Abstract <p>In this study, we characterize a Lorentzian manifold <InlineEquation ID="IEq3"> <EquationSource Format="TEX">\((M^{n},g)\)</EquationSource> <!--GravCos2670011Ghosh-m3--> </InlineEquation> of dimension <InlineEquation ID="IEq4"> <EquationSource Format="TEX">\(\geq 3\)</EquationSource> <!--GravCos2670011Ghosh-m4--> </InlineEquation> satisfying Gray’s <InlineEquation ID="IEq5"> <EquationSource Format="TEX">\(\mathcal{C}^{\bot}\)</EquationSource> <!--GravCos2670011Ghosh-m5--> </InlineEquation> condition. First, we prove that if a Lorentzian manifold <InlineEquation ID="IEq6"> <EquationSource Format="TEX">\(M\)</EquationSource> <!--GravCos2670011Ghosh-m6--> </InlineEquation> satisfies Gray’s <InlineEquation ID="IEq7"> <EquationSource Format="TEX">\(\mathcal{C}^{\bot}\)</EquationSource> <!--GravCos2670011Ghosh-m7--> </InlineEquation> condition and whose Ricci curvature annihilates the curvature transformation, then in the neighborhood of a point where <InlineEquation ID="IEq8"> <EquationSource Format="TEX">\(|\nabla\,r_{g}|\neq 0\)</EquationSource> <!--GravCos2670011Ghosh-m8--> </InlineEquation>, <InlineEquation ID="IEq9"> <EquationSource Format="TEX">\(M\)</EquationSource> <!--GravCos2670011Ghosh-m9--> </InlineEquation> is a generalized Robertson–Walker (GRW) space-time. Next, it is established that if a quasi-Einstein Lorentzian manifold satisfies Gray’s <InlineEquation ID="IEq10"> <EquationSource Format="TEX">\(\mathcal{C}^{\bot}\)</EquationSource> <!--GravCos2670011Ghosh-m10--> </InlineEquation> condition, then in the neighborhood of a point where <InlineEquation ID="IEq11"> <EquationSource Format="TEX">\(\beta\neq 0\)</EquationSource> <!--GravCos2670011Ghosh-m11--> </InlineEquation>, <InlineEquation ID="IEq12"> <EquationSource Format="TEX">\(M\)</EquationSource> <!--GravCos2670011Ghosh-m12--> </InlineEquation> is a GRW space-time. Furthermore, it is confirmed that any perfect fluid GRW space-time is Bach-flat.</p>

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Characterizations of Lorentzian Manifolds Satisfying Gray’s \(\boldsymbol{\mathcal{C}^{\bot}}\) Condition

  • Amalendu Ghosh

摘要

Abstract

In this study, we characterize a Lorentzian manifold \((M^{n},g)\) of dimension \(\geq 3\) satisfying Gray’s \(\mathcal{C}^{\bot}\) condition. First, we prove that if a Lorentzian manifold \(M\) satisfies Gray’s \(\mathcal{C}^{\bot}\) condition and whose Ricci curvature annihilates the curvature transformation, then in the neighborhood of a point where \(|\nabla\,r_{g}|\neq 0\) , \(M\) is a generalized Robertson–Walker (GRW) space-time. Next, it is established that if a quasi-Einstein Lorentzian manifold satisfies Gray’s \(\mathcal{C}^{\bot}\) condition, then in the neighborhood of a point where \(\beta\neq 0\) , \(M\) is a GRW space-time. Furthermore, it is confirmed that any perfect fluid GRW space-time is Bach-flat.