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Hot fusion

The hot fusion is a frequently used way to produce exotic nuclei. There are many experimental data concerning e.g. total and differential fusion cross-sections, spin distributions, multiplicites of particles emitted during fusion process or deep inelastic collision. These data should be compared with results of theoretical calculations.

The theoretical description of the heavy ion collisions at energies of the order of few hundreds MeV would be of great interest for studying the validity of the transport equation. At these energies the fused system will reach the temperature of 4-5 MeV and such a high temperature will influence:

$\rightarrow$ The heights of the fusion and fission barriers;

$\rightarrow$ The magnitude of the friction forces;

$\rightarrow$ The value of the diffusion and the mass tensors.

The change of the fusion barrier with temperature could be estimated within of the extended Thomas-Fermi (ETF) method applied to the Skyrme interaction. The ETF model predicts a significant decrease with temperature of the surface term in the liquid drop energy, while the Coulomb part is almost unchanged. The temperature dependence of the friction forces was extensively discussed within the linear response theory and other microscopic theories. All theoretical models predict an increase of the friction forces with temperature and saturation at higher temperatures. Also the commonly used Einstein relation between the diffusion and the friction forces should be tested in the wide range of temperatures. The last theoretical works suggest that the Einstein relation should be modified.

$\rightarrow$ Theoretical investigation of multifragmentation process.
A model of dynamical instabilities of finite, hot, expanding nuclear droplets is developed. The model accounts for small amplitudes density and surface isoscalar modes that become unstable for nuclear densities below 0.5-0.6 times the normal nuclear density. Adiabatic and diabatic evolution is considered. We plan to extend the model for isovector modes and include dissipation.


next up previous
Next: Decay of the compound Up: NUCLEAR COLLISIONS - RELATION Previous: Heavy ion collisions at

2000-04-17