Abstract <p>We study <InlineEquation ID="IEq3"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="12267_2025_5282_Article_IEq3.gif" Format="GIF" Height="12" Rendition="HTML" Resolution="72" Type="Linedraw" Width="13" /> </InlineMediaObject> <EquationSource Format="TEX">\(\eta\)</EquationSource> <!--GravCos2570028Baidya-m3--> </InlineEquation>-Ricci–Yamabe solitons and gradient <InlineEquation ID="IEq4"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="12267_2025_5282_Article_IEq3.gif" Format="GIF" Height="12" Rendition="HTML" Resolution="72" Type="Linedraw" Width="13" /> </InlineMediaObject> <EquationSource Format="TEX">\(\eta\)</EquationSource> <!--GravCos2570028Baidya-m4--> </InlineEquation>-Ricci–Yamabe solitons in generalized Robertson–Walker space-times . At first, we provide an example of an <InlineEquation ID="IEq5"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="12267_2025_5282_Article_IEq3.gif" Format="GIF" Height="12" Rendition="HTML" Resolution="72" Type="Linedraw" Width="13" /> </InlineMediaObject> <EquationSource Format="TEX">\(\eta\)</EquationSource> <!--GravCos2570028Baidya-m5--> </InlineEquation>-Ricci–Yamabe soliton. Next, we prove that if a generalized Robertson–Walker space-time admits an <InlineEquation ID="IEq6"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="12267_2025_5282_Article_IEq3.gif" Format="GIF" Height="12" Rendition="HTML" Resolution="72" Type="Linedraw" Width="13" /> </InlineMediaObject> <EquationSource Format="TEX">\(\eta\)</EquationSource> <!--GravCos2570028Baidya-m6--> </InlineEquation>-Ricci–Yamabe soliton or a gradient <InlineEquation ID="IEq7"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="12267_2025_5282_Article_IEq3.gif" Format="GIF" Height="12" Rendition="HTML" Resolution="72" Type="Linedraw" Width="13" /> </InlineMediaObject> <EquationSource Format="TEX">\(\eta\)</EquationSource> <!--GravCos2570028Baidya-m7--> </InlineEquation>-Ricci–Yamabe soliton, then it becomes a perfect fluid space-time. As a consequence, we obtain several interesting corollaries.</p>

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Generalized Robertson–Walker Space-Times Admitting \(\boldsymbol{\eta}\)-Ricci–Yamabe Solitons

  • Ansari Rakesh Baidya,
  • Uday Chand De,
  • Abul Kalam Mondal

摘要

Abstract

We study \(\eta\) -Ricci–Yamabe solitons and gradient \(\eta\) -Ricci–Yamabe solitons in generalized Robertson–Walker space-times . At first, we provide an example of an \(\eta\) -Ricci–Yamabe soliton. Next, we prove that if a generalized Robertson–Walker space-time admits an \(\eta\) -Ricci–Yamabe soliton or a gradient \(\eta\) -Ricci–Yamabe soliton, then it becomes a perfect fluid space-time. As a consequence, we obtain several interesting corollaries.