Viscous Cosmology and Thermodynamics of Apparent Horizon
arXiv:0808.0169 · doi:10.1088/0256-307X/25/12/004
Abstract
It is shown that the differential form of Friedmann equations of FRW universe can be recast as a similar form of the first law, , of thermodynamics at the apparent horizon of FRW universe filled with the viscous fluid. It is also shown that the generalized second law of thermodynamics holds at the apparent horizon of FRW universe and preserves dominant energy condition.
8 pages
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Cited by in corpus (11)
- Hawking Radiation of Apparent Horizon in a FRW Universe
- Thermodynamics of apparent horizon and modified Friedman equations
- Thermodynamics in gravity with phantom crossing
- Generalized second law of thermodynamics for FRW cosmology with logarithmic correction
- Generalized second law of thermodynamics for a phantom energy accreting BTZ black hole
- Accretion of Phantom Energy and Generalized Second Law of Thermodynamics for Einstein-Maxwell-Gauss-Bonnet Black Hole
- Generalized second law of thermodynamics in modified FRW cosmology with corrected entropy-area relation
- Generalized Second Law of Thermodynamics in Extended Theories of Gravity
- A statistical representation of the cosmological constant from finite size effects at the apparent horizon
- The Unified First law in "Cosmic Triad" Vector Field Scenario
- Generalized second law of thermodynamics in massive gravity