The 17O+58Ni collision was studied by means of a detailed analysis of the experimental spectra based on Monte Carlo simulations. The elastic scattering angular distributions were measured at five near-barrier energies in the range of 40–50 MeV and were investigated within the framework of the Optical Model, observing a relation between the imaginary radius parameter and the target mass. The Optical Model potential trend shows a normal Threshold Anomaly whereas the total reaction cross section, compared to the 16O+58Ni case, is in agreement with the theoretical predictions.
Discrimination of Processes and Optical Model Analysis in the 17O+58Ni Collision Around the Coulomb Barrier
STRANO, EMANUELE;TORRESI, DOMENICO MARIO;MAZZOCCO, MARCO;LA COMMARA, MARCO;MOLINI, PIETRO BENEDETTO;PARASCANDOLO, CONCETTA;SIGNORINI, COSIMO;SORAMEL, FRANCESCA;GHEORGHE, ADONIA;GLODARIU, TUDOR;VITTURI, ANDREA;
2017
Abstract
The 17O+58Ni collision was studied by means of a detailed analysis of the experimental spectra based on Monte Carlo simulations. The elastic scattering angular distributions were measured at five near-barrier energies in the range of 40–50 MeV and were investigated within the framework of the Optical Model, observing a relation between the imaginary radius parameter and the target mass. The Optical Model potential trend shows a normal Threshold Anomaly whereas the total reaction cross section, compared to the 16O+58Ni case, is in agreement with the theoretical predictions.
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