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Giant halo and anti-halo in the non-relativistic mean field approach

Authors :
N. Van Giai
M. Grasso
Satoshi Yoshida
N. Sandulescu
Institut de Physique Nucléaire d'Orsay (IPNO)
Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Istituto Nazionale di Fisica Nucleare, Sezione di Catania (INFN)
Università degli studi di Catania [Catania]
Horia Hulubei National Institute of Physics and Nuclear Engineering (NIPNE)
IFIN-HH
Peter von Neumann-Cosel, Thomas Aumann
Source :
Nuclear Physics A, 2nd International Conference on Collective Motion in Nuclei under Extreme Conditions-COMEX 2, 2nd International Conference on Collective Motion in Nuclei under Extreme Conditions-COMEX 2, Jun 2006, Sankt Goar, Germany. pp.337-342, ⟨10.1016/j.nuclphysa.2007.01.063⟩
Publication Year :
2007
Publisher :
Elsevier BV, 2007.

Abstract

International audience; Giant neutron halos are studied in the framework of the Skyrme-Hartree-Fock-Bogoliubov approach. The appearance of such structures depends sensitively on the effective interaction adopted. This is illustrated by comparing the predictions of SLy4 and SkI4 in the Zr isotopic chain. The latter force predicts a neutron halo in the Zr chain with A > 122 due to weakly bound p orbitals. The structure of the halo is analyzed and the anti-halo effect due to pairing is discussed.

Details

ISSN :
03759474
Volume :
788
Database :
OpenAIRE
Journal :
Nuclear Physics A
Accession number :
edsair.doi.dedup.....391e6e59a910865e0fa031aa6bf3d1fe
Full Text :
https://doi.org/10.1016/j.nuclphysa.2007.01.063