Session

Session 11

S11
12 Mar 2026, 09:00
Kore University of Enna

Kore University of Enna

Polo scientifico/tecnologico Santa Panasia

Conveners

Session 11

  • Takashi Nakamura

Presentation materials

There are no materials yet.

  1. Alessandro Roggero (Istituto Nazionale di Fisica Nucleare)
    12/03/2026, 09:00
  2. Manuela Cavallaro (INFN -LNS)
    12/03/2026, 09:30
  3. Anna Togni (Istituto Nazionale di Fisica Nucleare)
    12/03/2026, 10:00

    I will present the results of the commissioning campaign coupling the EXOTIC facility with the AGATA γ‑ray tracking array, with a focus on the delivery of the radioactive ion beam inside the AGATA reaction chamber. I will also introduce the experiment planned with this configuration and share preliminary results from the first experimental campaigns.

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  4. Francesco Andreis (UniPG, Istituto Nazionale di Fisica Nucleare)
    12/03/2026, 10:15

    The ADONIS experiment (Aluminum DestructION in Stars) is framed within the context of Multimessenger Astronomy and aims to improve the understanding of nucleosynthesis processes through the study of the radioactive isotope 26Al. This nucleus, the first γ-ray emitter observed in our Galaxy, is crucial for understanding the evolution of massive stars, the supernova explosions and the consequent...

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  5. Kenta Yoshimura (Institute of Science Tokyo)
    12/03/2026, 10:30

    Neutron stars are compact objects filled with nuclear (hadronic) matter that reaches several times the nuclear saturation density at their centers, and they are regarded as one of the frontier topics in modern theoretical physics. In the region known as the inner crust, a crystalline lattice of neutron-rich nuclei coexists with a superfluid gas of unbound neutrons, a state that carries crucial...

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  6. Silvia Trabucco (University of Innsbruck)
    12/03/2026, 10:45

    Supersolidity is a peculiar phase of matter in which superfluidity and crystalline order coexist. Owing to this dual character, it provides a powerful platform for investigating systems with multiple simultaneously broken symmetries, such as nuclear matter in the interior of neutron stars. In this work, we simulate the dynamics of the neutron-star inner crust during a glitch, focusing on the...

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