Reconstructing f(R) theory according to holographic dark energy
Xing Wu, Zong-Hong Zhu

TL;DR
This paper establishes a link between holographic dark energy and $f(R)$ gravity, reconstructing the $f(R)$ function for different parameter regimes to analyze their future cosmological evolution.
Contribution
It introduces a method to reconstruct $f(R)$ gravity models based on holographic dark energy parameters, highlighting their distinct future behaviors.
Findings
Different $f(R)$ models correspond to different holographic parameter regimes.
Reconstructed $f(R)$ functions exhibit unique future evolution patterns.
The approach provides a unified framework for connecting dark energy models with modified gravity.
Abstract
In this paper a connection between the holographic dark energy model and the theory is established. We treat the theory as an effective description for the holographic dark energy and reconstruct the function with the parameter , and , respectively. We show the distinctive behavior of each cases realized in theory, especially for the future evolution.
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