<p>In this paper, we study global well-posedness and temporal decay for the generalized magneto-hydrodynamic equations with some large initial data in Besov type spaces. Making full use of algebraic structure of equations, we prove that there exist two positive constants <InlineEquation ID="IEq1"> <EquationSource Format="TEX">\(c_0\)</EquationSource> </InlineEquation> and <InlineEquation ID="IEq2"> <EquationSource Format="TEX">\(C_0\)</EquationSource> </InlineEquation> such that if the initial velocity field <InlineEquation ID="IEq3"> <EquationSource Format="TEX">\(U_0\)</EquationSource> </InlineEquation> and the initial magnetic field <InlineEquation ID="IEq4"> <EquationSource Format="TEX">\(B_0\)</EquationSource> </InlineEquation> satisfy one of the following conditions: <Equation ID="Equ72"> <EquationSource Format="TEX">\(\begin{aligned} \big \Vert U_0-B_0\big \Vert _{\dot{B}^{1-2\alpha +\frac{d}{p}}_{p,1}}\exp \big \{C_0 \big \Vert U_0+B_0\big \Vert _{\dot{B}^{1-2\alpha +\frac{d}{q}}_{q,1}} \big \}\le c_0 \end{aligned}\)</EquationSource> </Equation>or <Equation ID="Equ73"> <EquationSource Format="TEX">\(\begin{aligned} \big \Vert U_0+B_0\big \Vert _{\dot{B}^{1-2\alpha +\frac{d}{q}}_{q,1}}\exp \big \{C_0 \big \Vert U_0-B_0\big \Vert _{\dot{B}^{1-2\alpha +\frac{d}{p}}_{p,1}} \big \}\le c_0, \end{aligned}\)</EquationSource> </Equation>then the generalized magneto-hydrodynamic equations admits a unique global solution. In addition, we establish the optimal decay rates of global solutions by using the Fourier splitting approach and the interpolation techniques.</p>

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Global existence and decay rates of large solutions for the generalized MHD equations in Besov type spaces

  • Zhongbo Cai,
  • Jihong Zhao

摘要

In this paper, we study global well-posedness and temporal decay for the generalized magneto-hydrodynamic equations with some large initial data in Besov type spaces. Making full use of algebraic structure of equations, we prove that there exist two positive constants \(c_0\) and \(C_0\) such that if the initial velocity field \(U_0\) and the initial magnetic field \(B_0\) satisfy one of the following conditions: \(\begin{aligned} \big \Vert U_0-B_0\big \Vert _{\dot{B}^{1-2\alpha +\frac{d}{p}}_{p,1}}\exp \big \{C_0 \big \Vert U_0+B_0\big \Vert _{\dot{B}^{1-2\alpha +\frac{d}{q}}_{q,1}} \big \}\le c_0 \end{aligned}\) or \(\begin{aligned} \big \Vert U_0+B_0\big \Vert _{\dot{B}^{1-2\alpha +\frac{d}{q}}_{q,1}}\exp \big \{C_0 \big \Vert U_0-B_0\big \Vert _{\dot{B}^{1-2\alpha +\frac{d}{p}}_{p,1}} \big \}\le c_0, \end{aligned}\) then the generalized magneto-hydrodynamic equations admits a unique global solution. In addition, we establish the optimal decay rates of global solutions by using the Fourier splitting approach and the interpolation techniques.