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Phase transition and frustration in nuclear physic and astrophysic. Phd Supervisors : Ph. Chomaz (1), F. Gulminelli (2). Collaborators : C. Ducoin (3),

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Presentation on theme: "Phase transition and frustration in nuclear physic and astrophysic. Phd Supervisors : Ph. Chomaz (1), F. Gulminelli (2). Collaborators : C. Ducoin (3),"— Presentation transcript:

1 Phase transition and frustration in nuclear physic and astrophysic. Phd Supervisors : Ph. Chomaz (1), F. Gulminelli (2). Collaborators : C. Ducoin (3), T. Furuta (1), P. Napolitani (2), D. Wood (1). Karim Hasnaoui (1) (1) GANIL (DSM-CEA/IN2P3-CNRS),Blvd. H. Becquerel, F-14076 Caen cédex, France. (2) LPC Caen (IN2P3-CNRS/Ensicaen et Université), F-14050 Caen cédex, France. (3) INFN, Sezione di Catania, Via Santa Sofia 64, I-95123 Catania, Italie. Les jeunots en physique nucléaire de basse énergie. On fait quoi ? Comment ?

2 Classical Approaches : LGM & RG. LGM (Lattice Gas Model) for star matter : Liquid-gas phase transition. Suppression of critical point. PRL98, 131102 (2007). PRC75, 65805 (2007). RG (Renormalisation Group) : Mixe short and long range interaction Critical Phenomena ?

3 Quantum Approach : FMD. Ingredients of FMD (Fermionic molecular dynamics) : Antisymetrisation of gaussian wave packet. Realistic interaction : Skyrme force. Nuclear thermometer. Thermodynamics : Caloric curve of finite nuclei. Treat the quantum probleme for star matter. Nuclear Structure : Ground State. Giant resonance GMR of light nuclei.

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