Analysis of a model in solar magnetohydrostatics.
Diffusion classique et quantique par un trou noir en formation
Effect of the radiative damping on magnetohydrodynamic waves in an isothermal medium.
Groupes conformes en relativité générale
Multiple solutions for inhomogeneous nonlinear elliptic problems arising in astrophyscs.
Numerical hydrodynamics and magnetohydrodynamics in general relativity.
Numerical simulations in astrophysics: Supernovae explosions, magnetorotational model and neutrino emission.
On resistive dissipation of Alfvén waves in an isothermal atmosphere.
On the linear force-free fields in bounded and unbounded three-dimensional domains
Linear Force-free (or Beltrami) fields are three-components divergence-free fields solutions of the equation curlB = αB, where α is a real number. Such fields appear in many branches of physics like astrophysics, fluid mechanics, electromagnetics and plasma physics. In this paper, we deal with some related boundary value problems in multiply-connected bounded domains, in half-cylindrical domains and in exterior domains.
On the mathematical structure of test relativistic magnetofluiddynamics
On the stability of stellar structure in one dimension II : the reactive case
Remarks on inhomogeneous elliptic problems arising in astrophysics.
Rotating shallow water modeling of planetary, astrophysical and plasma vortical structures. (Plasma transport across a magnetic field, model of the Jupiter's GRS, prediction of existence of giant vortices in spiral galaxies).
Thermal conductivity and dynamic pressure in extended thermodynamics of chemically reacting mixture of gases