Ouvrages édités à titre de seul éditeur ou en collaboration (1)
  1. 1. Jorissen, A., Goriely, S., Siess, L., Rayet, M., & Boffin, H. (2004). The Future Astronuclear Physics: From Microscopic Puzzles to Macroscopic Nightmares. Paris: EDP sciences.
    2.   Parties d'ouvrages collectifs (6)
  2. 1. Blaum, K., Eliseev, S., & Goriely, S. (2023). Masses of exotic nuclei. In I. Tanihata, H. Toki, & T. Kajino (Eds.), Handbook of Nuclear Physics, Handbook of Nuclear Physics. Singapore: Springer. doi:10.1007/978-981-15-8818-1_101-1
  3. 2. Goriely, S., & Kullmann, I. (2023). R-Process Nucleosynthesis in Neutron Star Merger Ejecta and Nuclear Dependences. In I. Tanihata, H. Toki, & T. Kajino (Eds.), Handbook of Nuclear Physics (pp. 1-26). Singapore: Springer. doi:10.1007/978-981-15-8818-1_91-1
  4. 3. Kankainen, A., & Goriely, S. (2022). Nuclear Data and Experiments for Astrophysics. In Lenzi & D. Cortina-Gil (Eds.), Nuclear Data and Experiments for Astrophysics, Vol. 1005. The Euroschool on Exotic Beams, Vol. VI. Lecture Notes in Physics (p. 141). Cham: Springer. doi:10.1007/978-3-031-10751-1_4
  5. 4. Chamel, N., Pearson, M. J., & Goriely, S. (2013). Pairing: from atomic nuclei to neutron-star crusts. In R. Broglia & V. Zelevinsky (Eds.), 50 years of nuclear BCS: Pairing in Finite Systems (pp. 284-296). World Scientific. doi:10.1142/9789814412490_0021
  6. 5. Arnould, M., & Goriely, S. (2012). The r-process of nucleosynthesis: The puzzle is still with us. In I. Küçük (Ed.), The r-process of nucleosynthesis: The puzzle is still with us (pp. 61-88). Croatia: InTech - Open Access Publisher.
  7. 6. Goriely, S., Chamel, N., & Pearson, M. J. (2012). Neutron-star crusts and finite nuclei. In C. Bertulani & J. Piekarewicz (Eds.), Neutron Star Crust (pp. 213-233). Hauppauge, New York: Nova Science Publishers.
    8.   Articles dans des revues avec comité de lecture (483)
  8. 1. Riyas, A., Karinkuzhi, D., Van Eck, S., Choplin, A., Goriely, S., Siess, L., Keerthy, M., Jorissen, A., & Merle, T. (2026). Abundance of heavy r-process elements in CEMP-rs stars: The role of the i-process. Astrophysical Journal.
  9. 2. Choplin, A., Siess, L., Goriely, S., Eggenberger, P., & Moyano, F. F. (2026). The intermediate neutron capture process. VI. Proton ingestion and i-process in rotating magnetic asymptotic giant branch stars. Astronomy & astrophysics. doi:10.1051/0004-6361/202557649
  10. 3. Sánchez Fernández, A., Bara, S., Ryssens, W., & Goriely, S. (2026). Accurate spontaneous fission half-lives from a microscopic large-scale nuclear structure model. Physics letters. Section B, 874, 140287. doi:10.1016/j.physletb.2026.140287
  11. 4. Xu, Y., Goriely, S., Krticka, M., & Khan, E. (2026). Systematic studies of M1 photon strength functions with Skyrme-HFB+QRPA and the derived total dipole (E1+M1) resonance properties. Physical review. C. Nuclear physics, 113, 014306. doi:10.1103/4z11-s1yc
  12. 5. Goriely, S., Ryssens, W., Hilaire, S., & Koning, A. (2026). Improved microscopic nuclear level densities within the triaxial Hartree-Fock-Bogoliubov plus combinatorial method. Physical Review C, 113(1). doi:10.1103/r6pn-xjnv
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