Leading relativistic corrections for atomic P states calculated with a finite-nuclear-mass approach and all-electron explicitly correlated Gaussian functions
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PhysRevA.97.012513.pdf
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Univ Arizona, Dept Chem & BiochemUniv Arizona, Dept Phys
Issue Date
2018-01-25
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AMER PHYSICAL SOCCitation
Leading relativistic corrections for atomic P states calculated with a finite-nuclear-mass approach and all-electron explicitly correlated Gaussian functions 2018, 97 (1) Physical Review AJournal
Physical Review ARights
© 2018 American Physical Society.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
In this work we report progress in the development and implementation of quantum-mechanical methods for calculating bound ground and excited states of small atomic systems. The work concerns singlet states with the L = 1 total orbital angular momentum (P states). The method is based on the finite-nuclear-mass (non-Born-Oppenheimer; non-BO) approach and the use of all-particle explicitly correlated Gaussian functions for expanding the nonrelativistic wave function of the system. The development presented here includes derivation and implementation of algorithms for calculating the leading relativistic corrections for singlet states. The corrections are determined in the framework of the perturbation theory as expectation values of the corresponding effective operators using the non-BO wave functions. The method is tested in the calculations of the ten lowest P-1 states of the helium atom and the four lowest P-1 states of the beryllium atom.ISSN
2469-99262469-9934
Version
Final published versionSponsors
Polish National Science Centre [DEC-2013/10/E/ST4/00033]; Ministry of Education and Science of Kazakhstan; NSF [1228509]Additional Links
https://link.aps.org/doi/10.1103/PhysRevA.97.012513ae974a485f413a2113503eed53cd6c53
10.1103/PhysRevA.97.012513