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

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4-1: Fusi<strong>on</strong> barriers B Table TCSM<br />

η<br />

are compared with <strong>the</strong> experimental<br />

surplus <str<strong>on</strong>g>of</str<strong>on</strong>g> energy ∆B exp above <strong>the</strong> Bass barrier.<br />

B Reacti<strong>on</strong>s TCSM(MeV<br />

) ∆B η exp (MeV)<br />

Zr + 90 Zr→180 Hg 4 0.0<br />

+0.5<br />

90<br />

−0.5<br />

Zr+<br />

96<br />

Zr→192 Hg 6 4.2<br />

+1.2<br />

96<br />

−1.2<br />

90 + 100<br />

Mo→190 Pb 5 5.1<br />

+1.0<br />

−1.0<br />

Zr<br />

96 + 100<br />

Mo→196 Pb 7 9.5<br />

+1.0<br />

−1.0<br />

Zr<br />

Mo+<br />

100<br />

Mo→194 Po1 0<br />

94<br />

6.3<br />

+1.0<br />

−1.0 1<br />

Mo+<br />

100<br />

Mo→200 100<br />

7 Po 2.2<br />

+0.5<br />

−0.5 1<br />

90 + 124<br />

Sn→214 Th 11 20.3<br />

+4.0<br />

−4.0<br />

Zr<br />

Zr + 124<br />

Sn→220 Th1 7 26.7<br />

+5.0<br />

96<br />

−3.0<br />

128 Sn+ 126 Sn → 254 Fm 22 -<br />

132 Sn + 132 Sn → 264 Fm 30 -<br />

4.2.2 Comparis<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> driv<strong>in</strong>g potentials calculated with different methods<br />

Figs. 4-6 a) and 4-7 a) show <strong>the</strong> driv<strong>in</strong>g potential calculated with <strong>the</strong> TCSM-method, with <strong>the</strong><br />

phenomenological method and with <strong>the</strong> alternative microscopical method for <strong>the</strong> systems 180 Hg<br />

and 246 Fm, which are produced <strong>in</strong> <strong>the</strong> reacti<strong>on</strong>s 90 Zr + 90 Zr and 76 Ge + 170 Er, respectively.<br />

Here, <strong>the</strong> <strong>nuclei</strong> form<strong>in</strong>g <strong>the</strong> DNS are c<strong>on</strong>sidered as spherical and <strong>the</strong> driv<strong>in</strong>g potential calculated<br />

with <strong>the</strong> alternative microscopical method is shown for a temperature T =1MeV. The driv<strong>in</strong>g<br />

potentials are given as a functi<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> charge Z <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> light nucleus <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> DNS. We can<br />

observe that <strong>the</strong> driv<strong>in</strong>g potential calculated with <strong>the</strong> TCSM-method is qualitatively similar to<br />

<strong>the</strong> driv<strong>in</strong>g potentials calculated with <strong>the</strong> phenomenological and <strong>the</strong> alternative microscopical<br />

methods.<br />

The phenomenological driv<strong>in</strong>g potential, where <strong>the</strong> shell effects are taken <strong>in</strong>to account <strong>on</strong>ly<br />

through <strong>the</strong> asymptotic b<strong>in</strong>d<strong>in</strong>g energies, reveals more structures [73] than <strong>the</strong> <strong>on</strong>es calculated<br />

with <strong>the</strong> TCSM-method or with <strong>the</strong> alternative microscopical method. Experiments ([28]-[32])<br />

c<strong>on</strong>firm <strong>the</strong> assumpti<strong>on</strong> that dur<strong>in</strong>g <strong>the</strong> collisi<strong>on</strong>, <strong>the</strong> <strong>in</strong>dividual properties <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> collid<strong>in</strong>g <strong>nuclei</strong><br />

are c<strong>on</strong>served and <strong>the</strong> shell effects play an essential role. For <strong>in</strong>stance, <strong>the</strong>re are local maxima<br />

corresp<strong>on</strong>d<strong>in</strong>g to <strong>the</strong> closed-shell <strong>nuclei</strong> [28] <strong>in</strong> <strong>the</strong> charge and mass distributi<strong>on</strong>s <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> reacti<strong>on</strong><br />

52

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