<p>In this paper, we establish the initial Taylor-Maclaurin coefficients for normalized analytic functions <InlineEquation ID="IEq1"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="41478_2025_893_Article_IEq1.gif" Format="GIF" Height="17" Rendition="HTML" Resolution="72" Type="Linedraw" Width="14" /> </InlineMediaObject> <EquationSource Format="TEX">\(f\,\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>f</mi> <mspace width="0.166667em" /> </mrow> </math></EquationSource> </InlineEquation> in the open unit disk. We also assume that <InlineEquation ID="IEq2"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="41478_2025_893_Article_IEq1.gif" Format="GIF" Height="17" Rendition="HTML" Resolution="72" Type="Linedraw" Width="14" /> </InlineMediaObject> <EquationSource Format="TEX">\(f\,\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>f</mi> <mspace width="0.166667em" /> </mrow> </math></EquationSource> </InlineEquation> and its inverse <InlineEquation ID="IEq3"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="41478_2025_893_Article_IEq3.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="62" /> </InlineMediaObject> <EquationSource Format="TEX">\(g=f\,^{-1}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>g</mi> <mo>=</mo> <mi>f</mi> <mmultiscripts> <mspace width="0.166667em" /> <mrow /> <mrow> <mo>-</mo> <mn>1</mn> </mrow> </mmultiscripts> </mrow> </math></EquationSource> </InlineEquation> satisfy the following conditions <Equation ID="Equ55"> <MediaObject> <ImageObject Color="BlackWhite" FileRef="41478_2025_893_Article_Equ55.gif" Format="GIF" Height="44" Rendition="HTML" Resolution="72" Type="Linedraw" Width="627" /> </MediaObject> <EquationSource Format="TEX">\(\begin{aligned} \rm{e}^{\rm{i}\phi }\left[ f\,^{\prime }\,(z)\right] ^{\tau }\left[ \frac{z}{f\,(z)}\right] ^{\nu }&amp;\prec \psi (z)\cos \phi +\rm{i}\sin \phi \quad \text {and} \quad \rm{e}^{\rm{i}\phi }\left[ g'(z)\right] ^{\tau }\left[ \frac{z}{g(z)}\right] ^{\nu }&amp;\prec \psi (z)\cos \phi +\rm{i}\sin \phi , \end{aligned}\)</EquationSource> <EquationSource Format="MATHML"><math display="block"> <mrow> <mtable> <mtr> <mtd columnalign="right"> <mrow> <msup> <mrow> <mi mathvariant="normal">e</mi> </mrow> <mrow> <mi mathvariant="normal">i</mi> <mi>ϕ</mi> </mrow> </msup> <mmultiscripts> <mfenced close="]" open="["> <mi mathvariant="normal">f</mi> <mmultiscripts> <mspace width="0.166667em" /> <mrow /> <mo>′</mo> </mmultiscripts> <mspace width="0.166667em" /> <mrow> <mo stretchy="false">(</mo> <mi mathvariant="normal">z</mi> <mo stretchy="false">)</mo> </mrow> </mfenced> <mrow /> <mi>τ</mi> </mmultiscripts> <msup> <mfenced close="]" open="["> <mfrac> <mi mathvariant="normal">z</mi> <mrow> <mi mathvariant="normal">f</mi> <mspace width="0.166667em" /> <mo stretchy="false">(</mo> <mi mathvariant="normal">z</mi> <mo stretchy="false">)</mo> </mrow> </mfrac> </mfenced> <mi>ν</mi> </msup> </mrow> </mtd> <mtd columnalign="left"> <mrow> <mo>≺</mo> <mi>ψ</mi> <mrow> <mo stretchy="false">(</mo> <mi>z</mi> <mo stretchy="false">)</mo> </mrow> <mo>cos</mo> <mi>ϕ</mi> <mo>+</mo> <mi mathvariant="normal">i</mi> <mo>sin</mo> <mi>ϕ</mi> <mspace width="1em" /> <mtext>and</mtext> <mspace width="1em" /> <msup> <mrow> <mi mathvariant="normal">e</mi> </mrow> <mrow> <mi mathvariant="normal">i</mi> <mi>ϕ</mi> </mrow> </msup> <msup> <mfenced close="]" open="["> <msup> <mi mathvariant="normal">g</mi> <mo>′</mo> </msup> <mrow> <mo stretchy="false">(</mo> <mi mathvariant="normal">z</mi> <mo stretchy="false">)</mo> </mrow> </mfenced> <mi>τ</mi> </msup> <msup> <mfenced close="]" open="["> <mfrac> <mi mathvariant="normal">z</mi> <mrow> <mi mathvariant="normal">g</mi> <mo stretchy="false">(</mo> <mi mathvariant="normal">z</mi> <mo stretchy="false">)</mo> </mrow> </mfrac> </mfenced> <mi>ν</mi> </msup> </mrow> </mtd> <mtd columnalign="right"> <mrow> <mo>≺</mo> <mi>ψ</mi> <mo stretchy="false">(</mo> <mi>z</mi> <mo stretchy="false">)</mo> <mo>cos</mo> <mi>ϕ</mi> <mo>+</mo> <mi mathvariant="normal">i</mi> <mo>sin</mo> <mi>ϕ</mi> <mo>,</mo> </mrow> </mtd> </mtr> </mtable> </mrow> </math></EquationSource> </Equation>for <InlineEquation ID="IEq4"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="41478_2025_893_Article_IEq4.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="124" /> </InlineMediaObject> <EquationSource Format="TEX">\(-\pi /2&lt;\phi &lt;\pi /2\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mo>-</mo> <mi>π</mi> <mo stretchy="false">/</mo> <mn>2</mn> <mo>&lt;</mo> <mi>ϕ</mi> <mo>&lt;</mo> <mi>π</mi> <mo stretchy="false">/</mo> <mn>2</mn> </mrow> </math></EquationSource> </InlineEquation>, where <InlineEquation ID="IEq5"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="41478_2025_893_Article_IEq5.gif" Format="GIF" Height="17" Rendition="HTML" Resolution="72" Type="Linedraw" Width="17" /> </InlineMediaObject> <EquationSource Format="TEX">\(\psi \)</EquationSource> <EquationSource Format="MATHML"><math> <mi>ψ</mi> </math></EquationSource> </InlineEquation> is a univalent function whose range is symmetric with respect to the real axis, and <InlineEquation ID="IEq6"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="41478_2025_893_Article_IEq6.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="11" /> </InlineMediaObject> <EquationSource Format="TEX">\(\tau \)</EquationSource> <EquationSource Format="MATHML"><math> <mi>τ</mi> </math></EquationSource> </InlineEquation> and <InlineEquation ID="IEq7"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="41478_2025_893_Article_IEq7.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="12" /> </InlineMediaObject> <EquationSource Format="TEX">\(\nu \)</EquationSource> <EquationSource Format="MATHML"><math> <mi>ν</mi> </math></EquationSource> </InlineEquation> are non-zero real numbers. We also examine other classes of related functions and establish connections with previously known results.</p>

