Thermal effects on nuclear matter properties

A quantitative description of the properties hot nuclear matter will be needed for interpretation available and forthcoming astrophysical data, providing information on post merger phase a neutron star coalescence. We have employed recently developed theoretical model, based phenomenological Hamiltonian including two- three-nucleon potentials, to study temperature dependence average single-particle relevant applications. The possibility represent results microscopic calculations using simple yet physically motivated parametrisations thermal effects, suitable use in numerical simulations processes, is also discussed.