Background:The fusion excitation function of the system 28 Si + 28 Si at energies near and below the Coulomb barrier is known only down to ≃15 mb. This precludes any information on both coupling effects on sub-barrier cross sections and the possible appearance of hindrance. For 28 Si + 30 Si even if the fusion cross section was measured down to ≃50µb, the evidence of hindrance is marginal. Both systems have positive fusion Q-values. While 28 Si has a deformed oblate shape, 30 Si is spherical.Purpose: Investigating: 1) the possible influence of the different structure of the two Si isotopes on the fusion excitation functions in the deep sub-barrier region; 2) whether hindrance exists in the Si+Si systems and whether it is strong enough to generate an S factor maximum, thus allowing a comparison with lighter heavy-ion systems of astrophysical interest.Methods: 28 Si beams from the XTU Tandem accelerator of INFN-Laboratori Nazionali di Legnaro were used. The set-up was based on an electrostatic beam separator, and fusion evaporation residues (ER) were detected at very forward angles. Angular distributions of ER were measured.Results: Fusion cross sections of 28 Si + 28 Si have been obtained down to ≃600 nb. The slope of the excitation function has a clear irregularity below the barrier but no indication of a S-factor maximum is found. For 28 Si + 30 Si the previous data have been confirmed and two smaller cross sections have been measured down to ≃4µb. The trend of the S-factor reinforces the previous weak evidence of hindrance.
Conclusions:The sub-barrier cross sections for 28 Si + 28 Si are overestimated by coupled-channels calculations based on a standard Woods-Saxon potential, except for the lowest energies. Calculations using the M3Y+repulsion potential are adjusted to fit the 28 Si + 28 Si and the existing 30 Si + 30 Si data. An additional weak imaginary potential (probably simulating the effect of the oblate 28 Si deformation) is required to fit the low-energy trend of 28 Si + 28 Si. The parameters of these calculations are applied to predict the ion-ion potential for 28 Si + 30 Si. Its cross sections are well reproduced by including also one-and successive two-neutron transfer channels, besides the low-lying surface excitations.