Y Z Y A 0,10 0,08 0,06 0,04 0,02 0,00 0 0,10 10 20 Z 30 40 50 60 0,08 0,06 0,04 0,02 48Ca + 244Pu th. exp. 0,00 0 20 40 60 80 100 120 140 A 292114 7-2: The same as <strong>in</strong> Fig. 7-1for <strong>the</strong> hot fusi<strong>on</strong> reacti<strong>on</strong> Figure 48 + Ca 244 Pu→ 292 The 114. mass distributi<strong>on</strong> (open po<strong>in</strong>ts) is taken from <strong>the</strong> Ref. [11]. The excitati<strong>on</strong> energy experimental <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> <strong>in</strong>itial DNS is E ∗ =10MeV (upper and lower parts). 99
estimated from <strong>the</strong> difference between <strong>the</strong> bombard<strong>in</strong>g energy Ec.m. <strong>in</strong> <strong>the</strong> system <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> center <str<strong>on</strong>g>of</str<strong>on</strong>g> mass and <strong>the</strong> value <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> nucleus-nucleus potential for R corresp<strong>on</strong>d<strong>in</strong>g to <strong>the</strong> bottom <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> pocket for <strong>the</strong> <strong>in</strong>itial c<strong>on</strong>figurati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> DNS. The charge (mass) quasi-fissi<strong>on</strong> distributi<strong>on</strong>s slightly <strong>on</strong> <strong>the</strong> excitati<strong>on</strong> energy E depend ∗ <strong>the</strong> <strong>in</strong>itial DNS (Fig. 7-1). This is due to <strong>the</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> dependence <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> transport coefficients ∆ weak (±) <strong>the</strong> temperature [33]. With an <strong>in</strong>creas<strong>in</strong>g <strong>on</strong> temperature <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> system, <strong>the</strong> <strong>in</strong>fluence <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> shell effects <strong>on</strong> <strong>the</strong> process <str<strong>on</strong>g>of</str<strong>on</strong>g> nucle<strong>on</strong> transfer decreases more slowly than <strong>the</strong> exp<strong>on</strong>ential decrease <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> shell correcti<strong>on</strong> <strong>in</strong> <strong>the</strong> potential energy [33]. It was experimentally found [113] <strong>in</strong> <strong>the</strong> quasifissi<strong>on</strong> reacti<strong>on</strong>s 238 U+ 16 O, 26 Mg, 27 Al, 32 S, 35 Cl, 40,48 Ca and nat Zn at several bombard<strong>in</strong>g energies, that <strong>the</strong> mass asymmetry moti<strong>on</strong> is dom<strong>in</strong>ated by <strong>the</strong> <strong>on</strong>e-body dissipati<strong>on</strong> which is <strong>in</strong>dependent <str<strong>on</strong>g>of</str<strong>on</strong>g> temperature. The observed relaxati<strong>on</strong> times for <strong>the</strong> mass asymmetry mode <str<strong>on</strong>g>of</str<strong>on</strong>g> all <strong>the</strong> systems c<strong>on</strong>sidered were <strong>in</strong> agreement with <strong>the</strong> wall dissipati<strong>on</strong> picture [113]. Z Fig. 7-3 shows <strong>the</strong> quasi-fissi<strong>on</strong> charge and mass distributi<strong>on</strong>s for <strong>the</strong> cold fusi<strong>on</strong> reacti<strong>on</strong>s with <strong>the</strong> projectiles 50 Ti, 64 Ni and 76 Ge <strong>on</strong> <strong>the</strong> target 208 Pb, which lead to <strong>the</strong> syn<strong>the</strong>sis <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> elements 258 104, 272 110 and 284 114, respectively, with an excitati<strong>on</strong> energy about 11-16 MeV [7, 8]. The ratio between <strong>the</strong> drifts <str<strong>on</strong>g>of</str<strong>on</strong>g> mass and charge toward symmetric c<strong>on</strong>figurati<strong>on</strong>s <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> DNS and toward more asymmetric <strong>on</strong>es becomes c<strong>on</strong>siderably larger with <strong>the</strong> <strong>in</strong>crease <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> charge number <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> super<strong>heavy</strong> element. Due to this fact, <strong>the</strong> complete fusi<strong>on</strong> probability <strong>in</strong> <strong>the</strong> mass asymmetry degree <str<strong>on</strong>g>of</str<strong>on</strong>g> freedom decreases from <strong>the</strong> nucleus 258 104 to 272 110. For <strong>the</strong> reacti<strong>on</strong> 76 Ge+ 208 Pb→ 284 114, we found that <strong>the</strong> quasi-fissi<strong>on</strong> products are practically associated with fragmentati<strong>on</strong>s near <strong>the</strong> <strong>in</strong>itial DNS due to small values <str<strong>on</strong>g>of</str<strong>on</strong>g> quasi-fissi<strong>on</strong> barriers B qf. Compar<strong>in</strong>g Fig. 7-3 with Fig.7-2, we see that <strong>the</strong> mass and charge yields <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> quasi-fissi<strong>on</strong> products for nearly symmetric c<strong>on</strong>figurati<strong>on</strong>s <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> DNS are larger for <strong>the</strong> hot fusi<strong>on</strong> reacti<strong>on</strong> 48 Ca+ 244 Pu than for <strong>the</strong> cold fusi<strong>on</strong> reacti<strong>on</strong> 76 Ge+ 208 Pb. The quasi-fissi<strong>on</strong> barrier B qf <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> <strong>in</strong>itial DNS becomes larger with decreas<strong>in</strong>g Z, and <strong>the</strong> nucle<strong>on</strong> transfer plays a larger role <strong>in</strong> <strong>the</strong> evoluti<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> this DNS than <strong>the</strong> decay process. This is c<strong>on</strong>sistent with <strong>the</strong> c<strong>on</strong>clusi<strong>on</strong> that <strong>the</strong> hot fusi<strong>on</strong> reacti<strong>on</strong> 48 Ca+ 244 Pu→ 292 114 is preferable for <strong>the</strong> syn<strong>the</strong>sis <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> element 114, although <strong>the</strong> survival probability <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> compound nucleus decreases with <strong>in</strong>creas<strong>in</strong>g excitati<strong>on</strong> energy [20, 22]. In <strong>the</strong> cold fusi<strong>on</strong> reacti<strong>on</strong>s, <strong>the</strong> quasi-fissi<strong>on</strong> is an important factor decreas<strong>in</strong>g <strong>the</strong> complete fusi<strong>on</strong> cross secti<strong>on</strong>s with <strong>in</strong>creas<strong>in</strong>g atomic number <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>the</strong> super<strong>heavy</strong> element. Produc<strong>in</strong>g <strong>the</strong> 100
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Effects of
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1 Introduction 6 1.1 The DNS-concep
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Chapter 1 The elements existing in
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observed the rapid fall-of<
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Figure 1-1 illustrates the compound
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smaller than the extra-extra push e
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fusion and quasi-fission processes
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In the present chapter we have pres
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higher collective velocities to rep
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2.1 General considerations We want
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couplings. Diabatic basis states ψ
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Chapter 3 The synthesis of<
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is calculated within the TCSM using
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E adiab (MeV) n E diab (MeV) n 30 2
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E diab (MeV) n 60 55 50 45 40 100Mo
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3-5: Diabatic potentials for the sy
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3-7: The same as in Fig. 3-6 for th
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The estimated collective velocities
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3-10: Diabatic contributions as a f
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effects give a justification for th
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The similarity of
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4.1.3 Alternative microscopical met
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to the DNS concept [18, 34], cross
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