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Clausius relation and Friedmann equation in FRW universe model

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arxiv 1001.2597 v2 pith:PWFT7WLC submitted 2010-01-15 hep-th gr-qc

Clausius relation and Friedmann equation in FRW universe model

classification hep-th gr-qc
keywords gravityapparentequationfriedmannhorizonkodamauniverseava-lifshitz
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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It has been shown that Friedmann equation of FRW universe can be derived from the first law of thermodynamics in Einstein gravity, Gauss-Bonnet gravity, Lovelock gravity, scalar-tensor gravity and $f(R)$ gravity. Moreover, it was pointed out that the temperature of the apparent horizon can be obtained using the tunneling formalism for the corresponding observers defined by Kodama vector. In this article, we find that the energy flux through the apparent horizon can be determined by using the Kodama vector. This implies the fact that the Clausius relation and the first law of thermodynamics associated with the apparent horizon in FRW universe is relative to the Kodama observers.We illustrate the derivation of Friedmann equation, and also extend the study to the cases of Ho\v{r}ava-Lifshitz gravity and IR modified Ho\v{r}ava-Lifshitz gravity.

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Cited by 1 Pith paper

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  1. Cosmological horizon thermodynamics in Gauss-Bonnet quasi-dilaton Massive Gravity

    gr-qc 2026-07 reject novelty 5.0

    Gauss-Bonnet quasi-dilaton massive gravity is claimed to obey horizon thermodynamics and the holographic entropy bound, provided the Gauss-Bonnet coupling is non-negative.