Variational procedure for nuclear shell-model calculations and energy-variance extrapolation
arXiv:1204.2626 · doi:10.1103/PhysRevC.85.054301
Abstract
We discuss a variational calculation for nuclear shell-model calculations and propose a new procedure for the energy-variance extrapolation (EVE) method using a sequence of the approximated wave functions obtained by the variational calculation. The wave functions are described as linear combinations of the parity, angular-momentum projected Slater determinants, the energy of which is minimized by the conjugate gradient method obeying the variational principle. The EVE generally works well using the wave functions, but we found some difficult cases where the EVE gives a poor estimation. We discuss the origin of the poor estimation concerning shape coexistence. We found that the appropriate reordering of the Slater determinants allows us to overcome this difficulty and to reduce the uncertainty of the extrapolation.
6 pages, 5 figures, submitted to Physical Review C
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- Large-scale shell-model calculations for unnatural-parity high-spin states in neutron-rich Cr and Fe isotopes
- Recent progress in configuration-interaction shell model
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- Effect of residual many-body forces due to the evolution in the in-medium similarity renormalization group method
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