%0 Journal Article
%T Late Time Behavior of the Cosmological Model in Modified Theory of Gravity
%A Sankarsan Tarai
%A Jagadish Kumar
%J Journal of High Energy Physics, Gravitation and Cosmology
%P 1019-1031
%@ 2380-4335
%D 2022
%I Scientific Research Publishing
%R 10.4236/jhepgc.2022.84072
%X We report a viable exponential gravity model for the accelerated expansion of the universe in Bianchi <i>VI<sub>h</sub></i> space-time. By considering the estimated physical parameters, the cosmological models are constructed and analyzed in detail. We found that the state parameter in both the models increases to a higher negative range in an early epoch of the phantom domain and it goes to the positive domain at a late phase of the evolution. The effective cosmological constant remains in a positive domain for both models, which is a good sign of accelerating expansion of the universe.
%K &lt
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%K (&lt
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%K R&lt
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%K &lt
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%K T&lt
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%K ) Gravity
%K Bianchi Type &lt
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%K VI&lt
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%K h&lt
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%K Perfect Fluid
%U http://www.scirp.org/journal/PaperInformation.aspx?PaperID=120379