<p>Let <InlineEquation ID="IEq1"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7878_Article_IEq1.gif" Format="GIF" Height="31" Rendition="HTML" Resolution="72" Type="Linedraw" Width="137" /> </InlineMediaObject> <EquationSource Format="TEX">\(f(z) = \displaystyle \sum \nolimits _{k = 1}^{\infty }f_k z^{k}\)</EquationSource> <EquationSource Format="MATHML"><math> <mstyle displaystyle="true" scriptlevel="0"> <mrow> <mi>f</mi> <mrow> <mo stretchy="false">(</mo> <mi>z</mi> <mo stretchy="false">)</mo> </mrow> <mo>=</mo> <msubsup> <mo>∑</mo> <mrow> <mi>k</mi> <mo>=</mo> <mn>1</mn> </mrow> <mi>∞</mi> </msubsup> <msub> <mi>f</mi> <mi>k</mi> </msub> <msup> <mi>z</mi> <mi>k</mi> </msup> </mrow> </mstyle> </math></EquationSource> </InlineEquation> be an entire transcendental function, let <InlineEquation ID="IEq2"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7878_Article_IEq2.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="31" /> </InlineMediaObject> <EquationSource Format="TEX">\((\lambda _n)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mo stretchy="false">(</mo> <msub> <mi>λ</mi> <mi>n</mi> </msub> <mo stretchy="false">)</mo> </mrow> </math></EquationSource> </InlineEquation> be a sequence of positive numbers increasing to <InlineEquation ID="IEq3"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7878_Article_IEq3.gif" Format="GIF" Height="15" Rendition="HTML" Resolution="72" Type="Linedraw" Width="36" /> </InlineMediaObject> <EquationSource Format="TEX">\( + \infty ,\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mo>+</mo> <mi>∞</mi> <mo>,</mo> </mrow> </math></EquationSource> </InlineEquation> and let a series <InlineEquation ID="IEq4"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7878_Article_IEq4.gif" Format="GIF" Height="31" Rendition="HTML" Resolution="72" Type="Linedraw" Width="172" /> </InlineMediaObject> <EquationSource Format="TEX">\(A(z) = \displaystyle \sum \nolimits _{n = 1}^{\infty }a_nf(\lambda _n z)\)</EquationSource> <EquationSource Format="MATHML"><math> <mstyle displaystyle="true" scriptlevel="0"> <mrow> <mi>A</mi> <mrow> <mo stretchy="false">(</mo> <mi>z</mi> <mo stretchy="false">)</mo> </mrow> <mo>=</mo> <msubsup> <mo>∑</mo> <mrow> <mi>n</mi> <mo>=</mo> <mn>1</mn> </mrow> <mi>∞</mi> </msubsup> <msub> <mi>a</mi> <mi>n</mi> </msub> <mi>f</mi> <mrow> <mo stretchy="false">(</mo> <msub> <mi>λ</mi> <mi>n</mi> </msub> <mi>z</mi> <mo stretchy="false">)</mo> </mrow> </mrow> </mstyle> </math></EquationSource> </InlineEquation> be regularly convergent in <InlineEquation ID="IEq5"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7878_Article_IEq5.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="128" /> </InlineMediaObject> <EquationSource Format="TEX">\({\mathbb {D}} = \{z:|z|&lt;1\}.\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi mathvariant="double-struck">D</mi> <mo>=</mo> <mo stretchy="false">{</mo> <mi>z</mi> <mo>:</mo> <mo stretchy="false">|</mo> <mi>z</mi> <mo stretchy="false">|</mo> <mo>&lt;</mo> <mn>1</mn> <mo stretchy="false">}</mo> <mo>.</mo> </mrow> </math></EquationSource> </InlineEquation> We study the starlikeness and convexity of the function <i>A</i>. For example, if <InlineEquation ID="IEq6"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7878_Article_IEq6.gif" Format="GIF" Height="31" Rendition="HTML" Resolution="72" Type="Linedraw" Width="170" /> </InlineMediaObject> <EquationSource Format="TEX">\(\displaystyle \sum \nolimits _{n = 1}^{\infty }\lambda ^{-\tau }_n = T&lt; + \infty ,\)</EquationSource> <EquationSource Format="MATHML"><math> <mstyle displaystyle="true" scriptlevel="0"> <mrow> <msubsup> <mo>∑</mo> <mrow> <mi>n</mi> <mo>=</mo> <mn>1</mn> </mrow> <mi>∞</mi> </msubsup> <msubsup> <mi>λ</mi> <mi>n</mi> <mrow> <mo>-</mo> <mi>τ</mi> </mrow> </msubsup> <mo>=</mo> <mi>T</mi> <mo>&lt;</mo> <mo>+</mo> <mi>∞</mi> <mo>,</mo> </mrow> </mstyle> </math></EquationSource> </InlineEquation> <InlineEquation ID="IEq7"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7878_Article_IEq7.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="110" /> </InlineMediaObject> <EquationSource Format="TEX">\(\ln |a_n|\le -e\lambda _n,\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mrow> <mo>ln</mo> <mo stretchy="false">|</mo> </mrow> <msub> <mi>a</mi> <mi>n</mi> </msub> <mrow> <mo stretchy="false">|</mo> <mo>≤</mo> <mo>-</mo> <mi>e</mi> </mrow> <msub> <mi>λ</mi> <mi>n</mi> </msub> <mo>,</mo> </mrow> </math></EquationSource> </InlineEquation> and <InlineEquation ID="IEq8"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7878_Article_IEq8.gif" Format="GIF" Height="33" Rendition="HTML" Resolution="72" Type="Linedraw" Width="318" /> </InlineMediaObject> <EquationSource Format="TEX">\(T\displaystyle \sum \nolimits _{k = 2}^{\infty }k|f_k| (k + \tau )^{k + \tau }\le \left| f_1\displaystyle \sum \nolimits _{n = 1}^{\infty }a_n\lambda _n\right| ,\)</EquationSource> <EquationSource Format="MATHML"><math> <mstyle displaystyle="true" scriptlevel="0"> <mrow> <mi>T</mi> <msubsup> <mo>∑</mo> <mrow> <mi>k</mi> <mo>=</mo> <mn>2</mn> </mrow> <mi>∞</mi> </msubsup> <mi>k</mi> <mrow> <mo stretchy="false">|</mo> <msub> <mi>f</mi> <mi>k</mi> </msub> <mo stretchy="false">|</mo> </mrow> <msup> <mrow> <mo stretchy="false">(</mo> <mi>k</mi> <mo>+</mo> <mi>τ</mi> <mo stretchy="false">)</mo> </mrow> <mrow> <mi>k</mi> <mo>+</mo> <mi>τ</mi> </mrow> </msup> <mo>≤</mo> <mfenced close="|" open="|"> <mstyle displaystyle="true" scriptlevel="0"> <msub> <mi>f</mi> <mn>1</mn> </msub> <msubsup> <mo>∑</mo> <mrow> <mi>n</mi> <mo>=</mo> <mn>1</mn> </mrow> <mi>∞</mi> </msubsup> <msub> <mi>a</mi> <mi>n</mi> </msub> <msub> <mi>λ</mi> <mi>n</mi> </msub> </mstyle> </mfenced> <mo>,</mo> </mrow> </mstyle> </math></EquationSource> </InlineEquation> then the function <i>A</i> is starlike. It is proved that, under certain conditions imposed on the parameters, the differential equation <InlineEquation ID="IEq9"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7878_Article_IEq9.gif" Format="GIF" Height="20" Rendition="HTML" Resolution="72" Type="Linedraw" Width="344" /> </InlineMediaObject> <EquationSource Format="TEX">\(z^2w'' + (\beta _0 z^2 + \beta _1z)w' + (\gamma _0z^2 + \gamma _1 z + \gamma _2) w = 0\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msup> <mi>z</mi> <mn>2</mn> </msup> <msup> <mi>w</mi> <mrow> <mo>′</mo> <mo>′</mo> </mrow> </msup> <mo>+</mo> <mrow> <mo stretchy="false">(</mo> <msub> <mi>β</mi> <mn>0</mn> </msub> <msup> <mi>z</mi> <mn>2</mn> </msup> <mo>+</mo> <msub> <mi>β</mi> <mn>1</mn> </msub> <mi>z</mi> <mo stretchy="false">)</mo> </mrow> <msup> <mi>w</mi> <mo>′</mo> </msup> <mo>+</mo> <mrow> <mo stretchy="false">(</mo> <msub> <mi>γ</mi> <mn>0</mn> </msub> <msup> <mi>z</mi> <mn>2</mn> </msup> <mo>+</mo> <msub> <mi>γ</mi> <mn>1</mn> </msub> <mi>z</mi> <mo>+</mo> <msub> <mi>γ</mi> <mn>2</mn> </msub> <mo stretchy="false">)</mo> </mrow> <mi>w</mi> <mo>=</mo> <mn>0</mn> </mrow> </math></EquationSource> </InlineEquation> has an entire solution <i>A</i>,&#xa0; which is starlike or convex in <InlineEquation ID="IEq10"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10958_2025_7878_Article_IEq10.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="18" /> </InlineMediaObject> <EquationSource Format="TEX">\({\mathbb {D}}.\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi mathvariant="double-struck">D</mi> <mo>.</mo> </mrow> </math></EquationSource> </InlineEquation></p>

