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Theoretical Spectroscopy Group

Vilnius University

The Theoretical Spectroscopy Group at Vilnius University focuses on the production of various spectroscopic parameters such as level energies, spontaneous transition wavelengths and probabilities, absorption oscillators strengths, radiative lifetimes, Landé g-factors for light and heavy atoms and ions, including highly charged ones.

Our ab initio calculation of the spectroscopic data is performed in a quasirelativistic Hartree-Fock (QRHF) approach with transformed radial orbitals (TRO) implemented in the original computer code developed at VU Institute of Theoretical Physics and Astronomy. This QRHF approximation applied in our investigation is quite unique one and significantly differs from other widely-utilized relativistic or quasirelativistic methods especially in constructing one-electron radial orbitals.

For the level energy calculation, we include all two-electron interactions in the same way as it is done in conventional Breit–Pauli approximation. This similarity makes it possible to apply widely used tools for the angular integration of the Breit-Pauli Hamiltonian matrix elements and codes for the radiative transition operator matrix elements which have been adopted specifically for use with the QRHF radial orbitals. The electron correlation effects are included using a common configuration interaction (CI) approximation. The one-electron orbitals of configurations under consideration are determined by solving the QRHF equations. The virtually excited electrons of admixed (correlation) configurations included in CI are described by TROs with variable parameters. Originally the method of transformed radial orbitals was developed for the usual Hartree-Fock approximation and successfully used for investigation of the medium-Z ions. Consequently this method was adopted to the quasirelativistic radial orbitals.

We apply both quasirelativistic and non-relativistic radial orbitals in our codes to acquire theoretical spectroscopic data needed in fusion plasma and astrophysical research. Utilization of the QRHF+TRO approach makes it possible to produce atomic spectroscopic parameters for the multi-electron multi-charged heavy ions, including tungsten ions. This work has started within EURATOM framework and it is still ongoing in studies of the ground and excited levels of high-Z species. For the low-ionization atoms, usually a standard non-relativistic CI approximation based on the HF+TRO orbitals ensures that generated spectroscopic parameters are accurate enough for their application in astronomy and in astrophysical models. Here our main priority is to assess and evaluate the accuracy of produced spectral data. We continue to maintain and constantly update an open-access database for theoretical atomic data ADAMANT at Vilnius University which contains our generated spectroscopic and other atomic data for numerous ions.

Principal Researchers
  • Rasa Karpuškienė
  • Romas Kisielius
Contact

Dr Romualdas KISIELIUS
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, Vilnius, LT-10257, Lithuania
Email: romualdas.kisielius@tfai.vu.lt
Phone: +370 64641632

References
  • [1] R. Kisielius et al., "ATOMIC DATA FOR ZN II: IMPROVING SPECTRAL DIAGNOSTICS OF CHEMICAL EVOLUTION IN HIGH-REDSHIFT GALAXIES", The Astrophysical Journal 804, 76 (2015). [link to article]
  • [2] M. L. Lykins et al., "STOUT: CLOUDY’S ATOMIC AND MOLECULAR DATABASE", The Astrophysical Journal 807, 118 (2015). [link to article]
  • [3] K. Aggarwal et al., "Energy levels and radiative rates for Cr-like Cu VI and Zn VII", Atomic Data and Nuclear Data Tables 111-112, 280-345 (2016). [link to article]
  • [4] R. Karpuškienė, P. Bogdanovich and R. Kisielius, "Radiative transitions for three lowest configurations of tungsten ions W38+–W43+", Lithuanian Journal of Physics 57 (2017). [link to article]
  • [5] K. Aggarwal et al., "Energy levels and radiative rates for transitions in Fe V, Co VI and Ni VII", Atomic Data and Nuclear Data Tables 114, 1-60 (2017). [link to article]
  • [6] F. H. Cashman et al., "Atomic Data Revisions for Transitions Relevant to Observations of Interstellar, Circumgalactic, and Intergalactic Matter", The Astrophysical Journal Supplement Series 230, 8 (2017). [link to article]
  • [7] R. Karpuškienė and R. Kisielius, "Theoretical level energies and transition data for 4p64d5, 4p54d6 and 4p64d44f configurations of W33+ ion", Atomic Data and Nuclear Data Tables 125, 287-312 (2019). [link to article]
  • [8] R. Karpuškienė and R. Kisielius, "Theoretical level energies and transition data for ion W28+", Atomic Data and Nuclear Data Tables 132, 101309 (2020). [link to article]
  • [9] R. Karpuškienė and R. Kisielius, "Theoretical level energies and transition data for ion W29+", Atomic Data and Nuclear Data Tables 137, 101383 (2021). [link to article]
  • [10] R. Karpuškienė and R. Kisielius, "Theoretical level energies and transition data for 4p64d8, 4p54d9 and 4p64d74f configurations of W30+ ion", Atomic Data and Nuclear Data Tables 143, 101478 (2022). [link to article]

Keywords

Argon Astrophysics Electronic Structure Calculations Highly Charged Ions Neon Nitrogen Spectral Line Positions Spontaneous Emission Theory Tungsten