Relativistic and thermodynamically consistent treatment for the finite volume effect of nucleons in nuclear matter.

Physics

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Neutron Stars: Phase Transitions

Scientific paper

A previous thermodynamically consistent procedure for considering the finite volume effect of nucleons in nuclear matter is developed to be relativistic. Parameters are determined by fitting all five empirical data for normal nuclear matter. The resulting nuclear equations of state may be used in researches for neutron stars and for phase transitions between nuclear matter and quark gluon plasma.

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