Events in our system are self-managed.  Group and event managers are encouraged to review privacy and security settings, and adjust them if needed.  If you need assistance please contact Indico Support - contact Help at bottom of page. https://learn.getindico.io/categories/managing/

10–15 Jul 2016
St. Mary's University
US/Pacific timezone

Neutron orbits near doubly-magic $^{78}$Ni and $^{132}$Sn from reactions with radioactive beams (Invited)

15 Jul 2016, 09:00
25m
Scotiabank Theatre (St. Mary's University)

Scotiabank Theatre

St. Mary's University

923 Robie Street Halifax Nova Scotia
Invited

Speaker

Dr Riccardo Orlandi (Japan Atomic Energy Agency, Advanced Science Research Center)

Description

Transfer reactions are a valuable tool to study the evolution of shell structure away from stability. In particular, studies of nuclei in the proximity of exotic doubly-magic nuclei like $^{78}$Ni and $^{132}$Sn are key systems to test our theoretical understanding, since the proximity of the doubly-magic core makes shell-model calculations feasible. Single-neutron states in the Z=30, N=49 isotope $^{79}$Zn have been populated using the $^{78}$Zn(d,p)$^{79}$Zn transfer reaction in inverse kinematics at REX-ISOLDE, CERN. The experimental setup allowed the combined detection of protons ejected in the reaction, and of γrays emitted by $^{79}$Zn. From the combined analysis of γ-ray and proton data, low-lying states in $^{79}$Zn were observed and identified. Comparison with large-scale shell-model calculations permits to constrain the size of the N=50 shell gap in $^{78}$Ni. Neutron-hole states in $^{131}$Sn were populated using the $^{132}$Sn(d,t)$^{131}$Sn reaction at the HFRIB facility at Oak Ridge National Laboratory. Measured proton differential cross sections and their impact of single-hole energies in $^{132}$Sn will also be presented.

Primary author

Dr Riccardo Orlandi (Japan Atomic Energy Agency, Advanced Science Research Center)

Presentation materials

There are no materials yet.