Next Article in Journal / Special Issue
Hyperfine Structure and Isotope Shifts in Dy II
Previous Article in Journal
An Investigation on the He(1s2s2 2S) Resonance in Debye Plasmas
Previous Article in Special Issue
Spectrum and Energy Levels of Four-Times Ionized Yttrium (Y V)
 
 
Font Type:
Arial Georgia Verdana
Font Size:
Aa Aa Aa
Line Spacing:
Column Width:
Background:
Article

Combining Multiconfiguration and Perturbation Methods: Perturbative Estimates of Core–Core Electron Correlation Contributions to Excitation Energies in Mg-Like Iron

1
Materials Science and Applied Mathematics, Malmö University, SE-205 06 Malmö, Sweden
2
Department of Computer Science, University of British Columbia, Vancouver, BC V6T 1Z4, Canada
3
Mathematical Institute, University of Oxford, Woodstock Road, Oxford OX2 6GG, UK
4
Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, Wilberforce Road, Cambridge CB3 0WA, UK
*
Author to whom correspondence should be addressed.
Submission received: 25 November 2016 / Revised: 22 December 2016 / Accepted: 6 January 2017 / Published: 12 January 2017
(This article belongs to the Special Issue Spectra of Ionized Atoms: From Laboratory to Space)

Abstract

:
Large configuration interaction (CI) calculations can be performed if part of the interaction is treated perturbatively. To evaluate the combined CI and perturbative method, we compute excitation energies for the 3 l 3 l , 3 l 4 l and 3 s 5 l states in Mg-like iron. Starting from a CI calculation including valence and core–valence correlation effects, it is found that the perturbative inclusion of core–core electron correlation halves the mean relative differences between calculated and observed excitation energies. The effect of the core–core electron correlation is largest for the more excited states. The final relative differences between calculated and observed excitation energies is 0.023%, which is small enough for the calculated energies to be of direct use in line identifications in astrophysical and laboratory spectra.

1. Introduction

Transitions from highly charged ions are observed in the spectra of astrophysical sources as well as in Tokamak and laser-produced plasmas, and they are routinely used for diagnostic purposes [1]. Often, transitions between configurations in the same complex are used, but transitions from higher lying configurations are also important (see, e.g., [2] for a discussion of the higher lying states in the case of Mg-like iron). Transition energies are available from experiments for many ions and collected in various data bases [3], but large amounts of data are still lacking. Although experimental work is aided by a new generation of light sources such as EBITs [4], spectral identifications are still a difficult and time-consuming task. A way forward is provided by theoretical transition energies that support line identification and render consistency checks for experimental level designations.
Much work has been done to improve both multiconfiguration methods and perturbative methods, each with their strengths and weaknesses, in order to provide theoretical transition energies of spectroscopic accuracy, i.e., transition energies with uncertainties of the same order as the ones obtained from experiments and observations using Chandra, Hinode or other space based missions in the X-ray and EUV spectral ranges [5,6,7,8]. Further advancements for complex systems with several electrons outside a closed atomic core calls for a combination of multiconfiguration and perturbative methods [9] and also for methods based on new principles [10,11].
In this paper, we describe how the multiconfiguration Dirac–Hartree–Fock (MCDHF) and relativistic configuration interaction (CI) methods can be modified to include perturbative corrections that account for core–core electron correlation. Taking Mg-like iron as an example, we show how the corrections improve excitation energies for the more highly excited states.

2. Relativistic Multiconfiguration Methods

2.1. Multiconfiguration Dirac–Hartree–Fock and Configuration Interaction

In the MCDHF method [12,13], as implemented in the GRASP2K program package [14], the wave function Ψ ( γ P J M J ) for a state labeled γ P J M J , where J and M J are the angular quantum numbers and P is the parity, is expanded in antisymmetrized and coupled configuration state functions (CSFs)
Ψ ( γ P J M J ) = j = 1 M c j Φ ( γ j P J M J ) .
The labels { γ j } denote other appropriate information of the configuration state functions, such as orbital occupancy and coupling scheme. The CSFs are built from products of one-electron orbitals, having the general form
ψ n κ , m ( r ) = 1 r P n κ ( r ) χ κ , m ( θ , φ ) ı Q n κ ( r ) χ κ , m ( θ , φ ) ,
where χ ± κ , m ( θ , φ ) are 2-component spin-orbit functions. The radial functions { P n κ ( r ) , Q n κ ( r ) } are numerically represented on a grid.
Wave functions for a number of targeted states are determined simultaneously in the extended optimal level (EOL) scheme. Given initial estimates of the radial functions, the energies E and expansion coefficients c = ( c 1 , , c M ) t for the targeted states are obtained as solutions to the configuration interaction (CI) problem
H c = E c ,
where H is the CI matrix of dimension M × M with elements
H i j = Φ ( γ i P J M J ) | H | Φ ( γ j P J M J ) .
In relativistic calculations, the Hamiltonian H is often taken as the Dirac–Coulomb Hamiltonian. Once the expansion coefficients have been determined, the radial functions are improved by solving a set of differential equations results from applying the variational principle on a weighted energy functional of the targeted states together with additional terms needed to preserve orthonormality of the orbitals. The CI problem and the solution of the differential equations are iterated until the radial orbitals and the energy are converged to a specified tolerance.
The MCDHF calculations are often followed by CI calculations where terms representing the transverse photon interaction are added to the Dirac-Coulomb Hamiltonian and the vacuum polarization effects are taken into account by including the Uehling potential. Electron self-energies are calculated with the screened hydrogenic formula [12,15]. Due to the relative simplicity of the CI method, often much larger expansions are included in the final CI calculations compared to the MCDHF calculations.

