Electron impact excitation of Be-like ions: a comparison of DARC and ICFT results

Abstract

Emission lines of Be-like ions are frequently observed in astrophysical plasmas, and many are useful for density and temperature diagnostics. However, accurate atomic data for energy levels, radiative rates (A-values) and effective electron excitation collision strengths (${\rm Y}$) are required for reliable plasma modelling. In general it is reasonably straightforward to calculate energy levels and A- values to a high level of accuracy. By contrast, considerable effort is required to calculate ${\rm Y}$, and hence it is not always possible to assess the accuracy of available data. Recently, two independent calculations (adopting the $R$-matrix method) but with different approaches (DARC and ICFT) have appeared for a range of Be-like ions. Therefore, in this work we compare the two sets of ${\rm Y}$, highlight the large discrepancies for a significant number of transitions and suggest possible reasons for these.

9 pages including 2 figures, will appear in 2015 MNRAS

References in corpus (2)

• Energy levels, radiative rates and electron impact excitation rates for transitions in Fe XIV
• Energy levels, radiative rates and electron impact excitation rates for transitions in Be-like Cl XIV, K XVI and Ge XXIX

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• Discrepancies in Atomic Data and Suggestions for their Resolutions