Thermodynamics of cosmological horizons in $f(T)$ gravity

Chao-Qiang Geng; Kazuharu Bamba

Thermodynamics of cosmological horizons in $f(T)$ gravity

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arxiv 1109.1694 v2 pith:URFADLQW submitted 2011-09-08 gr-qc astro-ph.COhep-th

Kazuharu Bamba , Chao-Qiang Geng This is my paper · ORCID

classification gr-qcastro-ph.COhep-th

keywords gravitythermodynamicsapparentequilibriumhorizonnon-equilibriumsamecosmological

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abstract

We explore thermodynamics of the apparent horizon in $f(T)$ gravity with both equilibrium and non-equilibrium descriptions. We find the same dual equilibrium/non-equilibrium formulation for $f(T)$ as for $f(R)$ gravity. In particular, we show that the second law of thermodynamics can be satisfied for the universe with the same temperature of the outside and inside the apparent horizon.

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Cosmological horizon thermodynamics in Gauss-Bonnet quasi-dilaton Massive Gravity
gr-qc 2026-07 reject novelty 5.0 of 10

Gauss-Bonnet quasi-dilaton massive gravity is claimed to obey horizon thermodynamics and the holographic entropy bound, provided the Gauss-Bonnet coupling is non-negative.

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