21–25 sept. 2026
Fuseau horaire Europe/Paris

Session

Heavy ion Collisions

24 sept. 2026, 15:00

Documents de présentation

Aucun document.

  1. Caterina Ciampi (GANIL)
    24/09/2026 15:00
  2. Dr Diego Gruyer (LPC Caen)
    24/09/2026 15:25
    Oral Presentation

    The equation of state (EoS) of neutron-rich matter is a cornerstone for understanding the structure and dynamics of neutron stars, from their radii and tidal deformability to cooling mechanisms. However, the density dependence of the nuclear symmetry energy term remains a major source of uncertainty, particularly at densities near, and above, nuclear saturation density. While astrophysical...

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  3. Ilham DEKHISSI
    24/09/2026 15:45
    Oral Presentation

    The second $0_{2}^+$ state of $^{12}$C at an excitation energy of 7.654 MeV, known as the Hoyle state [1], is crucial to understanding how $^{12}$C is formed in stellar nucleosynthesis. Despite recent studies, there is no consensus on the properties of the Hoyle state, with different theoretical models predicting a range of radii and spatial arrangements[2,3].

    Experimentally, only a few...

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