<p>We consider the Lorentz space <i>L</i><sub><i>q,τ</i></sub>(<InlineEquation ID="IEq2"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7807_Article_IEq2.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="23" /> </InlineMediaObject> <EquationSource Format="TEX">\({\mathbb{T}}^{m}\)</EquationSource> <EquationSource Format="MATHML"><math> <msup> <mrow> <mi mathvariant="double-struck">T</mi> </mrow> <mi>m</mi> </msup> </math></EquationSource> </InlineEquation>) of periodic functions of m variables and the class <InlineEquation ID="IEq3"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7807_Article_IEq1.gif" Format="GIF" Height="27" Rendition="HTML" Resolution="72" Type="Linedraw" Width="55" /> </InlineMediaObject> <EquationSource Format="TEX">\({\text{W}}_{q,\tau ,\theta }^{a,b\left(\cdot \right),\overline{r} }\)</EquationSource> <EquationSource Format="MATHML"><math> <msubsup> <mtext>W</mtext> <mrow> <mi>q</mi> <mo>,</mo> <mi>τ</mi> <mo>,</mo> <mi>θ</mi> </mrow> <mrow> <mi>a</mi> <mo>,</mo> <mi>b</mi> <mfenced close=")" open="("> <mo>·</mo> </mfenced> <mo>,</mo> <mover> <mi>r</mi> <mo>¯</mo> </mover> </mrow> </msubsup> </math></EquationSource> </InlineEquation> with 1 &lt; <i>q</i>, τ &lt; ∞, a &gt; 0, 1 &lt; θ ⩽ ∞, where <i>b</i>(<i>t</i>) is a weakly oscillating function on [1, ∞). We find a sufficient condition on a function <i>f</i> ∈ <InlineEquation ID="IEq4"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7807_Article_IEq4.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="32" /> </InlineMediaObject> <EquationSource Format="TEX">\({L}_{q,{\tau }_{1}}\)</EquationSource> <EquationSource Format="MATHML"><math> <msub> <mi>L</mi> <mrow> <mi>q</mi> <mo>,</mo> <msub> <mi>τ</mi> <mn>1</mn> </msub> </mrow> </msub> </math></EquationSource> </InlineEquation>(<InlineEquation ID="IEq5"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7807_Article_IEq2.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="23" /> </InlineMediaObject> <EquationSource Format="TEX">\({\mathbb{T}}^{m}\)</EquationSource> <EquationSource Format="MATHML"><math> <msup> <mrow> <mi mathvariant="double-struck">T</mi> </mrow> <mi>m</mi> </msup> </math></EquationSource> </InlineEquation>) to belong to the space <InlineEquation ID="IEq6"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7807_Article_IEq6.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="32" /> </InlineMediaObject> <EquationSource Format="TEX">\({L}_{q,{\tau }_{2}}\)</EquationSource> <EquationSource Format="MATHML"><math> <msub> <mi>L</mi> <mrow> <mi>q</mi> <mo>,</mo> <msub> <mi>τ</mi> <mn>2</mn> </msub> </mrow> </msub> </math></EquationSource> </InlineEquation>(<InlineEquation ID="IEq7"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7807_Article_IEq2.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="23" /> </InlineMediaObject> <EquationSource Format="TEX">\({\mathbb{T}}^{m}\)</EquationSource> <EquationSource Format="MATHML"><math> <msup> <mrow> <mi mathvariant="double-struck">T</mi> </mrow> <mi>m</mi> </msup> </math></EquationSource> </InlineEquation>) with 1 &lt; <i>q</i> &lt; <i>p</i> &lt; ∞, 1 &lt; τ<sub>1</sub> &lt; τ<sub>2</sub> &lt; ∞ and the embedding <InlineEquation ID="IEq8"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7807_Article_IEq8.gif" Format="GIF" Height="27" Rendition="HTML" Resolution="72" Type="Linedraw" Width="55" /> </InlineMediaObject> <EquationSource Format="TEX">\({\text{W}}_{q,{\tau }_{1},\theta }^{a,b\left(\cdot \right),\overline{r} }\)</EquationSource> <EquationSource Format="MATHML"><math> <msubsup> <mtext>W</mtext> <mrow> <mi>q</mi> <mo>,</mo> <msub> <mi>τ</mi> <mn>1</mn> </msub> <mo>,</mo> <mi>θ</mi> </mrow> <mrow> <mi>a</mi> <mo>,</mo> <mi>b</mi> <mfenced close=")" open="("> <mo>·</mo> </mfenced> <mo>,</mo> <mover> <mi>r</mi> <mo>¯</mo> </mover> </mrow> </msubsup> </math></EquationSource> </InlineEquation> ⊂ <InlineEquation ID="IEq9"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7807_Article_IEq6.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="32" /> </InlineMediaObject> <EquationSource Format="TEX">\({L}_{q,{\tau }_{2}}\)</EquationSource> <EquationSource Format="MATHML"><math> <msub> <mi>L</mi> <mrow> <mi>q</mi> <mo>,</mo> <msub> <mi>τ</mi> <mn>2</mn> </msub> </mrow> </msub> </math></EquationSource> </InlineEquation>(<InlineEquation ID="IEq10"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7807_Article_IEq2.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="23" /> </InlineMediaObject> <EquationSource Format="TEX">\({\mathbb{T}}^{m}\)</EquationSource> <EquationSource Format="MATHML"><math> <msup> <mrow> <mi mathvariant="double-struck">T</mi> </mrow> <mi>m</mi> </msup> </math></EquationSource> </InlineEquation>). We obtain upper bounds for the best M-term trigonometric approximations of functions of class <InlineEquation ID="IEq11"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7807_Article_IEq8.gif" Format="GIF" Height="27" Rendition="HTML" Resolution="72" Type="Linedraw" Width="55" /> </InlineMediaObject> <EquationSource Format="TEX">\({\text{W}}_{q,{\tau }_{1},\theta }^{a,b\left(\cdot \right),\overline{r} }\)</EquationSource> <EquationSource Format="MATHML"><math> <msubsup> <mtext>W</mtext> <mrow> <mi>q</mi> <mo>,</mo> <msub> <mi>τ</mi> <mn>1</mn> </msub> <mo>,</mo> <mi>θ</mi> </mrow> <mrow> <mi>a</mi> <mo>,</mo> <mi>b</mi> <mfenced close=")" open="("> <mo>·</mo> </mfenced> <mo>,</mo> <mover> <mi>r</mi> <mo>¯</mo> </mover> </mrow> </msubsup> </math></EquationSource> </InlineEquation> in the <InlineEquation ID="IEq12"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7807_Article_IEq6.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="32" /> </InlineMediaObject> <EquationSource Format="TEX">\({L}_{q,{\tau }_{2}}\)</EquationSource> <EquationSource Format="MATHML"><math> <msub> <mi>L</mi> <mrow> <mi>q</mi> <mo>,</mo> <msub> <mi>τ</mi> <mn>2</mn> </msub> </mrow> </msub> </math></EquationSource> </InlineEquation>(<InlineEquation ID="IEq13"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7807_Article_IEq2.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="23" /> </InlineMediaObject> <EquationSource Format="TEX">\({\mathbb{T}}^{m}\)</EquationSource> <EquationSource Format="MATHML"><math> <msup> <mrow> <mi mathvariant="double-struck">T</mi> </mrow> <mi>m</mi> </msup> </math></EquationSource> </InlineEquation>)-norm in the case 1 &lt; <i>q</i> &lt; 2 &lt; <i>p</i> &lt; ∞ under some conditions on a, τ<sub>1</sub>, τ<sub>2</sub>. For some values of a, τ<sub>1</sub>, τ<sub>2</sub>, the accuracy of the upper bound is established.</p>

