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E. Chabanat, P. Bonche, P. Haensel, J. Meyer and R. Schaeffer, “A Skyrme Parametrization from Subnuclear to Neutron Star Densities Part Ⅱ. Nuclei Far from Stabilities,” Nuclear Physics A, Vol. 635, No. 1-2, 1998, pp. 231-256. doi:10.1016/S0375-9474(98)00180-8

has been cited by the following article:

• TITLE: Influence of Tensor Interaction on Evolution of Nuclear Shells

  AUTHORS: Rupayan Bhattacharya

  KEYWORDS: Tensor Interaction; Hartree-Fock Theory; Nuclear Shells

  JOURNAL NAME: Journal of Modern Physics, Vol.4 No.5B, July 10, 2013

  ABSTRACT: Using Skyrme’s density dependent interaction the evolution of nuclear shells has been studied in Hartree-Fock formalism. Optimization of the strength of tensor interaction has been done in reproducing the observed splitting of shell model states of 40,48Ca, 56Ni and 208Pb. Spin-orbit splitting in Ca-isotopes, 56Ni, 90Zr, N = 82 isotones, Sn-isotopes and evolution of gaps in Z, N=8, 20 have been reanalyzed with the inclusion of tensor interaction. For doubly shell closed nuclei it has been observed that tensor interaction is sensitive to spin saturation of nuclear shells.