Journal
PHYSICAL REVIEW C
Volume 84, Issue 6, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevC.84.065810
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Funding
- CNPq (Brazil)
- CAPES (Brazil)/FCT (Portugal) [232/09]
- FCT (Portugal) [PTDC/FIS/113292/2009, CERN/FP/109316/2009]
- Fundação para a Ciência e a Tecnologia [CERN/FP/109316/2009] Funding Source: FCT
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The effect of the symmetry energy on the properties of compact stars is discussed. It is shown that, for stars with masses above 1M(circle dot), the radius of the star varies linearly with the symmetry energy slope L. We also analyze the dependence of the hyperon content and onset density of the direct Urca process on the symmetry energy and meson coupling parametrization.
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