NUSPIN 2016 Workshop of the Nuclear Spectroscopy Instrumentation Network and AGATA Physics Workshop

Session

Physics of neutron-rich nuclei

27 Jun 2016, 14:00

San Servolo, Venice

Conveners

Physics of neutron-rich nuclei

• Giacomo De Angelis (LNL)

54. Welcome

Prof. Silvia M. Lenzi (PD)

27/06/2016, 14:00

13. The Inversion Archipelago at The Neutron Rich Shores

Prof. Alfredo Poves (Universidad Autonoma de Madrid)

27/06/2016, 14:20

I will discuss the physical origin of the Islands if Inversion/Deformation which occur at different neutron magic numbers for very neutron rich isotopes and its connection with shape coexistence in doubly magic nuclei. I will present our predictions for a new IoI at N=50 which should add to the well known ones at N=8, 20, 28 and 40.

48. ISOLDE physics in the HIE-ISOLDE era

Dr Miguel Madurga (CERN)

27/06/2016, 14:50

The HIE-ISOLDE upgrade of the post-accelator LINAC complex at ISOLDE aimed to increase the intensity and energy of post-accelerated beams at the ISOLDE facility, CERN. With a projected energy of 12 MeV/U for beams of A/q up to 4.5 the HIE-ISOLDE facility will allow users to study entirety of the species available at ISOLDE. After the two year Long Shutdown 1 at CERN the first HIE-ISOLDE...

26. Shape coexistence in neutron-rich Strontium isotopes at N=60

Dr Emmanuel Clement (GANIL)

27/06/2016, 15:20

Neutron-rich A~100 nuclei are among the best examples of interplay of microscopic and macroscopic effects in nuclear matter. A dramatic onset of quadrupole deformation is observed in the neutron-rich Zr and Sr isotopes at N=60, making this region an active area of experimental and theoretical studies. This rapid shape transition is accompanied by the appearance of low-lying 0+2 states that,...

28. Collectivity of 4+ states in heavy Zn isotopes and the first HIE-ISOLDE experiment

Dr Magda Zielinska (CEA Saclay)

27/06/2016, 15:40

Shell evolution in the vicinity of 68Ni has recently attracted many theoretical and experimental investigations. By now it has been clearly established that the presumed subshell closure at N=40 is not very pronounced. While the intruder character of the 1g9/2 and 2d5/2 neutron orbital induces collectivity by pair excitations from the fp shell into the g9/2 orbital, the parity change hinders...