Viability of specific reconstructed f(T,𝒯) models
Abstract
The reconstruction scenario of well-established dark energy models such as pilgrim dark energy model and generalized ghost dark energy with Hubble horizon and f(T,𝒯) models is being considered. We have established f(T,𝒯) models and analyzed their viability through equation of state parameter and ω−ω′ (where prime denotes derivative with respect to lna) plane. The equation of state parameter evolutes the universe in three different phases such as quintessence, vacuum and phantom. However, the ω−ω′ plane also describes the thawing as well as freezing region of the universe. The recent observational data also favor our results.
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