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

635 citations · 6.4k across the 144 of their papers we have counts for

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9 papers · 1 filter

astro-ph2008★ 126 cited

Observational constraints on the dark energy and dark matter mutual coupling

Chang Feng, Bin Wang, Elcio Abdalla +1

We examine different phenomenological interaction models for Dark Energy and Dark Matter by performing statistical joint analysis with observational data arising from the 182 Gold…

astro-ph2006★ 207 cited

Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters

Bin Wang, Jiadong Zang, Chi-Yong Lin +2

Several observational constraints are imposed on the interacting holographic model of Dark Energy and Dark Matter. First we use the age parameter today, as given by the WMAP result…

astro-ph2000★ 33 cited

Entropy and holography constraints for inhomogeneous universes

Bin Wang, Elcio Abdalla, Takeshi Osada

We calculated the entropy of a class of inhomogeneous dust universes. Allowing spherical symmetry, we proposed a holographic principle by reflecting all physical freedoms on the su…

astro-ph1999★ 16 cited

Scale Invariance in a Perturbed Einstein-de Sitter Cosmology

Elcio Abdalla, Roya Mohayaee, Marcelo B. Ribeiro

This paper seeks to check the validity of the "apparent fractal conjecture" (Ribeiro 2001ab: gr-qc/9909093, astro-ph/0104181), which states that the observed power-law behaviour fo…

astro-ph1998★ 1 cited

Gravitational instabilities and faster evolving density perturbations

Elcio Abdalla, Roya Mohayaee

The evolution of inhomogeneities in a spherical collapse model is studied by expanding the Einstein equation in powers of inverse radial parameter. In the linear regime, the densit…

astro-ph1998

Gravitational Clustering to All Perturbative Orders

Elcio Abdalla, Roya Mohayaee

We derive the time evolution of the density contrast to all orders of perturbation theory, by solving the Einstein equation for scale-invariant fluctuations. These fluctuations are…