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Mario Centelles

11

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Unified Equation of State for Neutron Stars Based on the Gogny Interaction

2021 arXiv: Nuclear Theory
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Influence of direct Urca on the r-mode spin down features of newborn neutron star pulsars

2021 Physica Scripta
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Unified Equation of State for Neutron Stars Based on the Gogny Interaction

2021 Symmetry
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Microscopic-Macroscopic Approach for Ground-State Energies Based on the Gogny Force with the Wigner-Kirkwood Averaging Scheme.

2020 arXiv: Nuclear Theory
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Woods-Saxon-type of mean-field potentials with effective mass derived from the D1S Gogny force.

2020 arXiv: Nuclear Theory
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Structure and composition of the inner crust of neutron stars from Gogny interactions

2020 Physical Review C
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The physics of Chandrasekhar and Super-Chandrasekhar White Dwarfs

2015
- Edgar Molina Lumbreras
- Mario Centelles
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Origin of the neutron skin thickness of 208Pb in nuclear mean-field models

2010 Physical Review D
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Influence of the symmetry energy on the giant monopole resonance of neutron-rich nuclei

2009 arXiv: Nuclear Theory
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