70 citations · 261 across the 11 of their papers we have counts for
11 papers
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…
Constraints from GW170817 on the bulk viscosity of neutron star matter and the r-mode instability
T. R. Routray, S. P. Pattnaik, C. Gonzalez-Boquera +3
We perform a systematic study of the dependence of the r-mode phenomenology in normal fluid pulsar neutron stars on the symmetry energy slope parameter . An essential ingredient…
Comment on the paper Eur. Phys. J. A (2019) 55:150
C. Gonzalez-Boquera, M. Centelles, X. Viñas L. M. Robledo
The conclusions of the study published as Eur. Phys. J. A (2019) 55:150 questioning the adequacy of the recently proposed Gogny D1M* interaction for finite-nuclei calculations usin…
Neutron-rich matter in atomic nuclei and neutron stars
Claudia Gonzalez-Boquera
The proper understanding of the equation of state (EoS) of highly asymmetric nuclear matter is essential when studying systems such as neutron stars (NSs). Using zero-range Skyrme…
GW170817 constraints analyzed with Gogny forces and momentum-dependent interactions
O. Lourenço, M. Bhuyan, C. H. Lenzi +4
A set of equations of state obtained from finite-range Gogny forces and momentum-dependent interactions is used to investigate the recent observation of gravitational waves from th…
Interplay between Particles and Hyperons in Neutron Stars
Patricia Ribes, Angels Ramos, Laura Tolos +2
We analyze the effects of including isobars in an equation of state (EoS) for cold, -stable neutron star matter, employing relativistic nuclear mean field theory. The…
Study of the core-crust transition in neutron stars with finite-range interactions: the dynamical method
C. Gonzalez-Boquera, M. Centelles, X. Viñas +1
The properties of the core-crust transition in neutron stars are investigated using effective nuclear forces of finite-range. Special attention is paid to the so-called dynamical m…
Gogny forces in the astrophysical context
X. Viñas, C. Gonzalez-Boquera, M. Centelles +2
The most successful Gogny interactions of the D1 family, namely D1S, D1N and D1M, suffer the common problem of a too soft neutron matter equation of state at high density, which pr…
Comment on the manuscript 1806.02080v1 entitled "Spurious finite-size instabilities of a new Gogny interaction suitable for astrophysical applications"
C. Gonzalez-Boquera, M. Centelles, X. Viñas +1
The conclusions of the manuscript 1806.02080v1 questioning the adequacy of the recently proposed Gogny D1M* interaction for finite nuclei calculations using harmonic oscillator (HO…
New Gogny interaction suitable for astrophysical applications
C. Gonzalez-Boquera, M. Centelles, X. Viñas +1
The D1 family of parametrizations of the Gogny interaction commonly suffers from a rather soft neutron matter equation of state that leads to maximal masses of neutron stars well b…
Higher-order symmetry energy and neutron star core-crust transition with Gogny forces
C. Gonzalez-Boquera, M. Centelles, X. Viñas +1
We study the symmetry energy and the core-crust transition in neutron stars using the finite-range Gogny nuclear interaction and examine the deduced crustal thickness and crustal m…