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ON THE GEOMETRIC PROPERTIES OF SERIES IN SYSTEMS OF FUNCTIONS

  • Myroslav Sheremeta

摘要

Let \(f(z) = \displaystyle \sum \nolimits _{k = 1}^{\infty }f_k z^{k}\) f ( z ) = k = 1 f k z k be an entire transcendental function, let \((\lambda _n)\) ( λ n ) be a sequence of positive numbers increasing to \( + \infty ,\) + , and let a series \(A(z) = \displaystyle \sum \nolimits _{n = 1}^{\infty }a_nf(\lambda _n z)\) A ( z ) = n = 1 a n f ( λ n z ) be regularly convergent in \({\mathbb {D}} = \{z:|z|<1\}.\) D = { z : | z | < 1 } . We study the starlikeness and convexity of the function A. For example, if \(\displaystyle \sum \nolimits _{n = 1}^{\infty }\lambda ^{-\tau }_n = T< + \infty ,\) n = 1 λ n - τ = T < + , \(\ln |a_n|\le -e\lambda _n,\) ln | a n | - e λ n , and \(T\displaystyle \sum \nolimits _{k = 2}^{\infty }k|f_k| (k + \tau )^{k + \tau }\le \left| f_1\displaystyle \sum \nolimits _{n = 1}^{\infty }a_n\lambda _n\right| ,\) T k = 2 k | f k | ( k + τ ) k + τ f 1 n = 1 a n λ n , then the function A is starlike. It is proved that, under certain conditions imposed on the parameters, the differential equation \(z^2w'' + (\beta _0 z^2 + \beta _1z)w' + (\gamma _0z^2 + \gamma _1 z + \gamma _2) w = 0\) z 2 w + ( β 0 z 2 + β 1 z ) w + ( γ 0 z 2 + γ 1 z + γ 2 ) w = 0 has an entire solution A,  which is starlike or convex in \({\mathbb {D}}.\) D .