Thermodynamics of viscous dark energy in an RSII braneworld
arXiv:1103.1066 · doi:10.1142/S0218271810016361
Abstract
We show that for an RSII braneworld filled with interacting viscous dark energy and dark matter, one can always rewrite the Friedmann equation in the form of the first law of thermodynamics, , at apparent horizon. In addition, the generalized second law of thermodynamics can fulfilled in a region enclosed by the apparent horizon on the brane for both constant and time variable 5-dynamical Newton's constant . These results hold regardless of the specific form of the dark energy. Our study further support that in an accelerating universe with spatial curvature, the apparent horizon is a physical boundary from the thermodynamical point of view.
11 pages
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- Interacting Viscous Dark Energy in Bianchi Type-I Universe
- Viscous extended holographic Ricci dark energy in the framework of standard Eckart theory
- Thermodynamics of viscous dark energy for the late future time universe
- A comprehensive analysis of Barrow holographic Chaplygin gas model reconstruction and its cosmological consequences
- Thermodynamical aspects of modified holographic dark energy model
- Modelling brain based on canonical ensemble with functional MRI: A thermodynamic exploration on neural system
- Late time cosmological solutions in gravity in a viscous Universe