimated (by up to four orders of magnitude), for over 40 per cent of transitions and over a wide range of temperatures. To do this we have performed two sets of calculations for NIV, with two different model sizes consisting of 166 and 238 fine-structure energy levels. As in our previous work, for the determination of atomic structure the GRASP (General-purpose Relativistic Atomic Structure Package) is adopted and for the scattering calculations (the standard and parallelised versions of) the Dirac Atomic R-matrix Code (DARC) are employed. Calculations for collision strengths and effective collision strengths have been performed over a wide range of energy (up to 45 Ryd) and temperature (up to 2.0 × 106 K), useful for applications in a variety of plasmas. Corresponding results for energy levels, lifetimes and A-values for all E1, E2, M1 and M2 transitions among 238 levels of NIV are also reported.
CITATION STYLE
Aggarwal, K. M., Keenan, F. P., & Lawson, K. D. (2016). Electron impact excitation of NIV: Calculations with the DARC code and a comparison with ICFT results. Monthly Notices of the Royal Astronomical Society, 461(4), 3997–4012. https://doi.org/10.1093/mnras/stw1369
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