Hologrphy and holographic dark energy model

TL;DR

This paper explores the holographic dark energy model using the holographic principle, revealing that the Bekenstein-Hawking entropy bound is not saturated and deriving new constraints on model parameters.

Contribution

It introduces a more general parameter constraint for the holographic dark energy model based on holographic principle considerations.

Findings

Bekenstein-Hawking entropy bound is not saturated under certain conditions

Derived a more general constraint on the holographic dark energy parameter

Provided insights into the holographic principle's application to dark energy

Abstract

The holographic principle is used to discuss the holographic dark energy model. We find that the Bekenstein-Hawking entropy bound is far from saturation under certain conditions. A more general constraint on the parameter of the holographic dark energy model is also derived.