Abstract
Background: Near- and sub-barrier fusion of various Ca + Zr isotopic combinations have been widely investigated. A recent analysis of data has highlighted the importance of couplings to multiphonon excitations and to both neutron and proton transfer channels. Analogous studies of tend to exclude any role of transfer couplings. However, the lowest measured cross section for this system is rather high (). A rather complete data set is available for , while no measurement of fusion has been performed in the past.
Purpose: Our aim is to measure the full excitation function of near the barrier and to extend downward the existing data on , in order to estimate the transfer couplings that should be used in coupled-channels calculations of the fusion of these two systems and of .
Methods: beams from the XTU Tandem accelerator of INFN–Laboratori Nazionali di Legnaro were used, bombarding thin metallic () and targets (same thickness) enriched to and in masses 90 and 92, respectively. An electrostatic beam deflector allowed the detection of fusion evaporation residues (ER) at very forward angles, and angular distributions of ER were measured.
Results: The excitation function of has been measured down to the level of . Coupled-channels (CC) calculations using a standard Woods-Saxon (WS) potential and following the line of a previous analysis of fusion data give a good account of the new data, as well as of the existing data for . The previous excitation function of has been extended down to .
Conclusions: Transfer couplings play an important role in explaining the fusion data for and . The strength of the pair-transfer coupling is deduced by applying a simple recipe based on the value obtained for . The logarithmic slopes and the factors for fusion are reproduced fairly well for all three systems by the CC calculations, and there are no indications of a fusion hindrance at the lowest energies. In contrast, the new data for indicate the onset of a fusion hindrance at the lowest energies.
- Received 7 April 2017
DOI:https://doi.org/10.1103/PhysRevC.96.014603
©2017 American Physical Society