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<p>In this paper, we consider the spherically symmetric gravitational collapse of isotropic matter undergoing dissipation in the form of heat flux, with a generalized Vaidya exterior, in the context of <i>f</i>(<i>R</i>,&#xa0;<i>T</i>) gravity. Choosing <InlineEquation ID="IEq1"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10714_2025_3379_Article_IEq1.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="143" /> </InlineMediaObject> <EquationSource Format="TEX">\(f(R, T)=R+2\lambda T\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>f</mi> <mo stretchy="false">(</mo> <mi>R</mi> <mo>,</mo> <mi>T</mi> <mo stretchy="false">)</mo> <mo>=</mo> <mi>R</mi> <mo>+</mo> <mn>2</mn> <mi>λ</mi> <mi>T</mi> </mrow> </math></EquationSource> </InlineEquation>, and applying the <i>f</i>(<i>R</i>,&#xa0;<i>T</i>) junction conditions on the field equations for the interior and exterior regions, we have obtained matching conditions of the matter-Lagrangian and its derivatives across the boundary. The time of formation of singularity and the time of formation of apparent horizon have been determined and constraints on the integration constants are examined for which the final singularity is hidden behind the horizon.</p>

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Formation of singularity and apparent horizon for dissipative collapse in f(R, T) theory of gravity

  • 期刊论文

  • 发表日期：

    2025年2月18日

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  • Uttaran Ghosh,
  • Sarbari Guha

摘要

In this paper, we consider the spherically symmetric gravitational collapse of isotropic matter undergoing dissipation in the form of heat flux, with a generalized Vaidya exterior, in the context of f(R, T) gravity. Choosing \(f(R, T)=R+2\lambda T\) f ( R , T ) = R + 2 λ T , and applying the f(R, T) junction conditions on the field equations for the interior and exterior regions, we have obtained matching conditions of the matter-Lagrangian and its derivatives across the boundary. The time of formation of singularity and the time of formation of apparent horizon have been determined and constraints on the integration constants are examined for which the final singularity is hidden behind the horizon.