2.2. Large Expansions and Perturbative Corrections

The number of CSFs in the wave function expansions depend on the shell structure of the ionic system as well as the model for electron correlation (to be discussed in Section 3). For accurate calculations, a large number of CSFs are required, leading to very large matrices. To handle these large matrices, the CSFs can a priori be divided into two groups. The first group, P, with m elements ( m M ) contains CSFs that account for the major parts of the wave functions. The second group, Q, with M m elements contains CSFs that represent minor corrections. Allowing interaction between CSFs in group P, interaction between CSFs in group P and Q and diagonal interactions between CSFs in Q gives a matrix
H ( P P ) H ( P Q ) H ( Q P ) H ( Q Q ) ,
where H i j ( Q Q ) = δ i j E i Q . The restriction of H ( Q Q ) to diagonal elements results in a huge reduction in the total number of matrix elements and corresponding computational time. The assumptions of the approximation and the connections to the method of deflation in numerical analysis are discussed in [13]. This form of the CI matrix, which has been available in the non-relativistic and relativistic multiconfiguration codes for a long time [16,17], yields energies that are similar to the ones obtained by applying second-order perturbation theory (PT) corrections to the energies of the smaller m × m matrix. The method is therefore referred to here as CI combined with second-order Brillouin–Wigner perturbation theory [18]. Note, however, that the CI method with restrictions on the interactions gives, in contrast to ordinary perturbative methods, wave functions that can be directly used to evaluate expectation values such as transition rates.

3. Calculations

Calculations were performed for states belonging to the 3 s 2 , 3 p 2 , 3 s 3 d , 3 d 2 , 3 s 4 s , 3 s 4 d , 3 p 4 p , 3 p 4 f , 3 d 4 s , 3 d 4 d , 3 s 5 s , 3 s 5 d , 3 s 5 g even configurations and the 3 s 3 p , 3 p 3 d , 3 s 4 p , 3 p 4 s , 3 s 4 f , 3 p 4 d , 3 d 4 p , 3 d 4 f , 3 s 5 p , 3 s 5 f odd configurations of Mg-like iron. For 3 d 4 f , only states below the 3 p 5 s configuration were included. The above configurations define the multireference (MR) for the even and odd parities, respectively. Following the procedure in [19], an initial MCDHF calculation for all even and odd reference states was done in the EOL scheme. The initial calculation was followed by separate calculations in the EOL scheme for the even and odd parity states. The MCDHF calculations for the even states were based on CSF expansions obtained by allowing single (S) and double (D) substitutions of orbitals in the even MR configurations to an increasing active set of orbitals. In a similar way, the calculations for the odd states were based on CSF expansions obtained by allowing single (S) and double (D) substitutions of orbitals in the odd MR configurations to an increasing active set of orbitals. To prevent the CSF expansions from growing unmanageably large and in order to obtain orbitals that are spatially localized in the valence and core–valence region, at most, single substitutions were allowed from the 2 s 2 2 p 6 core. The 1 s 2 shell was always closed. The active sets of orbitals for the even and odd parity states were extended by layers to include orbitals with quantum numbers up to n = 8 and l = 6 , at which point the excitation energies are well converged.
To investigate the effects of electron correlation, three sets of CI calculations were done. In the first set of CI calculations, one calculation was done for the even states and one calculation for the odd states, the SD substitutions were only allowed from the valence shells of the MR, and the CSFs account for valence–valence correlation. In the second set of calculations, SD substitutions were such that there was at most one substitution from the 2 s 2 2 p 6 core, and the CSFs account for valence–valence and core–valence correlation. In the final set of calculations, all SD substitutions were allowed, and the CSFs account for valence–valence, core–valence and core–core correlation. When all substitutions are allowed, the number of CSFs grows very large. For this reason, we apply CI with second-order perturbation corrections. The CSFs describing valence–valence and core–valence effects (SD substitutions with at most one substitution from the 2 s 2 2 p 6 core) were included in group P, whereas the CSFs accounting for core–core correlation (D substitutions from 2 s 2 2 p 6 ) were included in group Q and treated in second-order perturbation theory. The number of CSFs for the different CI calculations are given in Table 1.

4. Results

The excitation energies from the different CI calculations, along with observed energies from the NIST database [3], are displayed in Table 2. From the table, we see that states belonging to 3 l 3 l , with the exception of 3 s 3 p   3 P 0 , 1 , 2 , are too high for the valence–valence correlation calculation. The states belonging to 3 l 4 l and 3 s 5 l , on the other hand, are too low. When including also the core–valence correlation, the states belonging to 3 l 3 l go down in energy and approach the observed excitation energies. The states belonging to 3 l 4 l and 3 s 5 l go up and are now too high. Including also the core–core correlation results in a rather small energy change for the states belonging to 3 l 3 l . The main effect of the core–core correlation is to lower the energies of the states belonging to 3 l 4 l and 3 s 5 l , bringing them in very good agreement with observations. The labeling of levels is normally done by looking at the quantum designation of the leading component in the CSF expansion [20]. There are two levels (67 and 69) with 3 p 4 d   3 D 3 as the leading component in the corresponding CSF expansion. To distinguish these levels, we added subscripts A and B to the labels of the dominant component. In a similar way, subscripts A and B were added to distinguish levels 78 and 80, both with 3 p 4 f   3 F 3 as the leading component.
Table 2 indicates that there are a few states that are either misidentified or assigned with a label that is inconsistent with the labels of the current calculation. The observed energy for 3 p 4 f   3 D 2 (level 84) is 2417 cm 1 too low compared to the calculated value and the observed energy for 3 s 5 s   3 S 1 (level 92) is 33,948 cm 1 too high. There seem to be no other computed energy levels that match the observed energies. The observed energy for 3 s 5 p   1 P 1 o (level 100) is 3733 cm 1 too low. The observed energy matches the computed energy of 3 s 5 p   3 P 1 o (level 97), and, thus, it seems like an inconsistency in the labeling. Finally, 3 s 5 f   1 F 3 o (level 117) is 101,545 cm 1 too high and there is no other computed energy level that matches. Removing the energy outliers above, the mean relative energy differences are, respectively, 0.217%, 0.051%, 0.023% for the valence, the valence and core–valence and the valence, core–valence and core–core calculations. The energy differences are mainly due to higher-order electron correlation effects that have not been accounted for in the calculations. At the same time, one should bear in mind that the observed excitation energies are also associated with uncertainties as reflected in the limited number of valid digits displayed in the NIST tables.
In Table 3, the excitation energies obtained by including core–core correlation in the CI calculations are compared with energies from calculations by Landi [2] using the FAC code and with energies by Aggarwal et al. [21] using CIV3 in the Breit–Pauli approximation. The uncertainties of the excitation energies for the latter calculations are substantially larger. The calculations by Landi support the conclusion that some of the levels in the NIST database are misidentified. One may note that Landi gives levels 78 and 80 the labels 3 p 4 f   3 F 3 and 3 p 4 f   1 F 3 , respectively, whereas Aggarwal et al. reverse the labels. This illustrates that labeling is dependent on the calculation and that the labeling process is far from straightforward [20].

