activity
20122019
most citedInner crust of neutron stars with mass-fitted Skyrme functionals

205 citations · 313 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2019★ 4 cited

Role of the Symmetry Energy on the Structure of Neutron Stars with Unified Equations of State

Nicolas Chamel, John Michael Pearson, Alexander Y. Potekhin +5

The role of the symmetry energy on the internal constitution and the global structure of a cold nonaccreted neutron star is studied using a set of unified equations of state. Based…

astro-ph.HE2019★ 52 cited

Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy

J. M. Pearson, N. Chamel, A. Y. Potekhin +4

The theory of the nuclear energy-density functional is used to provide a unified and thermodynamically consistent treatment of all regions of cold non-accreting neutron stars. In o…

astro-ph.HE2016★ 51 cited

Giant Pulsar Glitches and the Inertia of Neutron-Star Crusts

T. Delsate, N. Chamel, N. Gürlebeck +3

Giant pulsar frequency glitches as detected in the emblematic Vela pulsar have long been thought to be the manifestation of a neutron superfluid permeating the inner crust of a neu…

astro-ph.HE2012★ 1 cited

Structure of neutron stars with unified equations of state

A. F. Fantina, N. Chamel, J. M. Pearson +1

We present a set of three unified equations of states (EoSs) based on the nuclear energy-density functional (EDF) theory.These EoSs are based on generalized Skyrme forces fitted to…

nucl-th2012★ 205 cited

Inner crust of neutron stars with mass-fitted Skyrme functionals

J. M. Pearson, N. Chamel, S. Goriely +1

The equation of state and composition of the inner crust of neutron stars at zero temperature are calculated, using the T = 0 version of the TETFSI (temperature-dependent extended…