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Phys. Rev. C 68, 054312 (2003) [11 pages]

Systematic study of deformed nuclei at the drip lines and beyond

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M. V. Stoitsov1,2,3,4, J. Dobaczewski5, W. Nazarewicz3,4,5, S. Pittel6, and D. J. Dean3,4
1Institute of Nuclear Research and Nuclear Energy, Bulgarian Academy of Sciences, Sofia-1784, Bulgaria
2Joint Institute for Heavy Ion Research, Oak Ridge, Tennessee 37831, USA
3Department of Physics and Astronomy, The University of Tennessee, Knoxville, Tennessee 37996, USA
4Physics Division, Oak Ridge National Laboratory, P.O. Box 2008, Oak Ridge, Tennessee 37831 USA
5Institute of Theoretical Physics, Warsaw University, Hoża 69, PL-00-681 Warsaw, Poland
6Bartol Research Institute, University of Delaware, Newark, Delaware 19716, USA

Received 11 July 2003; published 21 November 2003

An improved prescription for choosing a transformed harmonic-oscillator (THO) basis for use in configuration-space Hartree-Fock-Bogoliubov (HFB) calculations is presented. The new HFB+THO framework that follows accurately reproduces the results of coordinate-space HFB calculations for spherical nuclei, including those that are weakly bound. Furthermore, it is fully automated, facilitating its use in systematic investigations of large sets of nuclei throughout the periodic table. As a first application, we have carried out calculations using the Skyrme force SLy4 and volume pairing, with exact particle-number projection following application of the Lipkin-Nogami prescription. Calculations were performed for all even-even nuclei from the proton drip line to the neutron drip line having proton numbers Z=2,4,…,108 and neutron numbers N=2,4,…,188. We focus on nuclei near the neutron drip line and find that there exist numerous particle-bound even-even nuclei (i.e., nuclei with negative Fermi energies) that have at the same time negative two-neutron separation energies. This phenomenon, which was earlier noted for light nuclei, is attributed to bound shape isomers beyond the drip line.

© 2003 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.68.054312
DOI:
10.1103/PhysRevC.68.054312
PACS:
21.60.Jz, 21.10.Dr, 21.10.Ky