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

June 27, 2016 to July 1, 2016
San Servolo, Venice
Europe/Rome timezone

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Session

Physics of neutron-rich nuclei

Jun 27, 2016, 2:00 PM
San Servolo, Venice

San Servolo, Venice

Conveners

Physics of neutron-rich nuclei

  • Giacomo De Angelis (LNL)

Presentation materials

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  1. 54. Welcome
    Prof. Silvia M. Lenzi (PD)
    6/27/16, 2:00 PM
  2. 13. The Inversion Archipelago at The Neutron Rich Shores
    Prof. Alfredo Poves (Universidad Autonoma de Madrid)
    6/27/16, 2:20 PM
    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.
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  3. 48. ISOLDE physics in the HIE-ISOLDE era
    Dr Miguel Madurga (CERN)
    6/27/16, 2:50 PM
    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...
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  4. 26. Shape coexistence in neutron-rich Strontium isotopes at N=60
    Dr Emmanuel Clement (GANIL)
    6/27/16, 3:20 PM
    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,...
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  5. 28. Collectivity of 4+ states in heavy Zn isotopes and the first HIE-ISOLDE experiment
    Dr Magda Zielinska (CEA Saclay)
    6/27/16, 3:40 PM
    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...
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