Study of neutron-rich nuclides in the A = 170−180 deformed region

28 mar. 2025 12:15
15m
1001-Primera-1-1-1 - Paterna. Seminario (Universe)

1001-Primera-1-1-1 - Paterna. Seminario

Universe

Seminary room at IFIC
60

Ponente

Julgen Pellumaj (INFN-Mi, INFN-LNL)

Descripción

The availability, for higher intense beams at Riken, of a 100 pnA $^{238}$U, in combination with the increased efficiency of the $\gamma$-ray detection array compared to the previous EURICA campaign, opens the way to new experimental studies in the largely unexplored region of neutron-rich rare-earth nuclei. The structure of these nuclei is important from both nuclear astrophysics and nuclear structure perspectives, with respect to the r-process formation of the rare-earth-element (REE) abundance peak, nuclear shape changes and shell evolution [1].

With this proposal, we aim at investigating the neutron-rich nuclei with 170$<$A$<$180, focusing on the Er, Dy and Gd isotopes where K-isomers are predicted to appear. The presence of isomers will allow us to perform gamma-ray spectroscopy below the isomeric states for the first time in several nuclei in this region. We will perform isomeric and β-decay measurements, with a focus on 100 ns $\rightarrow$ ms isomers as entry points to the most neutron-rich structures, exploiting the germanium detector array coupled to the WAS3ABi active stopper.

This measurement will provide an insight in quasiparticle structures and energies, shape, sub-shell and K-mixing effects, and help to develop our understanding of the formation of the r-process REE abundance peak.

[1] W.J. Huang et al., Eur. Phys. J. A 55 (2019) 96

Autores primarios

Marta Polettini (GSI Helmholtzzentrum für Schwerionenforschung) Philip Walker (University of Surrey) Julgen Pellumaj (INFN-Mi, INFN-LNL) Jose Javier Valiente Dobon (LNL-INFN) Giovanna Benzoni (INFN-Milano)

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