<p>We study the existence of forward self-similar solutions to the magnetohydrodynamic type (MHD type) system in the half space <InlineEquation ID="IEq1"> <EquationSource Format="TEX">\(\mathbb {R}^{3}_{+}\)</EquationSource> <EquationSource Format="MATHML"><math> <msubsup> <mrow> <mi mathvariant="double-struck">R</mi> </mrow> <mo>+</mo> <mn>3</mn> </msubsup> </math></EquationSource> </InlineEquation>. For any self-similar initial data belonging to <InlineEquation ID="IEq2"> <EquationSource Format="TEX">\(L^{\infty }_{loc}(\overline{\mathbb {R}^{3}_{+}}\setminus \{0\})\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msubsup> <mi>L</mi> <mrow> <mi mathvariant="italic">loc</mi> </mrow> <mi>∞</mi> </msubsup> <mrow> <mo stretchy="false">(</mo> <mover> <msubsup> <mrow> <mi mathvariant="double-struck">R</mi> </mrow> <mo>+</mo> <mn>3</mn> </msubsup> <mo>¯</mo> </mover> <mo lspace="0.15em" rspace="0.15em" stretchy="false">\</mo> <mrow> <mo stretchy="false">{</mo> <mn>0</mn> <mo stretchy="false">}</mo> </mrow> <mo stretchy="false">)</mo> </mrow> </mrow> </math></EquationSource> </InlineEquation>, we employ a compactness argument and Leray–Schauder theorem to construct a forward self-similar solution to the MHD type system that is smooth in <InlineEquation ID="IEq3"> <EquationSource Format="TEX">\(\mathbb {R}^{3}_{+}\times (0,\infty )\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msubsup> <mrow> <mi mathvariant="double-struck">R</mi> </mrow> <mo>+</mo> <mn>3</mn> </msubsup> <mo>×</mo> <mrow> <mo stretchy="false">(</mo> <mn>0</mn> <mo>,</mo> <mi>∞</mi> <mo stretchy="false">)</mo> </mrow> </mrow> </math></EquationSource> </InlineEquation>. Moreover, our results extend the existence theorem of Korobkov and Tsai [<CitationRef CitationID="CR25">25</CitationRef>] for the Navier–Stokes equations by relaxing the regularity requirement on the initial data from <InlineEquation ID="IEq4"> <EquationSource Format="TEX">\(C^{1}_{loc}(\overline{\mathbb {R}^{3}_{+}}\setminus \{0\})\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msubsup> <mi>C</mi> <mrow> <mi mathvariant="italic">loc</mi> </mrow> <mn>1</mn> </msubsup> <mrow> <mo stretchy="false">(</mo> <mover> <msubsup> <mrow> <mi mathvariant="double-struck">R</mi> </mrow> <mo>+</mo> <mn>3</mn> </msubsup> <mo>¯</mo> </mover> <mo lspace="0.15em" rspace="0.15em" stretchy="false">\</mo> <mrow> <mo stretchy="false">{</mo> <mn>0</mn> <mo stretchy="false">}</mo> </mrow> <mo stretchy="false">)</mo> </mrow> </mrow> </math></EquationSource> </InlineEquation> to <InlineEquation ID="IEq5"> <EquationSource Format="TEX">\(L^{\infty }_{loc}(\overline{\mathbb {R}^{3}_{+}}\setminus \{0\})\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msubsup> <mi>L</mi> <mrow> <mi mathvariant="italic">loc</mi> </mrow> <mi>∞</mi> </msubsup> <mrow> <mo stretchy="false">(</mo> <mover> <msubsup> <mrow> <mi mathvariant="double-struck">R</mi> </mrow> <mo>+</mo> <mn>3</mn> </msubsup> <mo>¯</mo> </mover> <mo lspace="0.15em" rspace="0.15em" stretchy="false">\</mo> <mrow> <mo stretchy="false">{</mo> <mn>0</mn> <mo stretchy="false">}</mo> </mrow> <mo stretchy="false">)</mo> </mrow> </mrow> </math></EquationSource> </InlineEquation>.</p>

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Forward Self-similar Solutions to the MHD Type System in the Half Space

  • Yifan Yang

摘要

We study the existence of forward self-similar solutions to the magnetohydrodynamic type (MHD type) system in the half space \(\mathbb {R}^{3}_{+}\) R + 3 . For any self-similar initial data belonging to \(L^{\infty }_{loc}(\overline{\mathbb {R}^{3}_{+}}\setminus \{0\})\) L loc ( R + 3 ¯ \ { 0 } ) , we employ a compactness argument and Leray–Schauder theorem to construct a forward self-similar solution to the MHD type system that is smooth in \(\mathbb {R}^{3}_{+}\times (0,\infty )\) R + 3 × ( 0 , ) . Moreover, our results extend the existence theorem of Korobkov and Tsai [25] for the Navier–Stokes equations by relaxing the regularity requirement on the initial data from \(C^{1}_{loc}(\overline{\mathbb {R}^{3}_{+}}\setminus \{0\})\) C loc 1 ( R + 3 ¯ \ { 0 } ) to \(L^{\infty }_{loc}(\overline{\mathbb {R}^{3}_{+}}\setminus \{0\})\) L loc ( R + 3 ¯ \ { 0 } ) .