Bianchi Type VI0 Generalized Ghost Pilgrims Dark Energy Cosmological Model in Saez-Ballester Theory of Gravitation
Abstract
The Generalized Ghost Pilgrim Dark Energy (GGPDE) in the Saez-Ballester Theory of Gravitation (SBTG) and the Bianchi type VI0 space-time framework serve as the foundation for this work. We used Mishra and Dua's [Astrophys. Space Sci. 366, 6 (2021)] straightforward parameterization of average scale factor a(t) = exp{(αt+β)p} to find precise solutions to the field equations. We have looked into the GGPDE and dark matter (DM), both when they interact and when they don't. For both models, some significant and well-known parameters are produced, including the Hubble parameter, the equation of state (EOS) parameter, the deceleration parameter, etc. It is discovered that for both models, the deceleration parameter denotes an accelerated phase and the EOS parameter a cosmological constant. For both the non-interacting and interacting models, the stability analysis and energy conditions are examined.
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