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 2007Show all

20 papers · 1 filter

gr-qc2007★ 43 cited

Quasinormal modes and phase Transition of black holes

Xiaoping Rao, Bin Wang, Guohong Yang

We have studied the scalar field as well as the fermonic field perturbations in the background of the massless BTZ black holes. Comparing with the perturbation results in the gener…

gr-qc2007★ 240 cited

Le Chatelier-Braun principle in cosmological physics

Diego Pavon, Bin Wang

Assuming that dark energy may be treated as a fluid with a well defined temperature, close to equilibrium, we argue that if nowadays there is a transfer of energy between dark ener…

hep-th2007★ 32 cited

Greybody Factors for Rotating Black Holes on Codimension-2 Branes

Songbai Chen, Bin Wang, Ru-Keng Su +1

We study the absorption probability and Hawking radiation of the scalar field in the rotating black holes on codimension-2 branes. We find that finite brane tension modifies the st…

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★ 83 cited

Thermodynamics on the apparent horizon in generalized gravity theories

Shao-Feng Wu, Bin Wang, Guo-Hong Yang

We present a general procedure to construct the first law of thermodynamics on the apparent horizon and illustrate its validity by examining it in some extended gravity theories. A…

hep-th2007★ 43 cited

Hawking radiation in a Rotating Kaluza-Klein Black Hole with Squashed Horizons

Songbai Chen, Bin Wang, Ru-Keng Su

We explore the signature of the extra dimension in the Hawking radiation in a rotating Kaluza-Klein black hole with squashed horizons. Comparing with the spherical case, we find th…