The Equations of Magnetohydrodynamics: On the Interaction Between Matter and Radiation in the Evolution of Gaseous Stars

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Serrin-Type Blowup Criterion for Viscous, Compressible, and Heat Conducting Navier-Stokes and Magnetohydrodynamic Flows (2012, background): “1) by physicists and mathematicians because of their physical importance, complexity, rich phenomena, and mathematical challenges; see [4,5,7,8,10,11,15,21,22,24,25,27,28,36,37] and the references”
Global Existence and Large-Time Behavior of Solutions to the Three-Dimensional Equations of Compressible Magnetohydrodynamic Flows (2009, background): “2) There have been a lot of studies on MHD by physicists and mathematicians because of its physical importance, complexity, rich phenomena, and mathematical challenges; see [3, 4, 5, 7, 12, 15, 19, 25] and the references cited therein.”
Weak–Strong Uniqueness Property for the Full Navier–Stokes–Fourier System (2011, background): “6) based on Second law of thermodynamics was introduced in [7].”
Global Solutions to the Three-Dimensional Full Compressible Magnetohydrodynamic Flows (2008, methodology): “10) We note that in [6], Ducomet and Feireisl studied, using the entropy method, the full compressible MHD equations with an additional Poisson’s equation under the assumption that the viscosity coefficients depend on the temperature and the magnetic field, and the pressure behaves like the power la”