
TL;DR
This paper explores a holographic dark energy model in a non-flat universe, demonstrating it can be described by a phantom scalar field with a reconstructed potential for certain parameter values.
Contribution
It provides a novel phantom scalar field representation of interacting holographic dark energy in non-flat cosmology for specific parameter ranges.
Findings
Dark energy modeled as a phantom scalar field for c ≤ 0.84
Reconstructed potential of the phantom scalar field
Described the holographic dark energy in non-flat universe
Abstract
In this paper we consider the holographic model of interacting dark energy in non-flat universe. With the choice of , the interacting holographic dark energy can be described by a phantom scalar field. Then we show this phantomic description of the holographic dark energy with and reconstruct the potential of the phantom scalar field.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
