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

Session

AGATA Collaboration Meeting: SESSION 4

12 Nov 2021, 09:30
Legnaro National Laboratory

Legnaro National Laboratory

Conveners

AGATA Collaboration Meeting: SESSION 4

  • Adriana Nannini (Istituto Nazionale di Fisica Nucleare)

Presentation materials

There are no materials yet.

  1. Valérian Alcindor (TU-Darmstadt)
    12/11/2021, 09:30

    Two recent measurements performed at GANIL studied the unbound nucleus $^{15}$F using a SPIRAL 1 radioactive $^{14}$O beam impinging on the hydrogen nuclei from a thick (100 $\mu$m) polyethylene (CH$_2$) target. The first experiment was performed using the MUST2 light-particle detector array at LISE. The second experiment was part of the campaign using the new MUGAST light particle detector...

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  2. Christian Aaen Diget (University of York)
    12/11/2021, 09:50

    We present new experimental results for a measurement utilising the combination of AGATA, MUGAST, and VAMOS for a determination of the astrophysical $^{15}$O alpha capture reaction rate [1]. This reaction is a key breakout route from the Hot CNO cycle leading to explosive nucleosynthesis via the rp-process on the surface of neutron stars in binary systems. Determining an accurate cross section...

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  3. Daniele Brugnara (Istituto Nazionale di Fisica Nucleare)
    12/11/2021, 10:10

    The evolution of the nuclear shell closure along N=28 has gathered much interest due to the observed
    discrepancies between the well established shell model with SDPF-U interaction and measurements of
    the half-magic 46Ar isotope.
    In particular, while remarkable agreement was observed between theoretical and experimental values
    of Sn, transition probabilities measured with intermediate...

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  4. Irene Zanon (Istituto Nazionale di Fisica Nucleare)
    12/11/2021, 10:30

    Neutron-rich oxygen isotopes constitute a perfect playground for testing three-body forces.
    For example, the neutron drip line is correctly predicted only when these forces are included in the calculation, as demonstrated by the work of Otsuka et al. [1].
    In fact, standard shell model calculations including only two-body forces predict the drip line to be positioned at $N=20$.
    The...

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