Higher-dimensional Bianchi type-I dark energy models with barotropic fluid in Saez-Ballester scalar-tensor theory of gravitation

In this paper, we delve into the cosmological assessments concerning the deceleration parameter [Formula: see text] in the context of the Bianchi type-III cosmological model within the framework of the Saez–Ballester theory of gravitation. By postulating a proportional relationship between the shear scalar ([Formula: see text]) and the expansion scalar ([Formula: see text]), we derive solutions for the corresponding field equations. Additionally, we conduct an examination and evaluation of the model’s physical and kinematic parameters, including the jerk parameter and snap parameter, while also discussing the energy condition of the model. Through the depiction of graphical representations, we illustrate the variations of the cosmological parameters for specific sets of constants.

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Higher-dimensional Bianchi type-I dark energy models with barotropic fluid in Saez-Ballester scalar-tensor theory of gravitation

Cited by 2 publications

References 55 publications

Anisotropic Bianchi type-$$VI_{0}$$ wet dark fluid cosmological models in Lyra’s manifold

Anisotropic Bianchi type-$$VI_{0}$$ wet dark fluid cosmological models in Lyra’s manifold

Studies on Bianchi type-III cosmological model with parametrization of deceleration parameter in a SBST theory

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