10–12 Nov 2021
Legnaro National Laboratory
Europe/Rome timezone

Session

REPORTS on AGATA Experiments

11 Nov 2021, 09:30
Legnaro National Laboratory

Legnaro National Laboratory

Conveners

REPORTS on AGATA Experiments: SESSION 1

  • Peter Reiter

Presentation materials

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  1. Tayfun Huyuk (IFIC (CSIC - Universidad de Valencia))
    11/11/2021, 09:30

    In this work, we studied the structure of the pf-shell N=Z nucleus $^{52}$Fe with relativistic radioactive ion beam techniques to reveal the collectivity in this region. $^{52}$Fe presents an interesting case in which we see the onset of a collective structure that is more common nuclear property in heavier nuclei. We deduced the reduced transition probability of the 0$_{gs}^{+}$ $\rightarrow$...

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  2. R. Perez-Vidal (INFN Legnaro)
    11/11/2021, 09:50

    In order to shed light on the open question of the seniority conservation in the proton g9/2 orbital in the N=50 isotones [1,2], reduced transition probabilities in 90Zr, 92Mo and 94Ru nuclei, have been determined experimentally for the first time via lifetime measurements at the GANIL laboratory. The unconventional use of multi-nucleon transfer reaction [3] with a differential plunger device...

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  3. Tamara Milanović
    11/11/2021, 10:10

    The experiment E708 was performed in GANIL in 2016, aiming to investigate evolution of collectivity in odd mass Ga isotopes around N=40 and neighbouring nuclei. The lifetime measurements of the low-lying states in nuclei of interest would allow us to deduce the transition probabilities and extend our knowledge of the interplay between single-particle and collective degrees of freedom in this...

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  4. Chloé Fougères (GANIL)
    11/11/2021, 10:30

    Simulations of novae explosive nucleosynthesis predict the production of the radionuclide $^{22}$Na. Its half life of 2.6 yr makes it a very interesting astronomical observable by allowing space and time correlations with the astrophysical object. This radionuclide should bring constraints on nova models. It may also help to explain abnormal $^{22}$Ne abundance observed in presolar grains and...

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