Light Nuclei within Nuclear Matter

We investigate the properties of 3 He, 4 He, 6 He, 7 Li and 16 O nuclei in nuclear matter of finite temperature and density. A Dyson expansion of the many-body Green function leads to few-body equations that are solved using the Integro-Differential Equation Approach (IDEA) and the Antisymmetrized Molecular Dynamics (AMD) methods. The use of the latter method allows us to trace the individual movement of the wave packet for each nucleon and the formation and disintegration of quasinuclei in a changing thermodynamical nuclear matter environment.