Peninsulas of the neutron stability of nuclei in the vicinity of neutron magic numbers |
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| Authors: | V. N. Tarasov K. A. Gridnev W. Greiner D. K. Gridnev V. I. Kuprikov D. V. Tarasov X. Viñas |
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| Affiliation: | 1.National Science Center,Kharkov Institute of Physics and Technology,Kharkov,Ukraine;2.Fock Institute of Physics,St. Petersburg State University,Petrodvorets, St. Petersburg,Russia;3.Institut für Theoretische Physik,Johann Wolfgang Goethe-Universit?t,Frankfurt am Main,Germany;4.Universitat de Barcelona,Barcelona,Spain |
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| Abstract: | On the basis of the Hartree-Fock method as implemented with Skyrme forces (Ska, SkM*, Sly4, and SkI2) and with allowance for an axial deformation and nucleon pairing in the Bardeen-Cooper-Schrieffer approximation, the properties of extremely neutron-rich even-even nuclei were calculated beyond the neutron drip line known earlier from theoretical calculations. It was shown that the chains of isotopes beyond the neutron drip line that contain N = 32, 58, 82, 126, and 184 neutrons form peninsulas of nuclei stable against the emission of one neutron and, in some cases, peninsulas of nuclei stable against the emission of two neutrons. The neutron- and proton-density distributions in nuclei forming stability peninsulas were found to be spherically symmetric. A mechanism via which the stability of nuclei might be restored beyond the neutron drip line was discussed. A comparison with the results of calculations by the Hartree-Fock-Bogolyubov method was performed for long chains of sulfur and gadolinium isotopes up to the neutron drip line. |
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