2006/11/30 by Rong-Gen Cai, Li-Ming Cao · 20 citations
Physics and Astronomy · #Apparent horizon #Black Holes and Theoretical Physics #Classical mechanics #Cosmology and Gravitation Theories #Entropy (arrow of time) #Event horizon #First law of thermodynamics #Friedmann–Lemaître–Robertson–Walker metric #Gravitation #Horizon #Mathematical physics #Physics #Quantum Electrodynamics and Casimir Effect #Quantum mechanics #Second law of thermodynamics #Thermodynamics #Universe #gr-qc #hep-th
paper · pdf · doi:10.1103/physrevd.75.064008
published as Phys.Rev.D75:064008,2007 · v2: revtex, 23 pages, references added, minor changes, to appear in PRD
arxiv created 2007/02/24 · openalex publication_date 2007/03/12 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
In this paper we revisit the relation between the Friedmann equations and the first law of thermodynamics. We find that the unified first law first proposed by Hayward to treat the outertrapping horizon of a dynamical black hole can be used to the apparent horizon (a kind of inner trapping horizon in the context of the FRW cosmology) of the FRW universe. We discuss three kinds of gravity theorties: Einstein theory, Lovelock thoery, and scalar-tensor theory. In Einstein theory, the first law of thermodynamics is always satisfied on the apparent horizon. In Lovelock theory, treating the higher derivative terms as an effective energy-momentum tensor, we find that this method can give the same entropy formula for the apparent horizon as that of black hole horizon. This implies that the Clausius relation holds for the Lovelock theory. In scalar-tensor gravity, we find, by using the same procedure, the Clausius relation no longer holds. This indicates that the apparent horizon of the FRW universe in the scalar-tensor gravity corresponds to a system of nonequilibrium thermodynamics. We show this point by using the method developed recently by Eling et al. for dealing with the f(R) gravity.