Energy levels, radiative rates and electron impact excitation rates for transitions in C iii
Energy levels, radiative rates and electron impact excitation rates for transitions in C iii
复制标题
C iii 跃迁的能级、辐射速率和电子碰撞激发速率
DOI:
10.1093/mnras/stv684
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发表时间:
2015
影响因子:
4.8
通讯作者:
Aggarwal K
中科院分区:
文献类型:
--
作者:
Aggarwal K
We report energy levels, radiative rates (A-values) and lifetimes for the astrophysically important Be-like ion Ciii. For the calculations, 166 levels belonging to then≤ 5 configurations are considered and thegrasp(General-purpose Relativistic Atomic Structure Package) is adopted. EinsteinA-coefficients are provided for all E1, E2, M1 and M2 transitions, while lifetimes are compared with available measurements as well as theoretical results, and no large discrepancies noted. Our energy levels are assessed to be accurate to better than 1 per cent for a majority of levels, andA-values to better than 20 per cent for most transitions. Collision strengths are also calculated, for which the Dirac AtomicR-matrix Code (darc) is used. A wide energy range, up to 21 Ryd, is considered and resonances resolved in a fine energy mesh in the thresholds region. The collision strengths are subsequently averaged over a Maxwellian velocity distribution to determine effective collision strengths up to a temperature of 8.0 × 105K, sufficient for most astrophysical applications. Our data are compared with the recentR-matrix calculations of Fernández-Menchero et al., and significant differences (up to over an order of magnitude) are noted for several transitions over the complete temperature range of the results.