Fusion hindrance and roles of shell effects in superheavy mass region
arXiv:nucl-th/0609049 · doi:10.1016/j.nuclphysa.2006.09.018
Abstract
We present the first attempt of systematically investigating the effects of shell correction energy for a dynamical process, which includes fusion, fusion-fission and quasi-fission processes. In the superheavy mass region, for the fusion process, shell correction energy plays a very important role and enhances the fusion probability when the colliding partner has a strong shell structure. By analyzing the trajectory in three-dimensional coordinate space with the Langevin equation, we reveal the mechanism of the enhancement of the fusion probability caused by `cold fusion valleys'. The temperature dependence of shell correction energy is considered.
arXiv comment31 pages, 23 figures, Accepted for publication in Nuclear Physics A
References in corpus (6)
- Transport coefficients for shape degrees in terms of Cassini ovaloids
- Variation of transport coefficients for average fission dynamics with temperature and shape
- Microscopic Enhancement of Heavy-Element Production
- Trajectory analysis for fusion path in superheavy-mass region
- Analysis of fusion-fission dynamics by pre-scission neutron emission in Ni+Pb
- Origin of the drastic decrease of fusion probability in superheavy mass region
Cited by in corpus (9)
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- Effects of Nuclear Structure on Quasi-fission
- A dynamical model of surrogate reactions
- Spin-dependent observables in surrogate reactions
- Effects of neck and nuclear orientations on the mass drift in heavy ion collisions
- Modeling of nuclear reactions with Langevin calculations