This WEB document provides supplementary contents for a paper:
``Study of Superdeformation in Non-rotating States
using the Skyrme-Hartree-Fock Method
''
Satoshi Takahara, Naoki Tajima and Naoki Onishi,
submitted to Nuclear Physics A.

Comparison with the results of the Nilsson-Strutinsky method

The Nilsson-Strutinsky(NS) method is a convenient and well-established method to treat nuclear deformations. Because NS computation is much simpler than self-consistent-field calculations, it seems worth doing another systematic survey of SD isomers using the NS method in order to compare the results with those of the Skyrme-HF method for the same nuclei. Our survey using NS method provides a useful overview of the situation outside the region investigated in section 4 of our paper [TTO98].

We have utilized a program for the standard Nilsson-Strutinsky calculation [NTS69] provided by Y.R. Shimizu [Shi97], which takes into account two axially symmetric deformations, i.e., the quadrupole deformation epsilon_2 and the hexadecapole deformation epsilon_4. For each value of epsilon_2, the value of epsilon_4 is optimized so as to minimize the total energy. The standard values given in Table 1 of Ref. [BR85] are used for the parameters kappa_N and mu_N of the Nilsson potential. The pairing correlation is active for single-particle levels within +/- 1.2 hbar omega from the Fermi level, while the strengths of the pairing force are determined such that the smoothed pairing gap becomes

bar{Delta} = 13 A^{-1/2} MeV.

The parameters of the macroscopic part [MS67] are

a_s=17.9439 MeV,
kappa_s=1.7826,
R_c=1.2249 A^{1/3} fm.

See Ref. [BRA91] for calculational details.

With this model one can calculate the entire region of the nuclear chart, i.e., from the proton drip line to the neutron drip line: The model does not suffer from the problem of neutron pairing in neutron-rich nuclei explained in section 4 of our paper [TTO98] because the Nilsson potential does not have a continuum spectrum. Concerning the expected enhancement of the pairing due to the coupling with the continuum states, however, the present model simply neglects its influences.

The calculation for 2000 even-even nuclei can be completed in a few hours with an ordinary personal computer owing to the simpleness of the NS method itself and also to the specialization of the code to non-rotating axially symmetric states.

Fig. 1 in formats of JPEG(143KB) or GIF(497KB) or PS(1.2MB) displays the resulting deformations epsilon_2, excitation energies E^*, and barrier heights E_B of the SD minima at epsilon_2 > 0.35. Let us discuss the results according to the grouping employed in section 4 of our paper [TTO98].

References

[TTO98]
Satoshi Takahara, Naoki Tajima and Naoki Onishi, submitted to Nuclear Physics A.
[NTS69]
S.G. Nilsson, C.F. Tsang, A. Sobiczewski, Z. Szymanski, S. Wycech, C. Gustafson, I. Lamm, P. Moeller and B. Nilsson, Nucl.Phys. A131 (1969) 1.
[Shi97]
Y.R. Shimizu, private communication.
[BR85]
T. Bengtsson and I. Ragnarsson, Nucl. Phys. A436 (1985) 14.
[MS67]
W.D. Myers and W.J. Swiatecki, Ark. Phys. 36 (1967) 343.
[BRA91]
T. Bengtsson, I. Ragnarsson and S. Aberg, in ``Computational Nuclear Physics 1'', ed. K. Langanke, J.A. Maruhn and S.E. Koonin, (Springer-Verlag, Berlin, 1991) 51.


Last modified on July 10, 1998
Mail to: < S. Takahara > or < N. Tajima >

Return to: Takahara, Tajima,