5. Conclusions

CI with restrictions on the interactions (CI combined with second-order Brillouin–Wigner perturbation theory) makes it possible to handle large CSF expansions. The calculations including core–core correlation take around 20 h with 10 nodes on a cluster and bring the computed and observed excitation energies into very good agreement. To improve the computed excitation energies, the orbital set would need to be further extended leading to even larger matrices. The combined CI and perturbation method can be applied to include core–valence correlation in systems with many valence electrons and calculations. Calculations including valence–valence correlation and where core–valence correlation is treated perturbatively are in progress for P-, S-, and Cl-like systems.

Acknowledgments

Per Jönsson gratefully acknowledges support from the Swedish Research Council under contract 2015-04842.

Author Contributions

All authors contributed equally to the work.

Conflicts of Interest

The authors declare no conflicts of interest.

References

  1. Young, P.R.; Del Zanna, G.; Mason, H.E.; Dere, K.P.; Landi, E.; Landini, M.; Doschek, G.A.; Brown, C.M.; Culhane, L.; Harra, L.K.; et al. EUV Emission Lines and Diagnostics Observed with Hinode/EIS. Publ. Astron. Soc. Jpn. 2007, 59, S857–S864. [Google Scholar] [CrossRef]
  2. Landi, E. Atomic data and spectral line intensities for Fe XV. At. Data Nucl. Data Tables 2011, 97, 587–647. [Google Scholar] [CrossRef]
  3. Kramida, A.; Ralchenko, Y.; Reader, J.; NIST ASD Team. Atomic Spectra Database (ver. 5.2); National Institute of Standards and Technology: Gaithersburg, MD, USA, 2014. Available online: http://physics.nist.gov/asd (accessed on 28 december 2014).
  4. Brown, G.V.; Beiersdorfer, P.; Utter, S.B.; Boyce, K.R.; Gendreau, K.C.; Kelley, R.; Porter, F.S.; Gygax, J. Measurements of Atomic Parameters of Highly Charged Ions for Interpreting Astrophysical Spectra. Phys. Scr. 2001. [Google Scholar] [CrossRef]
  5. Jönsson, P.; Bengtsson, P.; Ekman, J.; Gustafsson, S.; Karlsson, L.B.; Gaigalas, G.; Froese Fischer, C.; Kato, D.; Murakami, I.; Sakaue, H.A.; et al. Relativistic CI calculations of spectroscopic data for the 2p6 and 2p53l configurations in Ne-like ions between Mg III and Kr XXVII. At. Data Nucl. Data Tables 2014, 100, 1–154. [Google Scholar] [CrossRef]
  6. Wang, K.; Guo, X.L.; Li, S.; Si, R.; Dang, W.; Chen, Z.B.; Jönsson, P.; Hutton, R.; Chen, C.Y.; Yan, J. Calculations with spectroscopic accuracy: Energies and transition rates in the nitrogen isoelectronic sequence from Ar XII to Zn XXIV. Astrophys. J. Suppl. Ser. 2016, 223, 33. [Google Scholar]
  7. Vilkas, M.J.; Ishikawa, Y. High-accuracy calculations of term energies and lifetimes of silicon-like ions with nuclear charges Z = 24 − 30. J. Phys. B At. Mol. Opt. Phys. 2004, 37, 1803–1816. [Google Scholar] [CrossRef]
  8. Gu, M.F. Energies of 1s22lq (1 ≤ q ≤ 8) states for Z ≤ 60 with a combined configuration interaction and many-body perturbation theory approach. At. Data Nucl. Data Tables 2005, 89, 267–293. [Google Scholar] [CrossRef]
  9. Kozlov, M.G.; Porsev, S.G.; Safronova, M.S.; Tupitsyn, I.I. CI-MBPT: A package of programs for relativistic atomic calculations based on a method combining configuration interaction and many-body perturbation theory. Comput. Phys. Commun. 2015, 195, 199–213. [Google Scholar] [CrossRef]
  10. Verdebout, S.; Rynkun, P.; Jönsson, P.; Gaigalas, G.; Froese Fischer, C.; Godefroid, M. A partitioned correlation function interaction approach for describing electron correlation in atoms. J. Phys. B At. Mol. Opt. Phys. 2013, 46, 085003. [Google Scholar] [CrossRef]
  11. Dzuba, V.A.; Berengut, J.; Harabati, C.; Flambaum, V.V. Combining configuration interaction with perturbation theory for atoms with large number of valence electrons. 2016; arXiv:1611.00425v1. [Google Scholar]
  12. Grant, I.P. Relativistic Quantum Theory of Atoms and Molecules; Springer: New York, NY, USA, 2007. [Google Scholar]
  13. Froese Fischer, C.; Godefroid, M.; Brage, T.; Jönsson, P.; Gaigalas, G. Advanced multiconfiguration methods for complex atoms: Part I—Energies and wave functions. J. Phys. B At. Mol. Opt. Phys. 2016, 49, 182004. [Google Scholar] [CrossRef]
  14. Jönsson, P.; Gaigalas, G.; Bieroń, J.; Froese Fischer, C.; Grant, I.P. New Version: Grasp2K relativistic atomic structure package. Comput. Phys. Commun. 2013, 184, 2197–2203. [Google Scholar] [CrossRef]
  15. McKenzie, B.J.; Grant, I.P.; Norrington, P.H. A program to calculate transverse Breit and QED corrections to energylevels in a multiconfiguration Dirac-Fock environment. Comput. Phys. Commun. 1980, 21, 233–246. [Google Scholar] [CrossRef]
  16. Froese Fischer, C. The MCHF atomic-structure package. Comput. Phys. Commun. 1991, 64, 369–398. [Google Scholar] [CrossRef]
  17. Parpia, F.A.; Froese Fischer, C.; Grant, I.P. GRASP92: A package for large-scale relativistic atomic structure calculations. Comput. Phys. Commun. 1996, 94, 249–271. [Google Scholar] [CrossRef]
