<p>This paper investigates the global existence of smooth solutions near the equilibrium state <InlineEquation ID="IEq1"> <EquationSource Format="TEX">\((x_3,0)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mo stretchy="false">(</mo> <msub> <mi>x</mi> <mn>3</mn> </msub> <mo>,</mo> <mn>0</mn> <mo stretchy="false">)</mo> </mrow> </math></EquationSource> </InlineEquation> for the Cauchy problem of the incompressible MHD-type equations without magnetic diffusion in the whole space <InlineEquation ID="IEq2"> <EquationSource Format="TEX">\(\mathbb {R}^3\)</EquationSource> <EquationSource Format="MATHML"><math> <msup> <mrow> <mi mathvariant="double-struck">R</mi> </mrow> <mn>3</mn> </msup> </math></EquationSource> </InlineEquation>. In a prior work by Ren–Xiang–Zhang [Sci. China Math. 59 (2016), pp.1949-1974], the global existence and decay estimates of smooth solutions were established under a high regularity assumption on the initial data, namely <InlineEquation ID="IEq3"> <EquationSource Format="TEX">\((u_0,\nabla \psi _0)\in H^{14}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mrow> <mo stretchy="false">(</mo> <msub> <mi>u</mi> <mn>0</mn> </msub> <mo>,</mo> <mi mathvariant="normal">∇</mi> <msub> <mi>ψ</mi> <mn>0</mn> </msub> <mo stretchy="false">)</mo> </mrow> <mo>∈</mo> <msup> <mi>H</mi> <mn>14</mn> </msup> </mrow> </math></EquationSource> </InlineEquation>. In this paper, by employing the energy method with temporal weights in conjunction with anisotropic interpolation techniques, we prove the global existence of smooth solutions while significantly relaxing the regularity requirements on the initial data. As a by-product, we also derive explicit time decay rates for the solutions.</p>

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Global smooth solutions for 3D MHD-type equations in the absence of magnetic diffusion

  • Hao Liu

摘要

This paper investigates the global existence of smooth solutions near the equilibrium state \((x_3,0)\) ( x 3 , 0 ) for the Cauchy problem of the incompressible MHD-type equations without magnetic diffusion in the whole space \(\mathbb {R}^3\) R 3 . In a prior work by Ren–Xiang–Zhang [Sci. China Math. 59 (2016), pp.1949-1974], the global existence and decay estimates of smooth solutions were established under a high regularity assumption on the initial data, namely \((u_0,\nabla \psi _0)\in H^{14}\) ( u 0 , ψ 0 ) H 14 . In this paper, by employing the energy method with temporal weights in conjunction with anisotropic interpolation techniques, we prove the global existence of smooth solutions while significantly relaxing the regularity requirements on the initial data. As a by-product, we also derive explicit time decay rates for the solutions.