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Coefficient estimates for power Bi–univalent Ma-Minda starlike and derivative functions

  • Halit Orhan,
  • Vali Soltani Masih,
  • Ali Ebadian

摘要

In this paper, we establish the initial Taylor-Maclaurin coefficients for normalized analytic functions \(f\,\) f in the open unit disk. We also assume that \(f\,\) f and its inverse \(g=f\,^{-1}\) g = f - 1 satisfy the following conditions \(\begin{aligned} \rm{e}^{\rm{i}\phi }\left[ f\,^{\prime }\,(z)\right] ^{\tau }\left[ \frac{z}{f\,(z)}\right] ^{\nu }&\prec \psi (z)\cos \phi +\rm{i}\sin \phi \quad \text {and} \quad \rm{e}^{\rm{i}\phi }\left[ g'(z)\right] ^{\tau }\left[ \frac{z}{g(z)}\right] ^{\nu }&\prec \psi (z)\cos \phi +\rm{i}\sin \phi , \end{aligned}\) e i ϕ f ( z ) τ z f ( z ) ν ψ ( z ) cos ϕ + i sin ϕ and e i ϕ g ( z ) τ z g ( z ) ν ψ ( z ) cos ϕ + i sin ϕ , for \(-\pi /2<\phi <\pi /2\) - π / 2 < ϕ < π / 2 , where \(\psi \) ψ is a univalent function whose range is symmetric with respect to the real axis, and \(\tau \) τ and \(\nu \) ν are non-zero real numbers. We also examine other classes of related functions and establish connections with previously known results.