Notes on interacting holographic dark energy model in a closed universe

Details Notes on interacting holographic dark energy model in a closed universe Notes on interacting holographic dark energy model in a closed universe

2008-06-17

arxiv.org/abs/0806.2767v3

JCAP0808:036,2008

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

10 pages, typos corrected, some explanations and references added and updated, accepted for publication in JCAP

Scientific paper

10.1088/1475-7516/2008/08/036

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.

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