We have developed a theoretical model and a numerical code for stationary rotating superfluid neutron stars in full general relativity. The underlying two-fluid model is based on Carter's covariant multi-fluid hydrodynamic formalism. The two fluids, representing the superfluid neutrons on one hand, and the protons and electrons on the other, are restricted to uniform rotation around a common axis, but are allowed to have different rotation rates. We have performed extensive tests of the numerical code, including quantitative comparisons to previous approximative results for these models. The results presented here are the first ``exact'' calculations of such models in the sense that no approximations (other than that inherent in a discretiz...
We develop a formalism that can be used to model slowly rotating superfluid Newtonian neutron stars....
L'objectif de cette thèse est d'étudier différents aspects microscopiques et macroscopiques liés à l...
We present a general formalism to treat slowly rotating general relativistic superfluid neutron star...
We have developed a theoretical model and a numerical code for stationary rotating superfluid neutro...
We have developed a theoretical model and a numerical code for stationary rotating superfluid neutro...
International audienceWe have developed a theoretical model and a numerical code for stationary rota...
International audienceWe have developed a theoretical model and a numerical code for stationary rota...
International audienceWe have developed a theoretical model and a numerical code for stationary rota...
We describe recent progress in the numerical study of the structure of rapidly rotating superfluid n...
We describe recent progress in the numerical study of the structure of rapidly rotating superfluid n...
We study stationary axisymmetric configurations of a star model consisting of two barotropic fluids,...
We describe recent progress in the numerical study of the structure of rapidly rotating superfluid n...
We present a general formalism to treat slowly rotating general relativistic superfluid neutron star...
We study stationary axisymmetric configurations of a star model consisting of two barotropic fluids,...
International audienceWe describe recent progress in the modelling of realistic equilibrium configur...
We develop a formalism that can be used to model slowly rotating superfluid Newtonian neutron stars....
L'objectif de cette thèse est d'étudier différents aspects microscopiques et macroscopiques liés à l...
We present a general formalism to treat slowly rotating general relativistic superfluid neutron star...
We have developed a theoretical model and a numerical code for stationary rotating superfluid neutro...
We have developed a theoretical model and a numerical code for stationary rotating superfluid neutro...
International audienceWe have developed a theoretical model and a numerical code for stationary rota...
International audienceWe have developed a theoretical model and a numerical code for stationary rota...
International audienceWe have developed a theoretical model and a numerical code for stationary rota...
We describe recent progress in the numerical study of the structure of rapidly rotating superfluid n...
We describe recent progress in the numerical study of the structure of rapidly rotating superfluid n...
We study stationary axisymmetric configurations of a star model consisting of two barotropic fluids,...
We describe recent progress in the numerical study of the structure of rapidly rotating superfluid n...
We present a general formalism to treat slowly rotating general relativistic superfluid neutron star...
We study stationary axisymmetric configurations of a star model consisting of two barotropic fluids,...
International audienceWe describe recent progress in the modelling of realistic equilibrium configur...
We develop a formalism that can be used to model slowly rotating superfluid Newtonian neutron stars....
L'objectif de cette thèse est d'étudier différents aspects microscopiques et macroscopiques liés à l...
We present a general formalism to treat slowly rotating general relativistic superfluid neutron star...