Thermodynamics of Gravity with Disformal Transformation
arXiv:1902.04859 · doi:10.3390/e21020172
Abstract
We study thermodynamics in gravity with the disformal transformation. The transformation applied to the matter Lagrangian has the form of $\g_{\m\n} = A(ϕ,X)g_{\m\n} + B(ϕ,X)\pa_\m\f\pa_\n\f$ with the assumption of the Minkowski matter metric $\g_{\m\n} = \e_{\m\n}$, where is the disformal scalar and is the corresponding kinetic term of . We verify the generalized first and second laws of thermodynamics in this disformal type of gravity in the Friedmann-Lemaître-Robertson-Walker (FLRW) universe. In addition, we show that the Hubble parameter contains the disformally induced terms, which define the effectively varying equations of state for matter.
23 pages, no figure, published version in Entropy 21, 172 (2019)
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