Neutron star properties and the symmetry energy

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

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12 pages, 20 figures, submitted to Phyical Review C

Scientific paper

The effect of the symmetry energy on the properties of compact stars is
discussed. It is shown that, for stars with masses above 1 $M_\odot$, the
radius of the star varies linearly with the symmetry energy slope $L$. The
dependence of the hyperon content and onset density of the direct Urca process
on the symmetry energy and meson coupling parametrization are also analyzed.

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