activity
20052017
most citedCore-crust transition in neutron stars: predictivity of density developments

228 citations · 787 across the 16 of their papers we have counts for

collaborators

16 papers

nucl-th2017★ 4 cited

Elementary excitations in homogeneous superfluid neutron star matter: role of the neutron-proton coupling

Marcello Baldo, Camille Ducoin

The thermal evolution of Neutron Stars is affected by the elementary excitations that characterize the stellar matter. In particular, the low-energy excitations, with a spectrum li…

nucl-th2013★ 54 cited

Imprint of the symmetry energy on the inner crust and strangeness content of neutron stars

Constança Providência, Sidney S. Avancini, Rafael Cavagnoli +7

In this work we study the effect of the symmetry energy on several properties of neutron stars. First, we discuss its effect on the density, proton fraction and pressure of the neu…

nucl-th2011★ 5 cited

Plasmons in strong superconductors

Marcello Baldo, Camille Ducoin

We present a study of the possible plasmon excitations that can occur in systems where strong superconductivity is present. In these systems the plasmon energy is comparable to, or…

nucl-th2011★ 11 cited

Elementary excitations in homogeneous superfluid neutron star matter: Role of the proton component

Marcello Baldo, Camille Ducoin

The thermal evolution of neuron stars depends on the elementary excitations affecting the stellar matter. In particular, the low-energy excitations, whose energy is proportional to…

nucl-th2011★ 228 cited

Core-crust transition in neutron stars: predictivity of density developments

Camille Ducoin, Jérôme Margueron, Constança Providência +1

The possibility to draw links between the isospin properties of nuclei and the structure of compact stars is a stimulating perspective. In order to pursue this objective on a sound…

nucl-th2010★ 86 cited

Nuclear symmetry energy and core-crust transition in neutron stars: a critical study

Camille Ducoin, Jérôme Margueron, Constança Providencia

The slope of the nuclear symmetry energy at saturation density is pointed out as a crucial quantity to determine the mass and width of neutron-star crusts. This letter clarifie…