Thermodynamics in Modified Gravity Theories
arXiv:1101.3628 · doi:10.1142/S0218271811019542
Abstract
We demonstrate that there does exist an equilibrium description of thermodynamics on the apparent horizon in the expanding cosmological background for a wide class of modified gravity theories with the Lagrangian density , where is the Ricci scalar and is the kinetic energy of a scalar field . This comes from a suitable definition of an energy momentum tensor of the "dark" component obeying the local energy conservation law in the Jordan frame. It is shown that the equilibrium description in terms of the horizon entropy is convenient because it takes into account the contribution of the horizon entropy in non-equilibrium thermodynamics as well as an entropy production term.
8 pages, no figure, revised version, to be published in the Proceedings of the "2nd International Workshop on Dark Matter, Dark Energy and Matter-Antimatter Asymmetry."
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- Thermodynamic properties of modified gravity theories
- Note on the emergence of cosmic space in modified gravities
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