Add to ORKGAbstract. The existence of solutions of the equations for a self-gravitating fluid with prescribed angular velocity law is proved. The conditions on the angular velocity are nearly optimal. The system is formulated as a variational problem and concentration-compactness methods are used to prove the existence of minimizers of the energy functional. 1
We prove existence of rotating star solutions which are steady-state solutions of the compressible i...
We obtain an approximate global stationary and axisymmetric solution of Einstein's equations which c...
The paper considers properties of the normal modes of linear pulsation of perfect-fluid rotating sta...
Abstract. We study a two dimensional system in solid rotation at constant angular velocity driven by...
AbstractIn this paper we classify the free boundary associated to equilibrium configurations of comp...
Abstract. In this paper we classify the free boundary associated to equilib-rium configurations of c...
AbstractThe equations for axisymmetric self-gravitating rotating fluid have been studied extensively...
AbstractA variational method is used to study the shape of a self-gravitating fluid mass rotating wi...
Cataldo has found all rigidly rotating self-gravitating perfect fluid solutions in 2+1 dimensions wi...
In this paper, we study the steady solutions of Euler-Poisson equations in bounded domains with pres...
We study a three dimensional continuous model of gravitating matter rotating at constant angular vel...
We prove existence of rotating star solutions which are steady-state solutions of the compressible i...
AbstractIn this paper, minimization problems in L1(R3) are considered. These problems arise in astro...
We establish sufficient conditions for uniqueness in the context of an energy minimisation property ...
International audienceWe study spherically symmetric solutions to the Einstein–Euler equations which...
We prove existence of rotating star solutions which are steady-state solutions of the compressible i...
We obtain an approximate global stationary and axisymmetric solution of Einstein's equations which c...
The paper considers properties of the normal modes of linear pulsation of perfect-fluid rotating sta...
Abstract. We study a two dimensional system in solid rotation at constant angular velocity driven by...
AbstractIn this paper we classify the free boundary associated to equilibrium configurations of comp...
Abstract. In this paper we classify the free boundary associated to equilib-rium configurations of c...
AbstractThe equations for axisymmetric self-gravitating rotating fluid have been studied extensively...
AbstractA variational method is used to study the shape of a self-gravitating fluid mass rotating wi...
Cataldo has found all rigidly rotating self-gravitating perfect fluid solutions in 2+1 dimensions wi...
In this paper, we study the steady solutions of Euler-Poisson equations in bounded domains with pres...
We study a three dimensional continuous model of gravitating matter rotating at constant angular vel...
We prove existence of rotating star solutions which are steady-state solutions of the compressible i...
AbstractIn this paper, minimization problems in L1(R3) are considered. These problems arise in astro...
We establish sufficient conditions for uniqueness in the context of an energy minimisation property ...
International audienceWe study spherically symmetric solutions to the Einstein–Euler equations which...
We prove existence of rotating star solutions which are steady-state solutions of the compressible i...
We obtain an approximate global stationary and axisymmetric solution of Einstein's equations which c...
The paper considers properties of the normal modes of linear pulsation of perfect-fluid rotating sta...