Notes on interacting holographic dark energy model in a closed universe
General Relativity and Quantum Cosmology
2021-03-12 v3
Abstract
We consider interacting holographic dark energy model in Friedmann Robertson Walker space time with positive spatial curvature and investigate the behavior of curvature parameter and dark energy density in accelerated expanding epoch. We also derive some conditions needed to cross the phantom divide line in this model.
Keywords
Cite
@article{arxiv.0806.2767,
title = {Notes on interacting holographic dark energy model in a closed universe},
author = {H. Mohseni Sadjadi and N. Vadood},
journal= {arXiv preprint arXiv:0806.2767},
year = {2021}
}
Comments
10 pages, typos corrected, some explanations and references added and updated, accepted for publication in JCAP