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The ATSP2K and GRASP2K Multiconfiguration Atomic Structure Program Packages

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The ATSP2K and GRASP2K Multiconfiguration Atomic Structure

Program Packages

Per J¨onsson∗,1 Gediminas Gaigalas, Michel Godefroid, Jacek Biero´n∗∗, Charlotte Froese Fischerk,

Group for Materials Science and Applied Mathematics, Malm¨o University, Malm¨o, SwedenInstitute of Theoretical Physics and Astronomy, A. Gostauto 12, Vilnius LT-01108, LithuaniaService de Chimie Quantique et Photophysique, Universit´e Libre de Bruxelles B 1050 Brussels, Belgium

∗∗ Instytut Fizyki imienia Mariana Smoluchowskiego, Uniwersytet Jagiello´nski, Poland

k Atomic Physics Division, National Institute of Standards and Technology, Gaithersburg, Maryland, USA

Synopsis The ATSP2K and GRASP2K program packages for large scale atomic calculations are presented. A number of applications are given to illustrate the potential and restriction of the packages.

ATSP2K [1] and GRASP2K [2, 3] are two program packages designed primarily for large scale atomic calculations based on multiconfigu-ration methods. The ATSP2K is non-relativistic and adds relativistic corrections in the Breit-Pauli approximation. GRASP2K is fully rela-tivistic. By extensive use of default options to-gether with a naming convention for the files, the packages are user friendly with little input data for the typical cases. The program pack-ages are well documented [4] and comprehensive user manuals are available [3]. In both pack-ages the wave functions are given as expansions over configuration states functions that are built from antisymmetrized and coupled products of one-electron orbitals. The expansion coefficients and radial parts of the orbitals are determined in the self-consistent field procedure. Once one-electron orbitals are known configuration interac-tion can be performed, where higher order inter-actions such as the Breit interaction and quan-tum electrodynamic effects are added perturba-tively. Parallel processing using MPI allows large scale computing.

Both packages implement a biorthonormal transformation method that permits initial and final states in a transition array to be optimized separately, which, in many cases, leads to more accurate values of the resulting rates [5]. In ad-dition to energy structures and transition rates a number of other properties such as hyperfine structure, isotope shift with relativistic correc-tions to the normal and specific mass shift

op-erators [6] and splittings in external magnetic fields can be computed. New developments of the biorthonormal transformation methods allow general matrix elements between non-orthogonal states to be computed making an interesting link to continuum functions.

We present results for a number of systems and properties to illustrate the potential and re-striction of the packages. Among the properties are transition energies, hyperfine structures and isotope shifts in the boron-isoelectronic sequence, transition rates for nitrogen-like ions, Land´e gJ factors and splittings in external fields for neon-like ions.

References

[1] C. Froese Fischer, G. Tachiev, G. Gaigalas, and M R. Godefroid 2007 Comput. Phys. Commun. 176 559

[2] P. J¨onsson, X. He, C. Froese Fischer, and I.P. Grant 2007 Comput. Phys. Commun. 177 597 [3] P. J¨onsson, G. Gaigalas, J. Biero´n, C. Froese

Fis-cher, and I.P. Grant 2013 Comput. Phys. Com-mun., at press

[4] C. Froese Fischer, T. Brage, P. J¨onsson 1997 Computational Atomic Structure, IoP Publishing [5] J. Olsen, M. Godefroid, P. J¨onsson, P.˚A. Malmqvist and C. Froese Fischer 1995 Phys. Rev. E 52 4499

[6] C. Naz´e et al 2013 Comput. Phys. Commun., at press

References

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