Production of new superheavy Z=108-114 nuclei with U, Pu and Cm targets
arXiv:0912.4069 · doi:10.1103/PhysRevC.80.057601
Abstract
Within the framework of the dinuclear system (DNS) model, production cross sections of new superheavy nuclei with charged numbers Z=108-114 are analyzed systematically. Possible combinations based on the actinide nuclides U, Pu and Cm with the optimal excitation energies and evaporation channels are pointed out to synthesize new isotopes which lie between the nuclides produced in the cold fusion and the Ca induced fusion reactions experimentally, which are feasible to be constructed experimentally. It is found that the production cross sections of superheavy nuclei decrease drastically with the charged numbers of compound nuclei. Larger mass asymmetries of the entrance channels enhance the cross sections in 2n-5n channels.
5 pages, 4 figures
References in corpus (4)
Cited by in corpus (13)
- Production of neutron-rich isotopes around N=126 in multinucleon transfer reactions
- Production of heavy isotopes in transfer reactions by collisions of U+U
- Microscopic studies of production cross sections in multinucleon transfer reaction Ni+Sn
- Isotopic trends of quasifission and fusion-fission in the reactions Ca+Pu
- Systematics on production of superheavy nuclei in fusion-evaporation reactions
- To reach neutron-rich heavy and superheavy nuclei by multinucleon transfer reactions with radioactive isotopes
- Influence of entrance channels on formation of superheavy nuclei in massive fusion reactions
- Production of proton-rich nuclei around Z=84-90 in fusion-evaporation reactions
- Multinucleon transfer dynamics in heavy-ion collisions near Coulomb barrier energies
- Production mechanism of neutron-deficient actinide isotopes in complete fusion reactions and multinucleon transfer reactions
- Dynamics of light nuclei produced in the massive transfer reactions
- Production of neutron-rich heavy nuclei around N = 162 in multinucleon transfer reactions
- Potential energy surface and formation of superheavy nuclei with the Skyrme energy-density functional