Optimized perturbation theory scheme for calculating the interatomic potentials and hyperfine lines shift for heavy atoms in the buffer inert gas

2009 ◽  
Vol 109 (14) ◽  
pp. 3325-3329 ◽  
Author(s):  
S. V. Malinovskaya ◽  
A. V. Glushkov ◽  
O. Yu. Khetselius ◽  
A. A. Svinarenko ◽  
E. V. Mischenko ◽  
...  

1989 ◽  
Author(s):  
V. A. Dzuba ◽  
V. V. Flambaum ◽  
P. G. Silvestrov ◽  
O. P. Sushkov


An expansion of the propagator S F (F) (x 2 , x 1 ) of a relativistic electron in a central static potential is given. The terms of this expansion correspond to the angular momenta of the electron propagated by this function. Applications to problems concerning heavy atoms are indicated.



A method for evaluating transition amplitudes for bound electrons in second order in the effects of the radiation field is outlined. An example of the type of problem concerned is the coherent scattering of γ -rays by the K electrons in heavy atoms. The static field in which the electron moves is taken into account exactly; no expansion is made in its effects. In the usual perturbation theory this is equivalent to summing matrix elements over intermediate states which are solutions of the wave equation including the static potential. In the method presented here, however, the sum over radial eigenstates for a particular angular momentum of intermediate state is replaced by quadratures of the products of known functions with the solution of a pair of coupled inhomogeneous differential equations.



2012 ◽  
Vol 397 ◽  
pp. 012037 ◽  
Author(s):  
T A Florko ◽  
S V Ambrosov ◽  
A A Svinarenko ◽  
T B Tkach
Keyword(s):  


Atoms ◽  
2021 ◽  
Vol 9 (4) ◽  
pp. 104
Author(s):  
Igor M. Savukov ◽  
Dmytro Filin ◽  
Pinghan Chu ◽  
Michael W. Malone

Heavy atoms present challenges to atomic theory calculations due to the large number of electrons and their complicated interactions. Conventional approaches such as calculations based on Cowan’s code are limited and require a large number of parameters for energy agreement. One promising approach is relativistic configuration-interaction and many-body perturbation theory (CI-MBPT) methods. We present CI-MBPT results for various atomic systems where this approach can lead to reasonable agreement: La I, La II, Th I, Th II, U I, Pu II. Among atomic properties, energies, g-factors, electric dipole moments, lifetimes, hyperfine structure constants, and isotopic shifts are discussed. While in La I and La II accuracy for transitions is better than that obtained with other methods, more work is needed for actinides.





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