# Equation of State for Nucleonic and Hyperonic Neutron Stars with Mass and Radius Constraints

@article{Tolos2016EquationOS, title={Equation of State for Nucleonic and Hyperonic Neutron Stars with Mass and Radius Constraints}, author={Laura Tolos and Mario Centelles and {\`A}ngels Ramos}, journal={arXiv: High Energy Astrophysical Phenomena}, year={2016} }

We obtain a new equation of state for the nucleonic and hyperonic inner core of neutron stars that fulfills the 2$M_{\odot}$ observations as well as the recent determinations of stellar radii below 13 km. The nucleonic equation of state is obtained from a new parametrization of the FSU2 relativistic mean-field functional that satisfies these latest astrophysical constraints and, at the same time, reproduces the properties of nuclear matter and finite nuclei while fulfilling the restrictions on… Expand

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