activity
20032024
most citedCrustal Entrainment and Pulsar Glitches

208 citations · 1.7k across the 39 of their papers we have counts for

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Showing 2004Show all

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astro-ph2004

Covariant analysis of Newtonian multi-fluid models for neutron stars: III Transvective, viscous, and superfluid drag dissipation

Brandon Carter, Nicolas Chamel

As a follow up to articles dealing firstly with a convective variational formulation in a Milne-Cartan framework for non-dissipative multi fluid models, and secondly with various e…

astro-ph2004187 cited

Analytical representations of unified equations of state of neutron-star matter

P. Haensel, A. Y. Potekhin

Analytical representations are derived for two equations of state (EOSs) of neutron-star matter: FPS and SLy. Each of these EOSs is unified, that is, it describes the crust and the…

astro-ph2004

Effect of BCS pairing on entrainment in neutron superfluid current in neutron star crust

Brandon Carter, Nicolas Chamel, Pawel Haensel

The relative current density of conduction neutrons in a neutron star crust beyond the neutron drip threshold can be expected to be related to the corresponding particle mome…

nucl-th2004

Band structure effects for dripped neutrons in neutron star crust

Nicolas Chamel

The outer layers of a neutron star are supposed to be formed of a solid Coulomb lattice of neutron rich nuclei. At densities above neutron drip density (about one thousandth of nuc…

nucl-th2004

Entrainment coefficient and effective mass for conduction neutrons in neutron star crust: simple microscopic models

Brandon Carter, Nicolas Chamel, Pawel Haensel

In the inner crust of a neutron star, at densities above the ``drip'' threshold, unbound ``conduction'' neutrons can move freely past through the ionic lattice formed by the nuclei…