<p>This paper investigates the space-time decay properties of solutions to the compressible Navier-Stokes equations with hyperbolic heat conduction in the whole space <InlineEquation ID="IEq1"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="40840_2025_1916_Article_IEq1.gif" Format="GIF" Height="16" Rendition="HTML" Resolution="72" Type="Linedraw" Width="18" /> </InlineMediaObject> <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>. By employing weighted Sobolev space techniques and interpolation methods, we prove that the space–time decay rate of the <i>k</i>-th order spatial derivative (<InlineEquation ID="IEq2"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="40840_2025_1916_Article_IEq2.gif" Format="GIF" Height="16" Rendition="HTML" Resolution="72" Type="Linedraw" Width="81" /> </InlineMediaObject> <EquationSource Format="TEX">\(0\le k \le N\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mn>0</mn> <mo>≤</mo> <mi>k</mi> <mo>≤</mo> <mi>N</mi> </mrow> </math></EquationSource> </InlineEquation>) of the strong solution in the weighted Lebesgue space <InlineEquation ID="IEq3"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="40840_2025_1916_Article_IEq3.gif" Format="GIF" Height="22" Rendition="HTML" Resolution="72" Type="Linedraw" Width="21" /> </InlineMediaObject> <EquationSource Format="TEX">\( L_\gamma ^2 \)</EquationSource> <EquationSource Format="MATHML"><math> <msubsup> <mi>L</mi> <mi>γ</mi> <mn>2</mn> </msubsup> </math></EquationSource> </InlineEquation> is <InlineEquation ID="IEq4"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="40840_2025_1916_Article_IEq4.gif" Format="GIF" Height="20" Rendition="HTML" Resolution="72" Type="Linedraw" Width="58" /> </InlineMediaObject> <EquationSource Format="TEX">\(t^{-\frac{3}{4}-\frac{k}{2}+\gamma }\)</EquationSource> <EquationSource Format="MATHML"><math> <msup> <mi>t</mi> <mrow> <mo>-</mo> <mfrac> <mn>3</mn> <mn>4</mn> </mfrac> <mo>-</mo> <mfrac> <mi>k</mi> <mn>2</mn> </mfrac> <mo>+</mo> <mi>γ</mi> </mrow> </msup> </math></EquationSource> </InlineEquation> for any integer <InlineEquation ID="IEq5"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="40840_2025_1916_Article_IEq5.gif" Format="GIF" Height="16" Rendition="HTML" Resolution="72" Type="Linedraw" Width="48" /> </InlineMediaObject> <EquationSource Format="TEX">\(N\ge 3\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>N</mi> <mo>≥</mo> <mn>3</mn> </mrow> </math></EquationSource> </InlineEquation>. The key contribution lies in developing a unified framework that connects weighted energy estimates with time decay analysis, enabling simultaneous capture of both spatial regularity and temporal decay characteristics. This result improves previous decay estimates and provides a complete description of the solution’s asymptotic behavior for the compressible Navier-Stokes equations with hyperbolic heat conduction.</p>

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Space–Time Decay Rates of the Compressible Navier-Stokes Equations with Hyperbolic Heat Conduction

  • Tianzheng Yang,
  • Yinghui Zhang

摘要

This paper investigates the space-time decay properties of solutions to the compressible Navier-Stokes equations with hyperbolic heat conduction in the whole space \({\mathbb {R}}^3\) R 3 . By employing weighted Sobolev space techniques and interpolation methods, we prove that the space–time decay rate of the k-th order spatial derivative ( \(0\le k \le N\) 0 k N ) of the strong solution in the weighted Lebesgue space \( L_\gamma ^2 \) L γ 2 is \(t^{-\frac{3}{4}-\frac{k}{2}+\gamma }\) t - 3 4 - k 2 + γ for any integer \(N\ge 3\) N 3 . The key contribution lies in developing a unified framework that connects weighted energy estimates with time decay analysis, enabling simultaneous capture of both spatial regularity and temporal decay characteristics. This result improves previous decay estimates and provides a complete description of the solution’s asymptotic behavior for the compressible Navier-Stokes equations with hyperbolic heat conduction.