Nuclear charge radii from muonic X-ray transitions in F, Na, Al, Si, P, S and K

Schaller, L. A.; Dubler, T.; Kaeser, K.; Rinker, George A.; Robert-Tissot, B.; Schellenberg, L.; Schneuwly, H.

doi:10.1016/0375-9474(78)96128-6

Cited by 11 publications

(1 citation statement)

References 9 publications

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“…The limit of A = 30 was chosen because the programs were designed to include only the ld,,, and 2s1,, valence orbits. All stable even-even nuclei were calculated assuming that l60 is a closed shell and that the valence nucleons fill the Id,,,, 2s1/, and 1d3,, (dsd) orbits with occupation probabilities given by the wavefunctions calculated with Schaller et al(1978).…”

Section: Nuclei With a = 16-30mentioning

confidence: 99%

Proton and neutron density distributions for A=16-58 nuclei

Brown

Massen

Hodgson

1979

J. Phys. G: Nucl. Phys.

125

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A new method of calculating nuclear charge and matter distributions is described. It uses the sum of the squares of single-particle wavefunctions to give a first approximation and then iterates the proton and neutron densities in a formalism that takes into account the interaction between these densities and hetween the valence and core nacleons. The single-particle potentials are adjusted to give the experimental centroid separation energies, and configuration mixing is included using shell-model occupation probabilities. The method is applied to the core nuclei l6O and 40Ca, to their isotopes and to other nuclei in the sd and pf shells, Detailed comparisons are made with all available experimental data on nuclear charge and matter distributions.

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Section: Nuclei With a = 16-30mentioning

confidence: 99%