  18. Kotochigova, S.; Kirby, K.P.; Tupitsyn, I. Ab initio fully relativistic calculations of x-ray spectra of highly charged ions. Phys. Rev. A 2007, 76, 052513. [Google Scholar] [CrossRef]
  19. Gustafsson, S.; Jönsson, P.; Froese Fischer, C.; Grant, I.P. MCDHF and RCI calculations of energy levels, lifetimes and transition rates for 3l3l, 3l4l and 3s5l states in Ca IX—As XXII and Kr XXV. Astron. Astrophys. 2017, 579, A76. [Google Scholar] [CrossRef]
  20. Gaigalas, G.; Froese Fischer, C.; Rynkun, P.; Jönsson, P. JJ2LSJ transformation and unique labeling for energy levels. Atoms 2016. submitted. [Google Scholar]
  21. Aggarwal, K.M.; Tayal, V.; Gupta, G.P.; Keenan, F.P. Energy levels and radiative rates for transitions in Mg-like iron, cobalt and nickel. At. Data Nucl. Data Tables 2007, 93, 615–710. [Google Scholar] [CrossRef]
Table 1. Number of CSFs for the even and odd parity expansions for the different sets of CI calculations. VV are the expansions accounting for valence–valence correlation, VV+CV are the expansions accounting for valence–valence and core–valence correlation and VV+CV+CC are the expansions accounting for valence-valence, core–valence and core–core correlation.
Table 1. Number of CSFs for the even and odd parity expansions for the different sets of CI calculations. VV are the expansions accounting for valence–valence correlation, VV+CV are the expansions accounting for valence–valence and core–valence correlation and VV+CV+CC are the expansions accounting for valence-valence, core–valence and core–core correlation.
VVVV+CVVV+CV+CC
even2738644,3425,624,158
odd2728630,5026,214,393
Table 2. Comparison of calculated and observed excitation energies in Mg-like iron (Fe XV). E V V are energies from CI calculations that account for valence–valence correlation. E V V + C V are energies from CI calculations that account for valence–valence and core–valence electron correlation. E V V + C V + C C are energies that account for valence–valence and core–valence electron correlation and where core–core electron correlation effects have been included perturbatively. E N I S T are observed energies from the NIST database ([3]). Δ E are energy differences with respect to E N I S T . All energies are in cm 1 .
Table 2. Comparison of calculated and observed excitation energies in Mg-like iron (Fe XV). E V V are energies from CI calculations that account for valence–valence correlation. E V V + C V are energies from CI calculations that account for valence–valence and core–valence electron correlation. E V V + C V + C C are energies that account for valence–valence and core–valence electron correlation and where core–core electron correlation effects have been included perturbatively. E N I S T are observed energies from the NIST database ([3]). Δ E are energy differences with respect to E N I S T . All energies are in cm 1 .
No.Level E VV Δ E E VV + CV Δ E E VV + CV + CC Δ E E NIST
1 3 s 2   1 S 0 0000000
2 3 s 3 p   3 P 0 o 233,087−755233,828−14233,92886233,842
3 3 s 3 p   3 P 1 o 238,936−724239,6688239,74181239,660
4 3 s 3 p   3 P 2 o 253,017−803253,8299253,773−47253,820
5 3 s 3 p   1 P 1 o 354,9413030352,169258352,091180351,911
6 3 p 2   3 P 0 556,5942070554,643119554,895371554,524
7 3 p 2   1 D 2 559,900300559,834234559,66161559,600
8 3 p 2   3 P 1 566,5241922564,66361564,6747256,4602
9 3 p 2   3 P 2 583,3271524581,933130581,87067581,803
10 3 p 2   1 S 0 662,9993372660,269642660,229602659,627
11 3 s 3 d   3 D 1 680,5221750678,954182678,329−443678,772
12 3 s 3 d   3 D 2 681,5201735679,986201679,381−404679,785
13 3 s 3 d   3 D 3 683,0801664681,603187680,952−464681,416
14 3 s 3 d   1 D 2 766,6904597762,729636762,17683762,093
15 3 p 3 d   3 F 2 o 929,158917928,565324928,086−155928,241
16 3 p 3 d   3 F 3 o 938,885759938,469343938,068−58938,126
17 3 p 3 d   1 D 2 o 950,2261713948,768255948,383−130948,513
18 3 p 3 d   3 F 4 o 950,300642949,990332949,451−207949,658
19 3 p 3 d   3 D 1 o 986,2213353983,077209982,740−128982,868
20 3 p 3 d   3 P 2 o 986,4992985983,765251983,350−164983,514
21 3 p 3 d   3 D 3 o 998,3243472995,088236994,712−140994,852
22 3 p 3 d   3 P 0 o 998,5972708996,218329995,835−54995,889
23 3 p 3 d   3 P 1 o 999,1662923996,547304996,127−116996,243
24 3 p 3 d   3 D 2 o 999,7553132996,892269996,449−174996,623
25 3 p 3 d   1 F 3 o 1,066,90643911,063,1636481,062,7041891,062,515
26 3 p 3 d   1 P 1 o 1,078,91340261,075,7959081,075,3064191,074,887
27 3 d 2   3 F 2 1,373,37430431,370,8585271,369,758−5731,370,331
28 3 d 2   3 F 3 1,374,98329481,372,5274921,371,407−6281,372,035
29 3 d 2   3 F 4 1,376,96529091,374,5805241,373,475−5811,374,056
30 3 d 2   1 D 2 1,405,70231101,403,4748821,402,237−3551,402,592
31 3 d 2   3 P 0 1,409,066 1,406,328 1,405,381
32 3 d 2   3 P 1 1,409,639 1,406,926 1,405,672
33 3 d 2   1 G 4 1,409,70226441,407,9749161,406,831−2271,407,058
34 3 d 2   3 P 2 1,411,05332801,408,4676941,407,210−5631,407,773
35 3 d 2   1 S 0 1,489,91328591,488,99319391,487,4604061,487,054
36 3 s 4 s   3 S 1 1,761,471−22291,764,876117617,63,699−11,763,700
37 3 s 4 s   1 S 0 1,785,265−17351,788,45514551,787,3223221,787,000
38 3 s 4 p   3 P 0 o 1,880,014 1,883,187 1,882,236
