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nuclear physics in poland 1996 – 2006

nuclear physics in poland 1996 – 2006

nuclear physics in poland 1996 – 2006

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GLOBAL PROPERTIES OF NUCLEIA.Baran 1 , Z.Łojewski 2 , B.Nerlo-Pomorska 1 , K.Pomorski 1 , M.Warda 11 Institute of Physics, Maria Curie-Skłodowska University, Lubl<strong>in</strong>2 Institute of Informatics, Maria Curie-Skłodowska University, Lubl<strong>in</strong>The potential energy of β-stable nuclei wascalculated with<strong>in</strong> Hartree-Fock procedure withthe Relativistic Mean Field Theory (RMFT+NL3) ,the Gogny force (D1S), Skyrme <strong>in</strong>teraction andmacroscopic-microscopic method with theWoods-Saxon and Nilsson s<strong>in</strong>gle particlepotentials [1].The proton and neutron radii were calculatedand their isosp<strong>in</strong> dependence analysed for exoticnuclei us<strong>in</strong>g RMFT [2,3], D1S [4] and macroscopicmicroscopicmethod with Woods-Saxon potential[5]. The radii of K isomers [6] and neutron halo <strong>in</strong>heavy nuclei with D1S force were also calculated[7].In Fig. 1 the shell corrections are presented,extracted from the s<strong>in</strong>gle particle levels of selfconsistentmean fields of Gogny D1S [8,9,10,11]and RMFT+NL3 [12,13,14] by the Strut<strong>in</strong>skymethod smooth<strong>in</strong>g the energy <strong>in</strong> the energy space(NL3, D1S) or <strong>in</strong> nucleon number space (NL3N,D1SN). The smooth part of potential energy wascompared to various liquid drop models [15,16].The shell and pair<strong>in</strong>g energies were obta<strong>in</strong>ed byfold<strong>in</strong>g <strong>in</strong> nucleon number space [17,18]. Theaverage pair<strong>in</strong>g energy is also analysed with<strong>in</strong> n-fold<strong>in</strong>g [19] giv<strong>in</strong>g double value for scission po<strong>in</strong>t<strong>in</strong> fission isomers.The new way of evaluat<strong>in</strong>g the shellcorrections [21] by fold<strong>in</strong>g <strong>in</strong> nucleon numberspace conserves the particle number exactly andgives similar results as the traditional Strut<strong>in</strong>skyfold<strong>in</strong>g <strong>in</strong> s<strong>in</strong>gle particle energy space for largedeformed nuclei, while for spherical isotopes thenew shell corrections become deeper. This effect isconnected with the zero po<strong>in</strong>t vibrations, whichshould be taken <strong>in</strong>to account [22], but wereneglected previously ( Nucl. Phys. A95, 420(1967)). The whole macroscopic-microscopicmethod should be modified by the newmacroscopic – Lubl<strong>in</strong> Strasbourg Drop [23] part,Yukawa folded mean field, new shell corrections[21] and the n-folded average pair<strong>in</strong>g [18] term.All the parameters should be fitted to the actuallyavailable data. Then the macroscopic-microscopicmethod can compete with selfconsistent models,which are much more calculation timeconsum<strong>in</strong>g.Fig. 1. The shell corrections of neutrons (left) and protons (right) forisotopes (upper panels), isotones (middle panels) and β-stable nuclei(lowest panel).43

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