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Estimates for the Best M-Term Approximations of Functions of Class \({\text{W}}_{q,\tau ,\theta }^{a,b\left(\cdot \right),\overline{r} }\) in the Lorentz Space

  • Aigul Myrzagaliyeva,
  • Gabdolla Akishev

摘要

We consider the Lorentz space Lq,τ( \({\mathbb{T}}^{m}\) T m ) of periodic functions of m variables and the class \({\text{W}}_{q,\tau ,\theta }^{a,b\left(\cdot \right),\overline{r} }\) W q , τ , θ a , b · , r ¯ with 1 < q, τ < ∞, a > 0, 1 < θ ⩽ ∞, where b(t) is a weakly oscillating function on [1, ∞). We find a sufficient condition on a function f \({L}_{q,{\tau }_{1}}\) L q , τ 1 ( \({\mathbb{T}}^{m}\) T m ) to belong to the space \({L}_{q,{\tau }_{2}}\) L q , τ 2 ( \({\mathbb{T}}^{m}\) T m ) with 1 < q < p < ∞, 1 < τ1 < τ2 < ∞ and the embedding \({\text{W}}_{q,{\tau }_{1},\theta }^{a,b\left(\cdot \right),\overline{r} }\) W q , τ 1 , θ a , b · , r ¯ \({L}_{q,{\tau }_{2}}\) L q , τ 2 ( \({\mathbb{T}}^{m}\) T m ). We obtain upper bounds for the best M-term trigonometric approximations of functions of class \({\text{W}}_{q,{\tau }_{1},\theta }^{a,b\left(\cdot \right),\overline{r} }\) W q , τ 1 , θ a , b · , r ¯ in the \({L}_{q,{\tau }_{2}}\) L q , τ 2 ( \({\mathbb{T}}^{m}\) T m )-norm in the case 1 < q < 2 < p < ∞ under some conditions on a, τ1, τ2. For some values of a, τ1, τ2, the accuracy of the upper bound is established.