Original Articles |
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Viscous Cosmology and Thermodynamics of Apparent Horizon |
M. Akbar |
Centre for Advanced Mathematics and Physics National University of Sciences and Technology, Peshawar Road, Rawalpindi, Pakistan |
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Cite this article: |
M. Akbar 2008 Chin. Phys. Lett. 25 4199-4202 |
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Abstract It is shown that the differential form of Friedmann equations of Friedman--Robertson--Walker (FRW) universe can be recast as a similar form of the first law ThdSh = dE + WdV of thermodynamics at the apparent horizon of FRW universe filled with the viscous fluid. It is also shown that by employing the general expression of temperature associated with the apparent horizon of an FRW universe and assumed that the temperature Tm of the energy inside the apparent horizon is proportional to the horizon temperature Tm= bTh, we are able to show that the generalized second law of thermodynamics holds in the Einstein gravity provided Th-Tm/r~A ≤(ρ+P~).
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Keywords:
04.70.Dy
97.60.Lf
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Received: 16 September 2008
Published: 27 November 2008
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PACS: |
04.70.Dy
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(Quantum aspects of black holes, evaporation, thermodynamics)
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97.60.Lf
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(Black holes)
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