Probing fusion by using an isotopic chain of neutron-rich oxygen isotopes to bombard a carbon target

The recent observation of heavy element nucleosynthesis in the merging of two neutron stars, underscores the importance of better understanding the fusion of neutron-rich nuclei. While the fusion of stable nuclei has been well studied for several decades, only recently have radioactive beam facilities made it possible to systematically investigate fusion for an isotopic chain of nuclei. Investigating the fusion of neutron-rich nuclei with an extended neutron density distribution can reveal whether fusion dynamics for neutron-rich nuclei differs significantly from that of beta stable nuclei. It also allows one to explore the influence of pairing at low density. To address this question the fusion excitation functions for ^16,17,18O + ¹²C will be compared to that of ¹⁹O + ¹²C. The experimental results will be compared to both simple barrier penetration models as well as the predictions of coupled channels calculations (CCFULL) and a density constrained time-dependent Hartree-Fock model (DC-TDHF). The systematic behavior of the above-barrier cross-section with increasing neutron number will be emphasized.