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Units : Astronomy and Astrophysics Institute | ULB105
Theoretical study of various nuclear quantities of importance for stellar evolution models and for the nucleosynthesis: nuclear reaction rates, weak interaction fission, nuclear masses and level densities. Study of the non-explosive and explosive of stellar nucleosynthesis aiming to understand the chemical and isotopic composition of the solar system, of stars and galaxies.
• F.R.S.-FNRS et Fonds associés (hors FRIA)
• FRIA
• Fonds associés (toutes subventions, y compris la Loterie Nat.)
• PAI
• Autres ministères fédéraux
• Initiatives ministérielles et autres Communauté française
• Région flamande
• Autres U.E.