English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

An equilibrium picture of thermodynamics is discussed at the apparent horizonof FRW universe in $f(T,T_G)$ gravity, where $T$ represents the torsioninvariant and $T_G$ is the teleparallel equivalent of the Gauss-Bonnet term. Itis found that one can translate the Friedmann equations to the standard form offirst law of thermodynamics. We discuss GSLT in the locality of assumption thattemperature of matter inside the horizon is similar to that of horizon.Finally, we consider particular models in this theory and generate constraintson the coupling parameter for the validity of GSLT in terms of recent cosmicparameters and power law solutions.

Generalized Second Law of Thermodynamics in $f(T,T_{G})$ gravity