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Neutron star properties and the symmetry energy

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arxiv 1108.1733 v1 pith:H7TEC2B2 submitted 2011-08-08 hep-ph nucl-th

Rafael Cavagnoli , Constança Providência , Debora P. Menezes This is my paper · ORCID
classification hep-phnucl-th
keywords energysymmetrypropertiesstarstarsaboveanalyzedcompact
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abstract

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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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Impact of the Scalar Isovector $\delta$-meson on the description of nuclear matter and neutron star properties

    nucl-th 2024-12 conditional novelty 5.0 of 10

    Including the delta meson in relativistic mean-field models widens the allowed symmetry energy slope and curvature, changing low-mass neutron star radii while leaving maximum mass nearly fixed.

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