Can Holographic dark energy models fit the observational data?
Mohammad Malekjani, Mehdi Rezaei, Iman A. Akhlaghi

TL;DR
This study shows that holographic dark energy models with a time-varying parameter based on the current Hubble horizon can fit observational data well, unlike previous models based on other horizons.
Contribution
It introduces a new class of holographic dark energy models with a time-varying parameter on the Hubble scale and demonstrates their compatibility with observational data.
Findings
Models fit both expansion and growth rate data.
Transition epoch aligns with observational constraints.
Comparable fit to $ ext{Lambda}$CDM cosmology.
Abstract
In this work we investigate the holographic dark energy models with slowly time-varying model parameter defined based on the current Hubble horizon length scale. While the previous studies on the three popular holographic dark energy models defined based on the future event horizon, Ricci scale and Granda-Oliveros IR cutoffs showed that these models cannot fit the observational data [1], in this work we show that the holographic dark energy models with time-varying model parameter defined on the current Hubble radius are well favored by observations. Using the standard minimization in the context of Markov Chain Monte Carlo method, we compare the ability of holographic dark energy models with time-varying parameter constructed on the current Hubble length scale against different sets of observational data namely expansion data, growth rate data and expansion+growth rate…
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