Improvement of the basis for the solution of the Dirac equation in Cassini coordinates

We propose an improvement of the basis for the solution of the stationary two-centre Dirac equation in Cassini coordinates using the finite-basis-set method presented in our earlier article [J. Phys. B 43, 235207 (2010)]. For the calculations in the above article, we constructed the basis for approx...

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Bibliographic Details
Main Authors: Hahn, Walter (Author) , Artemyev, Anton (Author) , Surzhykov, Andrey (Author)
Format: Article (Journal)
Language:English
Published: 26 August 2017
In: Optics and spectroscopy
Year: 2017, Volume: 123, Issue: 2, Pages: 225-230
ISSN:1562-6911
DOI:10.1134/S0030400X17080094
Online Access:Verlag, Volltext: http://dx.doi.org/10.1134/S0030400X17080094
Verlag, Volltext: http://link.springer.com/10.1134/S0030400X17080094
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Author Notes:W. Hahn, A.N. Artemyev, and A. Surzhykov
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Summary:We propose an improvement of the basis for the solution of the stationary two-centre Dirac equation in Cassini coordinates using the finite-basis-set method presented in our earlier article [J. Phys. B 43, 235207 (2010)]. For the calculations in the above article, we constructed the basis for approximating the energy eigenfunctions by using smooth piecewise defined polynomials, called B-splines. In the present article, we report that an analysis of the employed representation of the Dirac matrices shows that the above approximation is not efficient using B-splines only. Therefore, we include basis functions which are defined using functions with step-like behavior instead of B-splines. Thereby, we achieve a significant increase of accuracy of results.
Item Description:Gesehen am 16.05.2018
Physical Description:Online Resource
ISSN:1562-6911
DOI:10.1134/S0030400X17080094