39 3 s 4 p   3 P 1 o 1,880,440 1,883,595 1,882,588
40 3 s 4 p   3 P 2 o 1,887,508 1,890,703 1,889,632
41 3 s 4 p   1 P 1 o 1,887,872−20981,891,05110811,890,042721,889,970
42 3 s 4 d   3 D 1 2,029,659−16512,032,90715972,031,6833732,031,310
43 3 s 4 d   3 D 2 2,030,413−16072,033,65316332,032,4133932,032,020
44 3 s 4 d   3 D 3 2,031,636−15442,034,88017002,033,6234432,033,180
45 3 s 4 d   1 D 2 2,032,991−22892,036,31810382,035,053−2272,035,280
46 3 p 4 s   3 P 0 o 2,051,314 2,053,909 2,053,031
47 3 p 4 s   3 P 1 o 2,054,922 2,057,446 2,056,493
48 3 p 4 s   3 P 2 o 2,071,700 2,074,376 2,073,372
49 3 p 4 s   1 P 1 o 2,085,097 2,087,237 2,086,235
50 3 s 4 f   3 F 2 o 2,105,597−29232,109,82113012,108,281−2392,108,520
51 3 s 4 f   3 F 3 o 2,105,804−28162,110,02914092,108,503−1172,108,620
52 3 s 4 f   3 F 4 o 2,106,098−27822,110,32714472,108,798−822,108,880
53 3 s 4 f   1 F 3 o 2,120,519−26312,124,65415042,123,180302,123,150
54 3 p 4 p   1 P 1 2,152,851 2,155,266 2,154,244
55 3 p 4 p   3 D 1 2,167,018 2,169,386 2,168,341
56 3 p 4 p   3 D 2 2,168,756 2,171,070 2,170,006
57 3 p 4 p   3 P 0 2,173,624 2,175,566 2,174,583
58 3 p 4 p   3 P 1 2,181,779 2,183,914 2,182,831
59 3 p 4 p   3 D 3 2,184,022 2,186,457 2,185,350
60 3 p 4 p   3 P 2 2,189,341 2,191,385 2,190,270
61 3 p 4 p   3 S 1 2,192,119 2,194,460 2,193,367
62 3 p 4 p   1 D 2 2,206,894 2,208,893 2,207,746
63 3 p 4 p   1 S 0 2,235,724 2,237,406 2,236,314
64 3 p 4 d   3 D 1 o 2,311,660 2,314,071 2,313,090
65 3 p 4 d   1 D 2 o 2,311,989 2,314,331 2,313,312
66 3 p 4 d   3 D 2 o 2,312,449 2,314,882 2,313,865
67 3 p 4 d   3 D 3 A o 2,313,908 2,316,401 2,315,387
68 3 p 4 d   3 F 2 o 2,329,261 2,331,722 2,330,678
69 3 p 4 d   3 D 3 B o 2,330,539 2,333,084 2,332,039
70 3 p 4 d   3 F 4 o 2,337,384 2,339,922 2,338,857
71 3 p 4 d   1 F 3 o 2,337,651 2,340,302 2,339,278
72 3 p 4 d   3 P 2 o 2,341,803 2,344,120 2,343,033
73 3 p 4 d   3 P 1 o 2,342,778 2,345,091 2,344,049
74 3 p 4 d   3 P 0 o 2,346,915 2,349,198 2,348,199
75 3 p 4 d   1 P 1 o 2,350,169 2,352,543 2,351,513
76 3 p 4 f   3 G 3 2,377,507−26532,381,28311232,379,714−4462,380,160
77 3 p 4 f   3 G 4 2,384,217−24832,387,97612762,386,434−2662,386,700
78 3 p 4 f   3 F 3 A 2,384,435 2,388,118 2,386,537
79 3 p 4 f   3 F 2 2,388,049−20512,391,67015702,390,091−92,390,100
80 3 p 4 f   3 F 3 B 2,397,860 2,401,630 2,400,029
81 3 p 4 f   3 G 5 2,399,542−25582,403,45313532,401,876−2242,402,100
82 3 p 4 f   3 F 4 2,400,524−15762,404,28621862,402,6975972,402,100
83 3 p 4 f   3 D 3 2,411,680−13202,415,36823682,413,7587582,413,000
84 3 p 4 f   3 D 2 2,414,6333332,418,31940192,416,71724172,414,300
85 3 p 4 f   3 D 1 2,417,852−22482,421,55714572,419,975−1252,420,100
86 3 p 4 f   1 G 4 2,426,828−18722,430,49717972,429,0633632,428,700
87 3 p 4 f   1 D 2 2,433,430−25702,437,03910392,435,534−4662,436,000
88 3 d 4 s   3 D 1 2,458,614 2,460,640 2,458,997
89 3 d 4 s   3 D 2 2,459,450 2,461,503 2,459,846
90 3 d 4 s   3 D 3 2,461,283 2,463,415 2,461,742
91 3 d 4 s   1 D 2 2,468,780 2,470,737 2,469,163
92 3 s 5 s   3 S 1 2,507,700−37,1002,512,036−32,7642,510,852−33,9482,544,800
93 3 s 5 s   1 S 0 2,516,613 2,520,681 2,519,752
94 3 d 4 p   1 D 2 o 2,561,358 2,563,408 2,561,899
95 3 d 4 p   3 D 1 o 2,564,069 2,567,301 2,565,949
96 3 s 5 p   3 P 0 o 2,564,472 2,568,582 2,567,624
97 3 s 5 p   3 P 1 o 2,565,848 2,568,791 2,567,639
98 3 d 4 p   3 D 2 o 2,567,134 2,569,092 2,567,703
99 3 d 4 p   3 D 3 o 2,568,154 2,571,175 2,569,693
100 3 s 5 p   1 P 1 o 2,568,20012002,571,83448342,570,73337332,567,000
101 3 s 5 p   3 P 2 o 2,569,213 2,572,157 2,570,743
102 3 d 4 p   3 F 2 o 2,570,296 2,572,316 2,571,126
103 3 d 4 p   3 F 3 o 2,573,116 2,575,101 2,573,592
104 3 d 4 p   3 F 4 o 2,576,139 2,578,374 2,576,829
105 3 d 4 p   3 P 1 o 2,583,286 2,585,242 2,583,862
106 3 d 4 p   3 P 2 o 2,583,400 2,585,407 2,583,960
107 3 d 4 p   3 P 0 o 2,583,734 2,585,658 2,584,322
108 3 d 4 p   1 F 3 o 2,592,868 2,594,519 2,593,236
109 3 d 4 p   1 P 1 o 2,603,279 2,605,145 2,604,533
110 3 s 5 d   3 D 1 2,637,190−29102,641,40013002,640,2471472,640,100
111 3 s 5 d   3 D 2 2,637,419−24812,641,63017302,640,4425422,639,900
112 3 s 5 d   3 D 3 2,637,852−24482,642,07217722,640,8705702,640,300
113 3 s 5 d   1 D 2 2,639,773 2,643,981 2,642,888
114 3 s 5 f   3 F 2 o 2,672,676−37242,677,3609602,675,889−5112,676,400
115 3 s 5 f   3 F 3 o 2,672,770−36302,677,45510552,675,988−4122,676,400
116 3 s 5 f   3 F 4 o 2,672,907−36932,677,5949942,676,123−4772,676,600
117 3 s 5 f   1 F 3 o 2,678,041−104,6592,682,597−100,1032,681,155−101,5452,782,700
118 3 s 5 g   3 G 3 2,682,487 2,687,368 2,685,680
119 3 s 5 g   3 G 4 2,682,654 2,687,556 2,685,877
120 3 s 5 g   3 G 5 2,682,855 2,687,777 2,686,099
121 3 s 5 g   1 G 4 2,685,580 2,690,506 2,688,841
122 3 d 4 d   1 F 3 2,699,116 2,701,602 2,699,874
123 3 d 4 d   3 D 1 2,703,542 2,705,972 2,704,354
124 3 d 4 d   3 D 2 2,704,742 2,707,218 2,705,580
125 3 d 4 d   3 D 3 2,706,116 2,708,636 2,706,964
126 3 d 4 d   3 G 3 2,707,934 2,710,522 2,708,828
127 3 d 4 d   1 P 1 2,709,315 2,711,813 2,710,163
128 3 d 4 d   3 G 4 2,709,360 2,711,928 2,710,264
