Reconstructing the interaction rate in holographic models of dark energy

TL;DR

This paper reconstructs the interaction rate of a holographic dark energy model using observational data, revealing its evolution over redshift and implications for dark energy behavior.

Contribution

It provides the first reconstruction of the interaction rate in a specific holographic dark energy model using multiple observational datasets.

Findings

Interaction rate increases with expansion in the past.

Interaction rate decreases at recent times.

Dark energy equation of state does not cross the phantom divide.

Abstract

We reconstruct the interaction rate of the holographic dark energy model recently proposed by Zimdahl and Pav\'{o}n \cite{wd} in the redshift interval $0 < z < 1.8$ with observational data from supernovae type Ia, baryon acoustic oscillations, gas mass fraction in galaxy clusters, and the growth factor. It shows a reasonable behavior in the sense that it increases with expansion from a small or vanishing value in the long past but starts decreasing at recent times. The later feature suggests that the equation of state parameter of dark energy does not cross the phantom divide.