Abstract
Absolute cross sections for isotopically identified products formed in multinucleon transfer in the system at are reported. The isotopic distributions obtained using a large acceptance spectrometer demonstrated the production of the “hard-to-reach” neutron-rich isotopes for around the shell closure far from stability. The main contribution to the formation of these exotic nuclei is shown to arise in collisions with a small kinetic energy dissipation. The present experimental finding corroborates for the first time recent predictions that multinucleon transfer reactions would be the optimum method to populate and characterize neutron-rich isotopes around which are crucial for understanding both astrophysically relevant processes and the evolution of “magic” numbers far from stability.
- Received 26 June 2015
DOI:https://doi.org/10.1103/PhysRevLett.115.172503
© 2015 American Physical Society