Fusion cross sections for nucleonic-halo systems in solar systems

The behavior of total fusion cross sections for proton and neutron-halo systems at near and sub-barrier energies have been studied using coupled-channel calculations. We have done the fusion distribution by considering phonon excitations and rotational deformation. Comparing with available experimental data represents a good agreement for neutron halo systems. A comparison between the reduced fusion cross sections of these systems shows different behavior in sub-barrier energies.