We discuss experimental data concerning Ca-48+Ca-48 and Ca-42+Fe-54 reactions at 25 MeV/nucleon obtained by using the 47 multi-detector Chimera. Effects due due to the different neutron to proton ratios (N/Z) of the two systems have been investigated. Charge distributions of forwardly emitted fragments show even-odd staggering whose amplitude is larger for the neutron poor system. Moreover, the neutron excess of the total system influence the evolution of fusion-like sources formed in semi-central collisions. In particular, for the neutron rich system, the relative emission yield of heavy residues is larger, while multi-fragmentation and binary-like events prevail in the neutron poor system.
We discuss experimental data concerning Ca-48+Ca-48 and Ca-42+Fe-54 reactions at 25 MeV/nucleon obtained by using the 47 multi-detector Chimera. Effects due due to the different neutron to proton ratios (N/Z) of the two systems have been investigated. Charge distributions of forwardly emitted fragments show even-odd staggering whose amplitude is larger for the neutron poor system. Moreover, the neutron excess of the total system influence the evolution of fusion-like sources formed in semi-central collisions. In particular, for the neutron rich system, the relative emission yield of heavy residues is larger, while multi-fragmentation and binary-like events prevail in the neutron poor system.
Entrance channel effects in medium mass nuclear systems at 25 MeV/nucleon
Geraci E;PAGANO, ANGELO;POLITI, Giuseppe;RIZZO, Francesca;
2014
Abstract
We discuss experimental data concerning Ca-48+Ca-48 and Ca-42+Fe-54 reactions at 25 MeV/nucleon obtained by using the 47 multi-detector Chimera. Effects due due to the different neutron to proton ratios (N/Z) of the two systems have been investigated. Charge distributions of forwardly emitted fragments show even-odd staggering whose amplitude is larger for the neutron poor system. Moreover, the neutron excess of the total system influence the evolution of fusion-like sources formed in semi-central collisions. In particular, for the neutron rich system, the relative emission yield of heavy residues is larger, while multi-fragmentation and binary-like events prevail in the neutron poor system.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
