Interacting holographic dark energy model in non-flat universe

By M. Setare. 2006

269 citations recorded by the source corpus.

We employ the holographic model of interacting dark energy to obtain the equation of state for the holographic energy density in non-flat (closed) universe enclosed by the event horizon measured from the sphere of horizon named L.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/7dcce587b2a897b1c0a2a2fe2554e3881a536dee

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Yi Wang
2. Emmanuel N. Saridakis
3. Shuang Wang
4. Fotios Anagnostopoulos
5. Miao Li
6. S. Basilakos
7. M. Setare
8. Ratbay Myrzakulov

In Nuclear and High Energy Physics

1. Yi Wang
2. Emmanuel N. Saridakis
3. Shuang Wang
4. Fotios Anagnostopoulos
5. Miao Li
6. S. Basilakos
7. M. Setare
8. Ratbay Myrzakulov

Citations in the corpus

• Observational constraints on Barrow holographic dark energy (2020, result): “Holographic dark energy is very efficient in quantitatively describe the late-time acceleration [23–34] and it is in agreement with observational data [35–43].”