dorsal/arxiv
View SchemaReduction of the spin-orbit potential in light drip-line nuclei
| Authors | G. A. Lalazissis, D. Vretenar, W. Poeschl, P. Ring |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9709020 |
| URL | https://arxiv.org/abs/nucl-th/9709020 |
| DOI | 10.1016/S0370-2693(97)01473-1 |
| Journal | Phys.Lett. B418 (1998) 7-12 |
Abstract
The isospin dependence of the spin-orbit interaction in light neutron rich nuclei is investigated in the framework of relativistic mean field theory. The magnitude of the spin-orbit potential is considerably reduced in drip line nuclei, resulting in smaller energy splittings between spin-orbit partners. The effect does not depend on the parametrization of the effective Lagrangian. The results are compared with corresponding calculations in the non-relativistic Skyrme model.
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"abstract": "The isospin dependence of the spin-orbit interaction in light neutron rich\nnuclei is investigated in the framework of relativistic mean field theory. The\nmagnitude of the spin-orbit potential is considerably reduced in drip line\nnuclei, resulting in smaller energy splittings between spin-orbit partners. The\neffect does not depend on the parametrization of the effective Lagrangian. The\nresults are compared with corresponding calculations in the non-relativistic\nSkyrme model.",
"arxiv_id": "nucl-th/9709020",
"authors": [
"G. A. Lalazissis",
"D. Vretenar",
"W. Poeschl",
"P. Ring"
],
"categories": [
"nucl-th"
],
"doi": "10.1016/S0370-2693(97)01473-1",
"journal_ref": "Phys.Lett. B418 (1998) 7-12",
"title": "Reduction of the spin-orbit potential in light drip-line nuclei",
"url": "https://arxiv.org/abs/nucl-th/9709020"
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