From nuclear matter to Neutron Stars

Details From nuclear matter to Neutron Stars From nuclear matter to Neutron Stars

2009-02-02

arxiv.org/abs/0902.0262v1

Physics

Nuclear Physics

Nuclear Theory

10 Figures, 1 Table

Scientific paper

Neutron stars are the most dense objects in the observable Universe and conventionally one uses nuclear theory to obtain the equation of state (EOS) of dense hadronic matter and the global properties of these stars. In this work, we review various aspects of nuclear matter within an effective Chiral model and interlink fundamental quantities both from nuclear saturation as well as vacuum properties and correlate it with the star properties.

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