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T. Gaitanos, M. Di Toro, S. Typel, V. Baran, C. Fuchs, V. Greco, and H. H. Wolter, Nucl. Phys. A 732
2004
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P. B. Demorest, T. Pennucci, S. M. Ransom, M. S. E. Roberts, and J. W. T. Hessels, Nature 467
2010
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Mariana Dutra, Odilon Lourenço, and Débora P. Menezes, Phys. Rev. C 93
2016
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2015

Stellar properties and nuclear matter constraints

Dutra, Mariana, Lourenço, Odilon, Menezes, Débora P.

Understand

We have analyzed stellar properties of the relativistic mean-field (RMF) parametrizations shown to be consistent with the recently studied constraints related to nuclear matter, pure neutron matter, symmetry energy and its derivatives [Dutra et al., Phys.

Rev.
C 90, 055203 (2014)].
Our results show that only two RMF parametrizations do not allow the emergence of the direct Urca process, important aspect regarding the evolution of a neutron star.