Neutron-proton effective mass splitting and thermal evolution in neutron rich matter

Details Neutron-proton effective mass splitting and thermal evolution in neutron rich matter Neutron-proton effective mass splitting and thermal evolution in neutron rich matter

2011-08-09

arxiv.org/abs/1108.1930v1

Physics

Nuclear Physics

Nuclear Theory

19 pages, 9 figures, Submitted to J.Phys.G:Nucl.Part.Phys

Scientific paper

The thermal evolution of properties of neutron rich asymmetric nuclear matter such as entropy density, internal energy density, free energy density and pressure are studied in the non-relativistic mean field theory using finite range effective interactions. In this framework the thermal evolution of nuclear matter properties is directly connected to the neutron and proton effective mass properties. Depending on the magnitude of neutron-proton effective mass splittings, two distinct behaviours in the thermal evolution of nuclear matter properties are noticed.

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