activity
19972025
most citedNuclear symmetry energy probed by neutron skin thickness of nuclei

568 citations · 4.4k across the 86 of their papers we have counts for

collaborators

86 papers

nucl-th2025

Asymmetric warm nuclear matter described by Gogny and Skyrme-version models

Odilon Lourenço, Mariana Dutra, Mario Centelles +1

In this work, we perform a detailed study of the thermodynamical properties of asymmetric nuclear matter at finite temperatures by means of the Gogny force, with a particular focus…

nucl-th2024★ 4 cited

Equation of State of Hot Neutron Star Matter using Finite Range Simple Effective Interaction

T. R. Routray, S. Sahoo, X. Viñas +2

The equation of state of hot neutron star matter of n+p+e+ composition in -equilibrium is studied for both neutrino-free isothermal and neutrino-trapped isentropic conditions…

nucl-th2024★ 6 cited

Impact of Hot Inner Crust on Compact Stars at Finite Temperature

Clara Dehman, Mario Centelles, Xavier Viñas

We conducted a study on the thermal properties of stellar matter with the nuclear energy density functional BCPM. This functional is based on microscopic Brueckner-Hartree-Fock cal…

nucl-th2023★ 28 cited

Correlations between charge radii differences of mirror nuclei and stellar observables

P. Bano, S. P. Pattnaik, M. Centelles +2

The correlation between the charge radii differences in mirror nuclei pairs and the neutron skin thickness has been studied with the so-called finite range simple effective interac…

nucl-th2022★ 6 cited

The finite range simple effective interaction including tensor terms

P. Bano, X. Viñas, T. R. Routray +3

The prediction of single particle level crossing phenomenon between and orbitals in - and -isotopic chains by the finite range simple effective intera…

nucl-th2021

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

Xavier Viñas, Claudia Gonzalez-Boquera, Mario Centelles +2

The most popular Gogny parametrizations, namely D1S, D1N and D1M, describe accurately the ground-state properties of spherical and deformed finite nuclei all across the mass table…