We consider the Cauchy problem of isentropic compressible magnetohydrodynamic equations with large potential force in R 3 . When the initial data ( 0 , u 0 , H 0 ) is of small energy, we investigate the global well-posedness of classical solutions where the flow density is allowed to contain vacuum states.
KEYWORDSCauchy problem, compressible magnetohydrodynamic equations, global classical solution, vacuum divH = 0, (1.4) with x = (x 1 , x 2 , x 3 ) ∈ R 3 , t ≥ 0. The unknown functions , u = (u 1 , u 2 , u 3 ), P, H = ( H 1 , H 2 , H 3 ), and f = (f 1 , f 2 , f 3 ) represent the density, the velocity, the pressure, the magnetic field, and the (assigned) external force field, respectively. In addition, the pressure is given by P( ) = a with a > 0, > 1, the viscosity coefficients and satisfy > 0, 3 + 2 ≥ 0, (1.5)Math Meth Appl Sci. 2019;42:747-766. wileyonlinelibrary.com/journal/mma