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Effects of diabaticity on fusion of heavy nuclei in the dinuclear model ...

Effects of diabaticity on fusion of heavy nuclei in the dinuclear model ...

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fusi<strong>on</strong> and quasi-fissi<strong>on</strong> processes after <strong>the</strong> capture stage <strong>in</strong> <strong>the</strong> DNS. In <strong>the</strong>se reacti<strong>on</strong>s <strong>the</strong><br />

quasi-fissi<strong>on</strong> channel dom<strong>in</strong>ates and leads to a str<strong>on</strong>g reducti<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> magnitude <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> fusi<strong>on</strong><br />

cross-secti<strong>on</strong>. The surviv<strong>in</strong>g probability Wsur estimates <strong>the</strong> competiti<strong>on</strong> between fissi<strong>on</strong> and<br />

neutr<strong>on</strong> evaporati<strong>on</strong> <strong>in</strong> <strong>the</strong> excited compound nucleus and may be calculated accord<strong>in</strong>g to <strong>the</strong><br />

statistical <strong>model</strong> [39] <strong>on</strong> <strong>the</strong> basis <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> M<strong>on</strong>te Carlo method.<br />

1.2 Goals <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> present work<br />

The basic microscopical <strong>model</strong> for <strong>the</strong> d<strong>in</strong>uclear system is <strong>the</strong> two-center shell <strong>model</strong> (TCSM)<br />

[40] (see Appendix). The usual parametrisati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> two-center potential c<strong>on</strong>sists <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong><br />

relative distance between <strong>the</strong> centers (or el<strong>on</strong>gati<strong>on</strong>), <strong>the</strong> mass (charge) asymmetry η =(A1 −<br />

A2)/(A1 + A2), <strong>the</strong> deformati<strong>on</strong>s <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> fragments β i and <strong>the</strong> neck coord<strong>in</strong>ate ε. The el<strong>on</strong>gati<strong>on</strong><br />

λ = l/(2R0) measures <strong>the</strong> length l <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> system <strong>in</strong> units <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> diameter 2R0 <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> spherical<br />

compound nucleus. This variable can be used to describe <strong>the</strong> relative moti<strong>on</strong>. The mass ratio<br />

between <strong>the</strong> fragments and <strong>the</strong> transiti<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> nucle<strong>on</strong>s through <strong>the</strong> neck are described by <strong>the</strong><br />

mass asymmetry η. The neck parameter ε = E0/E ′ is def<strong>in</strong>ed by <strong>the</strong> ratio <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> actual barrier<br />

height E0 to <strong>the</strong> barrier height E ′ <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> two-center oscillator. The deformati<strong>on</strong>s β i = a i/b i<br />

<str<strong>on</strong>g>of</str<strong>on</strong>g> axial symmetric fragments are def<strong>in</strong>ed by <strong>the</strong> ratio <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong>ir semiaxes. The neck grows with<br />

decreas<strong>in</strong>g ε (Fig.1-3). The potential energy surface (PES) <strong>in</strong> <strong>the</strong>se coord<strong>in</strong>ates is generally<br />

calculated with <strong>the</strong> Strut<strong>in</strong>sky method [41]. This is an adiabatic approach s<strong>in</strong>ce <strong>the</strong> nucle<strong>on</strong>s<br />

occupy <strong>the</strong> s<strong>in</strong>gle particle states up to <strong>the</strong> Fermi level <strong>in</strong> calculat<strong>in</strong>g <strong>the</strong> shell correcti<strong>on</strong>s.<br />

The adiabatic potential energy surfaces calculated as functi<strong>on</strong>s <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> el<strong>on</strong>gati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong><br />

DNS and <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> neck parameter were used to study classical trajectories for various <strong>heavy</strong> i<strong>on</strong><br />

reacti<strong>on</strong>s by us<strong>in</strong>g dissipative forces and mass parameters obta<strong>in</strong>ed with <strong>the</strong> Werner-Wheeler<br />

aproximati<strong>on</strong> [42]. The fusi<strong>on</strong> probabilities <strong>in</strong> <strong>the</strong> adiabatic TCSM are much larger than those<br />

obta<strong>in</strong>ed from experimental data and show an <strong>in</strong>correct isotopic dependence.<br />

The reacti<strong>on</strong>s c<strong>on</strong>sidered were for example <strong>the</strong> symmetric <strong>on</strong>es 90 Zr+ 90 Zr, 100 Mo+ 100 Mo,<br />

110 Pd+ 110 Pd, 124 Sn+ 124 Sn and 136 Xe+ 136 Xe and asymmetric <strong>on</strong>es. Therefore, it is c<strong>on</strong>cluded<br />

that a h<strong>in</strong>drance exists which prohibits <strong>the</strong> fast growth <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> neck and <strong>the</strong> moti<strong>on</strong> to smaller<br />

el<strong>on</strong>gati<strong>on</strong>s and allows <strong>the</strong> DNS to survive a time comparable with <strong>the</strong> reacti<strong>on</strong> time.<br />

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