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Generalized entropies and the expansion law of the universe

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arxiv 1406.3712 v2 pith:HTVGJALN submitted 2014-06-14 gr-qc

classification gr-qc
keywords expansionobtainuniversefirstkodamaobserverthermodynamicsapproach
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We suggest that using the first law of thermodynamics is a convenient method to obtain a correct form of the expansion law of the universe \cite{T. Padmanabhan1}. We will, then, use this idea to obtain the expansion law for a Kodama observer. By using the expansion law for a Kodama observer, we can obtain the dynamic equation of the FRW universe for deformed Horava-Lifshitz gravity. The use of the first law of thermodynamics also leads to a new approach for obtaining the Friedmann equations for f(R) and scalar tensor gravities.

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  1. First Law of Thermodynamics and Emergence of Cosmic Space in a Non-Flat Universe

    gr-qc 2019-08 conditional novelty 5.0 of 10

    In a non-flat Friedmann universe, the unified first law dE = TdS + WdV and the energy-flux form -dE = TdS are consistent only when the horizon volume is taken as the areal volume, not the proper invariant volume.

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