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19992024
most citedInteracting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters

207 citations · 630 across the 14 of their papers we have counts for

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hep-th2022★ 10 cited

Analogous Hawking radiation and quantum entanglement in two-component Bose-Einstein condensates: the gapped excitations

Wei-Can Syu, Da-Shin Lee, Chi-Yong Lin

The condensates of cold atoms at zero temperature in the tunable binary Bose-Einstein condensate system are studied with the Rabi transition between atomic hyperfine states where t…

hep-th2008★ 48 cited

Quasinormal modes in the background of charged Kaluza-Klein black hole with squashed horizons

Xi He, Songbai-Chen, Bin Wang +2

We study the scalar perturbation in the background of the charged Kaluza-Klein black holes with squashed horizons. We find that the position of infinite discontinuities of the heat…

hep-th2007★ 158 cited

Thermodynamical description of the interaction between holographic dark energy and dark matter

Bin Wang, Chi-Yong Lin, Diego Pavon +1

We present a thermodynamical description of the interaction between holographic dark energy and dark matter. If holographic dark energy and dark matter evolve separately, each of t…

hep-th2007★ 29 cited

The transition of equation of state of effective dark energy in the DGP model with bulk contents

Shaoyu Yin, Bin Wang, Elcio Abdalla +1

We investigate the effect of the bulk contents in the DGP braneworld on the evolution of the universe. We find that although the pure DGP model cannot accommodate the transition of…

hep-th2005

Constraints on the interacting holographic dark energy model

Bin Wang, Chi-Yong Lin, Elcio Abdalla

We examined the interacting holographic dark energy model in a universe with spatial curvature. Using the near-flatness condition and requiring that the universe is experiencing an…

hep-th2003

WMAP constraint on the P-term inflationary model

Bin Wang, Chi-Yong Lin, Elcio Abdalla

In light of WMAP results, we examine the observational constraint on the P-term inflation. With the tunable parameter , P-term inflation contains richer physics than D-term and…