The asymptotic expansion method based on a core polarization potential for the Rydberg electron is reviewed and extended to the high angular momentum states of helium up to L=15. A comparison with recent large-scale configuration interaction calculations for the nonrelativistic energies shows that there is good agreement for L=7, but there are serious systematic disagreements for the states of higher angular momentum. A possible explanation is that there is an important class of configurations missing from the CI calculations. © 2009 The American Physical Society
The cross section for single K-shell ionization by a high-energy photon is evaluated in the next-to-...
Cosmological models can be constrained by determining primordial abundances. Accurate predictions of...
Photoelectron spectra of helium have been measured at different angles and at various energies above...
The asymptotic expansion method based on a core polarization potential for the Rydberg electron is r...
The results of an extended series of high-precision variational calculations for all states of heliu...
This paper extends the methods of asymptotic analysis extensively developed for energy-level calcula...
This paper reviews progress that has been made in obtaining essentially exact solutions to the nonre...
High-precision variational eigenvalues are obtained for the 10D, 10F, 10G and 10H states of helium b...
The aim of this work is to explore the range of validity of the asymptotic expansion method for a nu...
The aim of this work is to solve the quantum mechanical three-body problem for helium, and to obtain...
With a 12-parameter Hylleraas-type wave function containing only positive powers, a new calculation ...
The principal result of this paper is a general expression for the second-order dipole polarization ...
ERV accurate calculations of the energies of the 1s2 1S and 1s2s3S states of helium have been made r...
Cosmological models can be constrained by determining primordial abundances. Accurate predictions of...
Ground state ionization potential of the He^4 atom is evaluated to be 5 945 204 221 (42) MHz. Along ...
The cross section for single K-shell ionization by a high-energy photon is evaluated in the next-to-...
Cosmological models can be constrained by determining primordial abundances. Accurate predictions of...
Photoelectron spectra of helium have been measured at different angles and at various energies above...
The asymptotic expansion method based on a core polarization potential for the Rydberg electron is r...
The results of an extended series of high-precision variational calculations for all states of heliu...
This paper extends the methods of asymptotic analysis extensively developed for energy-level calcula...
This paper reviews progress that has been made in obtaining essentially exact solutions to the nonre...
High-precision variational eigenvalues are obtained for the 10D, 10F, 10G and 10H states of helium b...
The aim of this work is to explore the range of validity of the asymptotic expansion method for a nu...
The aim of this work is to solve the quantum mechanical three-body problem for helium, and to obtain...
With a 12-parameter Hylleraas-type wave function containing only positive powers, a new calculation ...
The principal result of this paper is a general expression for the second-order dipole polarization ...
ERV accurate calculations of the energies of the 1s2 1S and 1s2s3S states of helium have been made r...
Cosmological models can be constrained by determining primordial abundances. Accurate predictions of...
Ground state ionization potential of the He^4 atom is evaluated to be 5 945 204 221 (42) MHz. Along ...
The cross section for single K-shell ionization by a high-energy photon is evaluated in the next-to-...
Cosmological models can be constrained by determining primordial abundances. Accurate predictions of...
Photoelectron spectra of helium have been measured at different angles and at various energies above...