activity
19972026
most citedTransition of the dark energy equation of state in an interacting holographic dark energy model

635 citations · 12.7k across the 245 of their papers we have counts for

collaborators
Showing 2004 · hep-thShow all

7 papers · 2 filters

hep-th2004★ 173 cited

Constraints on the Dark Energy from the holographic connection to the small l CMB Suppression

Jianyong Shen, Bin Wang, Elcio Abdalla +1

Using the recently obtained holographic cosmic duality, we reached a reasonable quantitative agreement between predictions of the Cosmic Microwave Background Radiation at small l a…

hep-th2004★ 105 cited

The Holographic dark energy reexamined

Yungui Gong, Bin Wang, Yuan-Zhong Zhang

We have reexamined the holographic dark energy model by considering the spatial curvature. We have refined the model parameter and observed that the holographic dark energy model d…

hep-th2004★ 56 cited

Probing the curvature of the Universe from supernova measurement

Bin Wang, Yungui Gong, Ru-Keng Su

We study the possibility to probe the spatial geometry of the Universe by supernova measurement of the cubic correction to the luminosity distance. We illustrate with an accelerati…

hep-th2004★ 124 cited

Quasinormal behavior of massless scalar field perturbation in Reissner-Nordstrom anti-de Sitter spacetimes

Bin Wang, Chi-Yong Lin, C. Molina

We present a comprehensive study of the massless scalar field perturbation in the Reissner-Nordstrom anti-de Sitter (RNAdS) spacetime and compute its quasinormal modes (QNM). For t…

hep-th2004★ 140 cited

Constraints on the dark energy from holography

Bin Wang, Elcio Abdalla, Ru-Keng Su

Using the holographic principle we constrained the Friedmann equation, modified by brane-cosmology inspired terms which accommodate dark energy contributions in the context of extr…

hep-th2004★ 96 cited

Quasinormal modes in pure de sitter spacetimes

Da-Ping Du, Bin Wang, Ru-Keng Su

We have studied scalar perturbations as well as fermion perturbations in pure de Sitter space-times. For scalar perturbations we have showed that well-defined quasinormal modes can…