Large-scale multiconfiguration Dirac-Hartree-Fock calculations for astrophysics: n=4 levels in P-like ions from Mn~XI to Ni~XIV

Abstract

Using the multiconfiguration Dirac-Hartree-Fock and the relativistic configuration interaction methods, a consistent set of transition energies and radiative transition data for the lowest 546 (623, 701, 745) states of the $3p^{4}3d$, $3s3p^{2}3d^2$, $3s3p^{3}4p$, $3s3p^4$, $3s^{2}3d^3$, $3s^{2}3p^{2}3d$, $3s^{2}3p^{2}4d$, $3s^{2}3p^{2}4s$, $3p^{3}3d^2$, $3p^5$, $3s3p3d^3$, $3s3p^{3}3d$, $3s3p^{3}4s$, $3s^{2}3p3d^2$, %$3s^{2}3p^{2}4f$, $3s^{2}3p^{2}4p$, $3s^{2}3p^3$ configurations in Mn~XI (Fe~XII, Co~XIII, Ni~XIV) is provided. The comparison between calculated excitation energies for the $n=4$ states and available experimental values for Fe XII indicate that the calculations are highly accurate, with uncertainties of only a few hundred cm${}^{-1}$. Lines from these states are prominent in the soft X-rays. With the present calculations, several recent new identifications are confirmed. Other identifications involving $3p^{2}4d$ levels in Fe~XII that were found questionable are discussed and a few new assignments are recommended. As some $n=4$ states of the other ions also show large discrepancies between experimental and calculated energies, we reassess their identification. The present study provides highly accurate atomic data for the $n=4$ states of P-like ions of astrophysical interest, for which experimental data are scarce.

References in corpus (13)

• Solar UV and X-Ray Spectral Diagnostics
• CHIANTI - an atomic database for emission lines - Paper XV: Version 9, improvements for the X-ray satellite lines
• High precision density measurements in the solar corona: I. Analysis methods and results for Fe XII and Fe XIII
• Spectroscopic LSJ notation for atomic levels obtained from relativistic calculations
• Calculations with spectroscopic accuracy: energies and transition rates in the nitrogen isoelectronic sequence from Ar XII to Zn XXIV
• Benchmarking atomic data for astrophysics: a first look at the soft X-ray lines
• Extended relativistic configuration interaction and many-body perturbation calculations of spectroscopic data for the $n\le 6$ configurationsin ne-like ions between Cr XV and Kr XXVII
• Extended Calculations of Spectroscopic Data: Energy Levels, Lifetimes and Transition rates for O-like ions from Cr XVII to Zn XXIII
• Multi-configuration Dirac-Hartree-Fock calculations of forbidden transitions within the 3d^k ground configurations of highly charged ions (Z=72-83)
• Large-scale multiconfiguration Dirac-Hartree-Fock calculations for astrophysics: Cl-like ions from Cr~VIII to Zn~XIV
• Energy Levels, Lifetimes and Transition rates for P-like ions from Cr X to Zn XVI from large-scale Relativistic Multiconfiguration Calculations
• Benchmarking Atomic Data for Astrophysics: Be-like Ions between B II and Ne VII
• Extended calculations of energy levels, radiative properties, and lifetimes for oxygen-like Mo XXXV

Cited by in corpus (2)

• CHIANTI -- an atomic database for emission lines -- Paper XVI: Version 10, further extensions
• Extended Calculations with Spectroscopic Accuracy: Energy Levels and Radiative Rates for O-like Ions between Ar XI and Cr XVII