The prospects of hot and dense asymmetric nuclear matter

The study of the equation of state (EOS) of hot asymmetric nuclear matter (ANM) has become a major area of research in nuclear physics and astrophysics during the last two decades. It plays an important role in the interpretation of nucleus-nucleus collision in which a hot and dense state of matter is formed. The many-body problem at finite temperatures has been considered by several authors within different approaches, such as the finite temperature Green's function method, the thermo-field method, or the Bloch-De Domicis (BD) diagrammatic expansion. In the present study we will examine the properties of ANM like binding energy per nucleon and internal energy using a simple density dependent finite range effective interaction