2016/01/31 by Yumei Huang, YuMei Huang, Yungui Gong +1
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Entropy (arrow of time) #Equivalence (formal languages) #Extended irreversible thermodynamics #First law of thermodynamics #Laws of thermodynamics #Non-equilibrium thermodynamics #Pulsars and Gravitational Waves Research #Scalar field #Second law of thermodynamics #Time derivative #astro-ph.CO #gr-qc #hep-th
paper · pdf · doi:10.1007/s11433-016-5793-9
published as Sci. China-Phys. Mech. Astron. 59, 640402 (2016) · 10 pages, no figure, minor corrections, SCIENCE CHINA Physics,Mechanics & Astronomy in press
arxiv created 2016/02/02 · openalex publication_date 2016/02/22 · arxiv updated 2016/03/04 · openalex created_date 2017/04/07 · openalex updated_date 2026/08/05
With the usual definitions for the entropy and the temperature associated with the apparent horizon, we discuss the first law of the thermodynamics on the apparent in the general scalar-tensor theory of gravity with the kinetic term of the scalar field non-minimally coupling to Einstein tensor. We show the equivalence between the first law of thermodynamics on the apparent horizon and Friedmann equation for the general models, by using a mass-like function which is equal to the Misner-Sharp mass on the apparent horizon. The results further support the universal relationship between the first law of thermodynamics and Friedmann equation.