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Advances in Radioactive Isotope Science

4–9 juin 2023
Palais des Papes - Avignon - France
Fuseau horaire Europe/Paris
Thanks to all for an outstanding conference - see you in Fukushima for ARIS 2026!

Session

plenary 03

5 juin 2023, 14:30
conclave

conclave

Présidents de session

plenary 03

  • Byungsik Hong (Korea University)

Documents de présentation

Aucun document.

  1. 620. The Decay Spectroscopy Setup at the GSI-FAIR fascility and the physics results from FAIR-0
    Biswarup Das (GSI Helmholtzzentrum für Schwerionenforschung)
    05/06/2023 14:30
    spectroscopy
    invited presentation

    The DEcay SPECtroscopy (DESPEC) setup assembled for the future GSI-FAIR fascility in Darmstadt, Germany, aims to study the nuclear footprint mainly through gamma ray spectroscopic measurements.
    As a part of the NUSTAR project, the DESPEC collaboration aims to search for the exotic nuclear structure phenomena such as shell evolution in nuclei which take part in the astrophysical r-processes....

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  2. 631. Evolution of single-particle properties probed with the ISOLDE Solenoidal Spectrometer
    David Sharp (The University of Manchester)
    05/06/2023 14:55
    reactions
    invited presentation

    The ISOLDE Solenoidal Spectrometer (ISS) has been built for measuring direct reactions in inverse kinematics with radioactive beams (RIBs) from HIE-ISOLDE, with a focus on obtaining excellent charged particle resolution. ISS was fully commissioned in 2021 with a new silicon array developed by the University of Liverpool. This array makes use of double-sided silicon strip detectors, with ASIC...

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  3. 654. Proton radioactivity studies with ACTAR TPC
    Jérôme Giovinazzo (LP2IB (CENBG) CNRS / Univ. Bordeaux)
    05/06/2023 15:20
    ground-state properties
    invited presentation

    (for the E690 and E791 collaborations)

    For nuclear systems that are slightly unbound with respect to the nuclear strong interaction, the 1- and 2-proton radioactivity decay channel opens [1,2]. The experimental study of these radioactivities offers a unique access to the structure properties of the emitting states. Such data can represent real challenges in terms of theoretical...

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  4. 650. r process and supernova signatures in deep-sea archives
    Anton Wallner (Helmholtz Center Dresden-Rossendorf / Australian National University)
    05/06/2023 15:45
    astrophysics/nucleosynthesis
    invited presentation

    Half of the heavy elements are produced in r-process nucleosynthesis, which is exclusively responsible for actinide production, such as Pu-244 (t$_{1/2}$=81 Myr). The r-process requires an explosive scenario but is far from being fully understood; in particular, its sites and history.

    The solar system moves through the interstellar medium (ISM) and collects interstellar dust particles that...

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