Global classical solution to 3D compressible magnetohydrodynamic equations with large initial data and vacuum

preprint2015arXivOpen access

Abstract

In this paper, we study the Cauchy problem of the isentropic compressible magnetohydrodynamic equations in R3\mathbb{R}^{3}. When (γ−1)16E012(γ-1)^{\frac{1}{6}}E_{0}^{\frac{1}{2}}, together with the ∥H0∥L2\|H_{0}\|_{L^{2}}, is suitably small, a result on the existence of global classical solutions is obtained. It should be pointed out that the initial energy E0E_{0} except the L2L^{2}- norm of H0H_{0} can be large as γγ goes to 1, and that throughout the proof of the theorem in the present paper, we make no restriction upon the initial data (ρ0,u0)(ρ_{0},u_{0}). Our result improves the one established by Li-Xu-Zhang in \cite{H.L. L}, where, with small initial engergy, the existence of classical solution was proved.

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