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Structure and Dynamics in the Fusion of Neutron-Rich Nuclei

INVITED · APR-S05 · ID: 2683640







Presentations

  • Astrophysical implications from C12 + C12 deep sub barrier fusion

    ORAL · Invited

    Publication: - Submitted to Phys. Rev. C Phys.Rev. C, J. Nippert, S. Courtin et al., Complementing the picture of deep sub-barrier 12C + 12C fusion with STELLA<br>- Phys.Rev. Lett., 124, 192701 (2020), G. Fruet, S. Courtin et al., Advances in the direct study of carbon burning in massive stars.<br>- Astronomy & Astrophysics 668 A115 (2024), T. Dumont, E. Monpribat, S. Courtin et al. Massive star evolution with a new 12C + 12C nuclear reaction rate: the core carbon burning phase.<br>- Phys. Rev. Lett. 129, 102701 (2022), P. Adsley, M. Heine, D. G. Jenkins, S. Courtin et al. Extending the Hoyle-State Paradigm to 12C+12C Fusion.<br>- Astronomy & Astrophysics 660 A47 (2022), E. Monpribat, S. Martinet, S. Courtin et al. A new 12C +12C nuclear reaction rate: impact on stellar evolution.

    Presenters

    • Sandrine Courtin

      CNRS

    Authors

    • Sandrine Courtin

      CNRS

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