MCDHF and RCI calculations of energy levels, lifetimes, and transition rates in Si III and Si IV

@article{Atalay2019MCDHFAR,
  title={MCDHF and RCI calculations of energy levels, lifetimes, and transition rates in Si III and Si IV},
  author={B. Atalay and Tomas Brage and Per J{\"o}nsson and Henrik Hartman},
  journal={Astronomy \& Astrophysics},
  year={2019}
}
We present extensive multiconfiguration Dirac-Hartree-Fock and relativistic configuration interaction calculations including 106 states in doubly ionized silicon (Si III) and 45 states in triply ionized silicon (Si IV), which are important for astrophysical determination of plasma properties in different objects. These calculations represents an important extension and improvement of earlier calculations especially for Si III. The calculations are in good agreement with available experiments… 
2 Citations

Figures and Tables from this paper

Multiconfiguration Dirac-Hartree-Fock calculations of Landég-factors for ions of astrophysical interest: B II, C I−IV, Al I−II, Si I−IV, P II, S II, Cl III, Ar IV, Ca I, Ti II, Zr III, and Sn II

Aims.The Landég-factor is an important parameter in astrophysical spectropolarimetry, used to characterize the response of a line to a given value of the magnetic field. The purpose of this paper is

References

SHOWING 1-10 OF 78 REFERENCES

Radiative-lifetime measurements in Si 11-Si v

Radiative lifetimes have been measured for transitions in Si II to Si v in the vacuum ultraviolet region using the beam-foil technique. Lifetime results for Si IIHV transitions resolve existing

Excitation energies and transition rates in magnesiumlike ions

Excitation energies, transition probabilities, and lifetimes are calculated for 3 l 13l 2-3l 33l 4 electric dipole transitions in Mg-like ions with nuclear charges Z ranging from 13 to 100.

Atomic Data and Nuclear Data Tables

a b s t r a c t The ab initio quasirelativistic Hartree–Fock method developed specifically for the calculation of spectral parameters of heavy atoms and highly charged ions is used to derive

Relativistic calculations of radiative properties and fine structure constant varying sensitivity coefficients in the astrophysically relevant Zn ii, Si iv and Ti iv ions

We have carried out calculations of the relativistic sensitivity coefficients, oscillator strengths, transition probabilities, lifetimes and magnetic dipole hyperfine structure constants for a number

Plunging configurations and J-dependent lifetimes in Mg-like ions

The results of configuration interaction calculations for Mg-like P IV, S V and Cl VI, concerning energy levels, oscillator strengths and lifetimes, are presented with emphasis on the isoelectronic

CIV3 and relativistic quantum defect orbital (RQDO) oscillator strengths in Mg-like ions of astrophysical interest

Astrophysically relevant transitions in the Mg-like ions Si III, S V and Fe XV have been studied. A J-dependent CIV3 calculation, more extensive than other, earlier ones, has led to improved accuracy

Si III line ratios in the sun

New atomic data for Si III have been used to predict level populations and emission-line intensity ratios for electron densities and temperatures appropriate to the solar transition region. The

Evidence for Non-Maxwellian Electron Energy Distributions in the Solar Transition Region: Si III Line Ratios from SUMER

Recent calculations of Si III emission-line strengths are compared with SUMER observations from a quiet solar region, a coronal hole, and an active region. Diagnostic line ratios are used to derive

Oscillator strengths for transitions to high-lying excited states of carbon

A spline frozen-cores method for treating Rydberg series is presented and applied to series in carbon. The method can be used for accurate calculations of oscillator strengths for states with high
...