129 3 d 4 d   3 G 5 2,711,220 2,713,878 2,712,174
130 3 d 4 d   3 S 1 2,720,698 2,723,175 2,721,783
131 3 d 4 d   3 F 2 2,726,309 2,728,092 2,726,350
132 3 d 4 d   3 F 3 2,727,568 2,729,398 2,727,634
133 3 d 4 d   3 F 4 2,729,029 2,730,908 2,729,156
134 3 d 4 d   1 D 2 2,741,839 2,743,862 2,742,627
135 3 d 4 d   3 P 0 2,744,213 2,746,022 2,744,706
136 3 d 4 d   3 P 1 2,744,807 2,746,626 2,745,163
137 3 d 4 d   3 P 2 2,745,935 2,747,809 2,746,300
138 3 d 4 d   1 G 4 2,748,985 2,751,121 2,749,474
139 3 d 4 f   3 H 4 o 2,765,833 2,770,098 2,768,443
140 3 d 4 f   1 G 4 o 2,767,533 2,771,821 2,770,030
141 3 d 4 f   3 H 5 o 2,767,692 2,771,943 2,770,434
142 3 d 4 d   1 S 0 2,775,538 2,779,275 2,777,362
143 3 d 4 f   3 F 2 o 2,776,151 2,779,298 2,778,011
144 3 d 4 f   3 F 3 o 2,776,264 2,779,933 2,778,867
145 3 d 4 f   3 F 4 o 2,776,981 2,780,796 2,780,729
146 3 d 4 f   1 D 2 o 2,786,768 2,790,305 2,788,248
Table 3. Comparison of calculated and observed excitation energies in Mg-like iron (Fe XV). E V V + C V + C C are energies that account for valence–valence and core–valence electron correlation and where core–core electron correlation effects have been included perturbatively. E F A C are energies by Landi [2] using the FAC code. E C I V 3 are energies by Aggarwal et al. [21] using the CIV3 code. E N I S T are observed energies from the NIST database ([3]). Δ E are energy differences with respect to E N I S T . All energies are in cm 1 .
Table 3. Comparison of calculated and observed excitation energies in Mg-like iron (Fe XV). E V V + C V + C C are energies that account for valence–valence and core–valence electron correlation and where core–core electron correlation effects have been included perturbatively. E F A C are energies by Landi [2] using the FAC code. E C I V 3 are energies by Aggarwal et al. [21] using the CIV3 code. E N I S T are observed energies from the NIST database ([3]). Δ E are energy differences with respect to E N I S T . All energies are in cm 1 .
No.Level E VV + CV + VV Δ E E FAC Δ E E CIV 3 Δ E E NIST
1 3 s 2   1 S 0 0000000
2 3 s 3 p   3 P 0 o 233,92886233,068−774235,0131171233,842
3 3 s 3 p   3 P 1 o 239,74181238,900−760240,511851239,660
4 3 s 3 p   3 P 2 o 253,773−47252,917−903253,548−272253,820
5 3 s 3 p   1 P 1 o 352,091180356,1264215356,2624351351,911
6 3 p 2   3 P 0 554,895371556,9942470560,2755751554,524
7 3 p 2   1 D 2 559,66161560,266666563,2163616559,600
8 3 p 2   3 P 1 564,67472566,8322230569,2954693564,602
9 3 p 2   3 P 2 581,87067583,5641761584,8563053581,803
10 3 p 2   1 S 0 660,229602665,7686141665,2605633659,627
11 3 s 3 d   3 D 1 678,329−443680,1461374687,6808908678,772
12 3 s 3 d   3 D 2 679,381−404681,1291344688,73389486797,85
13 3 s 3 d   3 D 3 680,952−464682,6671251690,4018985681,416
14 3 s 3 d   1 D 2 762,17683769,3697276774,29512,202762,093
15 3 p 3 d   3 F 2 o 928,086−155928,786545938,26510,024928,241
16 3 p 3 d   3 F 3 o 938,068−58938,555429947,3079181938,126
17 3 p 3 d   1 D 2 o 948,383−130949,447934958,4029889948,513
18 3 p 3 d   3 F 4 o 949,451−207949,927269957,8208162949,658
19 3 p 3 d   3 D 1 o 982,740−128986,0823214995,52612,658982,868
20 3 p 3 d   3 P 2 o 983,350−164986,4072893995,76712,253983,514
21 3 p 3 d   3 D 3 o 994,712−140997,94430921,007,02612,174994,852
22 3 p 3 d   3 P 0 o 995,835−54998,76228731,006,70810,819995,889
23 3 p 3 d   3 P 1 o 996,127−116999,17329301,007,36611,123996,243
24 3 p 3 d   3 D 2 o 996,449−174999,57829551,008,12411,501996,623
25 3 p 3 d   1 F 3 o 1,062,7041891,070,79482791,077,45614,9411,062,515
26 3 p 3 d   1 P 1 o 1,075,3064191,083,82689391,089,69114,8041,074,887
27 3 d 2   3 F 2 1,369,758−5731,372,40020691,388,11117,7801,370,331
28 3 d 2   3 F 3 1,371,407−6281,373,98819531,389,83417,7991,372,035
29 3 d 2   3 F 4 1,373,475−5811,375,93818821,391,94117,8851,374,056
30 3 d 2   1 D 2 1,402,237−3551,407,42848361,421,70219,1101,402,592
31 3 d 2   3 P 0 1,405,381 1,409,507 1,424,577
32 3 d 2   3 P 1 1,405,672 1,410,109 1,425,246
33 3 d 2   1 G 4 1,406,831−2271,412,12750691,425,87218,8141,407,058
34 3 d 2   3 P 2 1,407,210−5631,411,64338701,426,81519,0421,407,773
35 3 d 2   1 S 0 1,487,4604061,498,66811,6141,508,95421,9001,487,054
36 3 s 4 s   3 S 1 1,763,699−11,760,910−27901,764,0053051,763,700
37 3 s 4 s   1 S 0 1,787,3223221,786,052−9481,787,9509501,787,000
38 3 s 4 p   3 P 0 o 1,882,236 1,880,319 1,883,685
39 3 s 4 p   3 P 1 o 1,882,588 1,880,746 1,884,091
40 3 s 4 p   3 P 2 o 1,889,632 1,887,756 1,890,313
41 3 s 4 p   1 P 1 o 1,890,042721,888,124−18461,890,6316611,889,970
42 3 s 4 d   3 D 1 2,031,6833732,029,563−17472,034,12428142,031,310
43 3 s 4 d   3 D 2 2,032,4133932,030,328−16922,034,84828282,0320,20
44 3 s 4 d   3 D 3 2,033,6234432,031,544−16362,036,05528752,033,180
45 3 s 4 d   1 D 2 2,035,053−2272,033,212−20682,037,56922892,035,280
46 3 p 4 s   3 P 0 o 2,053,031 2,051,778 2,055,797
47 3 p 4 s   3 P 1 o 2,056,493 2,055,514 2,059,308
48 3 p 4 s   3 P 2 o 2,073,372 2,072,083 2,074,452
49 3 p 4 s   1 P 1 o 2,086,235 2,086,607 2,088,795
50 3 s 4 f   3 F 2 o 2,108,281−2392,107,228−12922,110,07315532,108,520
