[Submitted on 8 Nov 2024]
Configuration interaction relativistic Hartree-Fock model
Jia Liu · Yi Fei Niu · Wen Hui Long
The configuration interaction relativistic Hartree-Fock (CI-RHF) model is developed in this work. Compared to the conventional configuration interaction shell model (CISM), the CI-RHF model can be applied to study the structural properties of a wide range of nuclei without readjusting any parameters, as the effective Hamiltonian for different model space can be deduced consistently from a universal density-dependent Lagrangian based on the Hartree-Fock single-particle basis. The convergence of intermediate-state excitations has been examined in evaluating the effective interactions, and the core-polarization effects are illustrated, by using O as an example. Employing the CI-RHF model, both the bulk properties and low-lying spectra of even-even nuclei Ne have been well reproduced with the model space restricted to the shell. Studies of the isotopic evolution concerning charge radii and low-lying spectra highlight the shell closure at for neon isotopes. Furthermore, the cross-shell calculations extending from the to shell successfully reproduced the low-lying spectra of Ne and Ne. Notably, remarkably low excitation energies of Ne suggest the disappearance of the conventional magicity .
- Comments:
- 6 figures
- Subjects:
- Nuclear Theory (nucl-th)
- arXiv:
- 2411.05370 [pdf]