13–17 Jul 2026
Europe/Lisbon timezone

Session

NUC-RIA Internal Days

13 Jul 2026, 09:30

Presentation materials

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  1. Manuel Xarepe (Faculty of Science of the University of Lisbon)
    13/07/2026, 09:30
  2. Carolina Felgueiras
    13/07/2026, 10:30
  3. Paula De Dios Caro
    13/07/2026, 11:00
  4. Afonso Vicente (IJCLab-IN2P3-CNRS)
    13/07/2026, 11:30

    Radioactive molecules have recently emerged as precision probes for anomalous electromagnetic moments, possibly offering unprecedented sensitivity to parity violation and time reversal symmetry violation [1]. In current experiments at radioactive ion beam facilities, the high temperature of the different molecular degrees of freedom is a crucial limiting factor for sensitive measurements. To...

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  5. Margarida Paulino
    13/07/2026, 12:00
  6. Tomás Campante (Deparment of Physics, Faculty of Sciences of the University of Lisbon (FCUL). Laboratory of Instrumentation and Experimental Particle Physics (LIP).)
    15/07/2026, 09:00
    Oral Presentation

    Observations of kilonovae, the electromagnetic counterparts to (binary) neutron star mergers, confirm their role as key sites for $r$-process nucleosynthesis, producing elements heavier than ion in the expanding ejecta following this event. The groundbreaking observation of the 2017’s kilonova (astronomical transient AT2017gfo) associated with the renowned gravitational wave event GW170817...

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  7. Ricardo Ferreira da Silva (LIP)
    15/07/2026, 09:30

    Comprehensive datasets of electron-impact excitation (EIE) collision strengths for near-neutral lanthanides and other r-process elements remain notably incomplete, despite their central role in setting the level populations of neutron-star merger ejecta during the late phase (non local thermodynamic equilibrium, more commonly known as non-LTE, regime), of kilonova emission [1, 2]. A...

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  8. João Jantarada (Nuc-Ria)
    15/07/2026, 10:00
    Oral Presentation

    The astrophysical origin of the heavy neutron-deficient isotopes, commonly referred to as p-nuclei, remains one of the major open problems in Nuclear Astrophysics. Among the proposed production sites, Core-Collapse Supernovae (CCSNe) are considered one of the most promising environments for their nucleosynthesis. In this presentation, I will discuss the current results of my PhD research,...

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  9. Francisca Afonso (LIP)
    15/07/2026, 11:00
  10. Beatriz Amorim (University of York)
    15/07/2026, 11:30
    Oral Presentation

    The upgraded setup for the R3B experiments at FAIR introduces a pixel-based Target Recoil Tracker (TRT) detector, designed to enhance the detection capabilities of light-charged particles, such as protons, emitted in nuclear reactions. The TRT surrounds the reaction
    target and is further enclosed within a highly segmented calorimeter, named CALIFA, focusing on precise angle measurements of...

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  11. Duarte Casquilho, Filipa Quadrilheiro
    15/07/2026, 14:00
  12. André Torcato (LIP)
    15/07/2026, 14:30
    Oral Presentation

    Simplifying the three-body equations that describe baryons in low-energy non-perturbative QCD into two-body equations, introducing the diquark, quark-quark bound states, as baryon constituents. From these, baryon mass calculations, partial wave decompositions and diquark contributions to the baryon states can be done.

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  13. José Graça
    15/07/2026, 15:00
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