51 3 s 4 f   3 F 3 o 2,108,503−1172,107,423−11972,110,28116612,108,620
52 3 s 4 f   3 F 4 o 2,108,798−822,107,701−11792,110,56716872,108,880
53 3 s 4 f   1 F 3 o 2,123,180302,124,0549042,125,88627362,123,150
54 3 p 4 p   1 P 1 2,154,244 2,167,343 2,158,599
55 3 p 4 p   3 D 1 2,168,341 2,153,046 2,171,635
56 3 p 4 p   3 D 2 2,170,006 2,169,173 2,173,578
57 3 p 4 p   3 P 0 2,174,583 2,175,103 2,178,812
58 3 p 4 p   3 P 1 2,182,831 2,182,790 2,185,901
59 3 p 4 p   3 D 3 2,185,350 2,184,242 2,187,229
60 3 p 4 p   3 P 2 2,190,270 2,190,674 2,193,265
61 3 p 4 p   3 S 1 2,193,367 2,192,597 2,195,756
62 3 p 4 p   1 D 2 2,207,746 2,209,221 2,211,163
63 3 p 4 p   1 S 0 2,236,314 2,239,314 2,241,187
64 3 p 4 d   3 D 1 o 2,313,090 2,311,999 2,318,014
65 3 p 4 d   1 D 2 o 2,313,312 2,312,326 2,318,179
66 3 p 4 d   3 D 2 o 2,313,865 2,312,835 2,318,826
67 3 p 4 d   3 D 3 A o 2,315,387 23,144,663 2,320,538
68 3 p 4 d   3 F 2 o 2,330,678 2,329,647 2,334,178
69 3 p 4 d   3 D 3 B o 2,332,039 2,331,0213 2,335,726
70 3 p 4 d   3 F 4 o 2,338,857 2,338,064 2,342,277
71 3 p 4 d   1 F 3 o 2,339,278 2,338,703 2,343,517
72 3 p 4 d   3 P 2 o 2,343,033 2,342,598 2,347,544
73 3 p 4 d   3 P 1 o 2,344,049 2,343,850 2,348,795
74 3 p 4 d   3 P 0 o 2,348,199 2,347,823 2,352,406
75 3 p 4 d   1 P 1 o 2,351,513 2,351,661 2,356,773
76 3 p 4 f   3 G 3 2,379,714−4462,379,430−7302,384,30641462,380,160
77 3 p 4 f   3 G 4 2,386,434−2662,386,688−122,391,19844982,386,700
78 3 p 4 f   3 F 3 A 2,386,537 2,386,430 2,390,473
79 3 p 4 f   3 F 2 2,390,091−92,390,112122,393,84237422,390,100
80 3 p 4 f   3 F 3 B 2,400,029 2,399,796 2,402,786
81 3 p 4 f   3 G 5 2,401,876−2242,401,746−3542,405,61735172,402,100
82 3 p 4 f   3 F 4 2,402,6975972,402,5074072,405,49633962,402,100
83 3 p 4 f   3 D 3 2,413,7587582,414,12011202,417,15141512,413,000
84 3 p 4 f   3 D 2 2,416,71724172,417,27629762,420,12458242,414,300
85 3 p 4 f   3 D 1 2,419,975−1252,420,5124122,423,21931192,420,100
86 3 p 4 f   1 G 4 2,429,0633632,432,90842082,435,82871282,428,700
87 3 p 4 f   1 D 2 2,435,534−4662,438,98229822,440,23942392,436,000
88 3 d 4 s   3 D 1 2,458,997 2,458,814 2,468,047
89 3 d 4 s   3 D 2 2,459,846 2,459,675 2,468,969
90 3 d 4 s   3 D 3 2,461,742 2,461,461 2,470,911
91 3 d 4 s   1 D 2 2,469,163 2,470,364 2,479,437
92 3 s 5 s   3 S 1 2,510,852−33,9482,507,572−37,228 2,544,800
93 3 s 5 s   1 S 0 2,519,752 2,517,043
94 3 d 4 p   1 D 2 o 2,561,899 2,561,169 2,571,814
95 3 d 4 p   3 D 1 o 2,565,949 2,566,041 2,576,851
96 3 s 5 p   3 P 0 o 2,567,624 2,564,597
97 3 s 5 p   3 P 1 o 2,567,639 2,564,254
98 3 d 4 p   3 D 2 o 2,567,703 2,567,341 2,577,905
99 3 d 4 p   3 D 3 o 2,569,693 2,569,518 2,583,117
100 3 s 5 p   1 P 1 o 2,570,73337332,568,3581358 2,567,000
101 3 s 5 p   3 P 2 o 2,570,743 2,568,240
102 3 d 4 p   3 F 2 o 2,571,126 2,570,526 2,580,319
103 3 d 4 p   3 F 3 o 2,573,592 2,573,370 2,579,847
104 3 d 4 p   3 F 4 o 2,576,829 2,576,531 2,586,036
105 3 d 4 p   3 P 1 o 2,583,862 2,584,287 2,593,158
106 3 d 4 p   3 P 2 o 2,583,960 2,584,326 2,593,586
107 3 d 4 p   3 P 0 o 2,584,322 2,584,699 2,593,641
108 3 d 4 p   1 F 3 o 2,593,236 2,596,425 2,604,571
109 3 d 4 p   1 P 1 o 2,604,533 2,607,817 2,610,870
110 3 s 5 d   3 D 1 2,640,2471472,637,143−2957 2,640,100
111 3 s 5 d   3 D 2 2,640,4425422,637,376−2524 2,639,900
112 3 s 5 d   3 D 3 2,640,8705702,637,804−2496 2,640,300
113 3 s 5 d   1 D 2 2,642,888 2,640,0840
114 3 s 5 f   3 F 2 o 2,675,889−5112,673,354−3046 2,676,400
115 3 s 5 f   3 F 3 o 2,675,988−4122,673,444−2956 2,676,400
116 3 s 5 f   3 F 4 o 2,676,123−4772,673,575−3025 2,676,600
117 3 s 5 f   1 F 3 o 2,681,155−101,5452,679,558−103,142 2,782,700
118 3 s 5 g   3 G 3 2,685,680 2,683,089
119 3 s 5 g   3 G 4 2,685,877 2,683,272
120 3 s 5 g   3 G 5 2,686,099 2,683,494
121 3 s 5 g   1 G 4 2,688,841 2,686,809
122 3 d 4 d   1 F 3 2,699,874 2,697,717 2,710,391
123 3 d 4 d   3 D 1 2,704,354 2,702,464 2,714,967
124 3 d 4 d   3 D 2 2,705,580 2,703,625 2,716,229
125 3 d 4 d   3 D 3 2,706,964 2,705,001 2,717,578
126 3 d 4 d   3 G 3 2,708,828 2,707,726 2,717,919
127 3 d 4 d   1 P 1 2,710,163 2,708,170 2,721,079
128 3 d 4 d   3 G 4 2,710,264 2,709,064 2,719,345
129 3 d 4 d   3 G 5 2,712,174 2,710,955 2,721,463
130 3 d 4 d   3 S 1 2,721,783 2,720,286 2,732,634
131 3 d 4 d   3 F 2 2,726,350 2,726,401 2,738,407
132 3 d 4 d   3 F 3 2,727,634 2,727,604 2,739,745
133 3 d 4 d   3 F 4 2,729,156 2,729,075 2,741,293
134 3 d 4 d   1 D 2 2,742,627 2,743,889 2,755,547
135 3 d 4 d   3 P 0 2,744,706 2,745,181 2,757,907
136 3 d 4 d   3 P 1 2,745,163 2,745,727 2,758,477
137 3 d 4 d   3 P 2 2,746,300 2,747,024 2,759,619
138 3 d 4 d   1 G 4 2,749,474 2,752,675 2,761,254
139 3 d 4 f   3 H 4 o 2,768,443 2,766,350 2,778,483
140 3 d 4 f   1 G 4 o 2,770,030 2,768,154 2,780,096
141 3 d 4 f   3 H 5 o 2,770,434 2,768,448 2,780,831
142 3 d 4 d   1 S 0 2,777,362 2,781,322 2,792,233
143 3 d 4 f   3 F 2 o 2,778,011 2,775,995 2,787,305
144 3 d 4 f   3 F 3 o 2,778,867 2,776,790 2,787,964
145 3 d 4 f   3 F 4 o 2,780,729 2,777,446 2,788,842
146 3 d 4 f   1 D 2 o 2,788,248 2,787,354 2,798,312

