“…The nuclear equation of state is usually interpreted as average energy of a nucleonic system per number of nucleons ) ( A E . This equation of state can explain the average energy per nucleon of a symmetric nuclear matter, around its equilibrium state, using two variables: temperature T and density ) , ( T e A E sym (1) and it can describe the average energy per nucleon of an asymmetric nuclear matter, around the condition in which the system is equilibrated, using three variables: temperature T , density and which appears as a result of asymmetry in the number of protons and neutrons in the system ) , , ( T e A E asym (2) this variable is defined as the following: When the thermal energy in a nucleonic system is low, the temperature T will be negligible and the nuclear equation of state for the asymmetric nuclear matter around its equilibrium state will be expressed as a function of two variable:…”