A Plane symmetric Bianchi type-I cosmological model coupled with magnetized strange quark matter in f(ℛ,𝒯) gravity admitting almost Schouten solitons

In this paper, we study a magnetized strange quark matter with the help of a plane symmetric Bianchi-I cosmological model in [Formula: see text] gravity. Additionally, we demonstrate that some specific physical properties of a plane symmetric Bianchi-I spacetime that permit the inclusion of magnetized strange quark matter in [Formula: see text] gravity, with a [Formula: see text]-vector field, where the metric exhibits properties as almost Schouten soliton and gradient almost Schouten soliton. We further investigate the modified Liouville and Poisson equations associated with the almost Schouten soliton on a plane symmetric Bianchi-I spacetime. Along with [Formula: see text] gravity and magnetized strange quark matter, we explore the harmonic aspects of almost Schouten soliton on such a spacetime. However, we analyze the results from the solution of field equations in association with shear scalar and scalar expansion on spacetime using the power law. In conclusion, we compute dynamical cosmological parameters by using an equation of state for magnetized strange quark matter and we examine some physical and geometrical aspects of such a model in [Formula: see text] gravity.