Share and Cite

MDPI and ACS Style

Gustafsson, S.; Jönsson, P.; Froese Fischer, C.; Grant, I. Combining Multiconfiguration and Perturbation Methods: Perturbative Estimates of Core–Core Electron Correlation Contributions to Excitation Energies in Mg-Like Iron. Atoms 2017, 5, 3. https://doi.org/10.3390/atoms5010003

AMA Style

Gustafsson S, Jönsson P, Froese Fischer C, Grant I. Combining Multiconfiguration and Perturbation Methods: Perturbative Estimates of Core–Core Electron Correlation Contributions to Excitation Energies in Mg-Like Iron. Atoms. 2017; 5(1):3. https://doi.org/10.3390/atoms5010003

Chicago/Turabian Style

Gustafsson, Stefan, Per Jönsson, Charlotte Froese Fischer, and Ian Grant. 2017. "Combining Multiconfiguration and Perturbation Methods: Perturbative Estimates of Core–Core Electron Correlation Contributions to Excitation Energies in Mg-Like Iron" Atoms 5, no. 1: 3. https://doi.org/10.3390/atoms5010003

APA Style

Gustafsson, S., Jönsson, P., Froese Fischer, C., & Grant, I. (2017). Combining Multiconfiguration and Perturbation Methods: Perturbative Estimates of Core–Core Electron Correlation Contributions to Excitation Energies in Mg-Like Iron. Atoms, 5(1), 3. https://doi.org/10.3390/atoms5010003

Note that from the first issue of 2016, this journal uses article numbers instead of page numbers. See further details here.

Article Metrics

Back to TopTop