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In our study, we have examined the holographic origin of cosmological inflation in the modified f(R, T) gravity model using two distinct forms of the scale factor, namely intermediate and logamediate. The reconstruction of f(R, T) gravity involves selecting a combination of f while assuming the generalised Holographic Dark Energy as the background fluid with an IR cutoff of \(\alpha H^2+\beta \dot{H}\) . The Equation of State (EoS) parameters have been examined in every instance. At last, the model’s slow-roll parameters are calculated. A potential for the model to serve as a unifying framework between early inflation and late-time acceleration has been observed.

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Probing the Inflationary Cosmology in f(R, T) Framework with Holographic Background Fluid

  • 会议论文

  • 发表日期：

    2025年

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  • Khandro K. Chokyi,
  • Surajit Chattopadhyay

摘要

In our study, we have examined the holographic origin of cosmological inflation in the modified f(R, T) gravity model using two distinct forms of the scale factor, namely intermediate and logamediate. The reconstruction of f(R, T) gravity involves selecting a combination of f while assuming the generalised Holographic Dark Energy as the background fluid with an IR cutoff of \(\alpha H^2+\beta \dot{H}\) . The Equation of State (EoS) parameters have been examined in every instance. At last, the model’s slow-roll parameters are calculated. A potential for the model to serve as a unifying framework between early inflation and late-time acceleration has been observed.