Aktaş, Can2025-01-272025-01-2720171300-01011303-6122https://doi.org/10.3906/fiz-1706-4https://hdl.handle.net/20.500.12428/28761https://search.trdizin.gov.tr/tr/yayin/detay/244533In this article, we have investigated the behaviors of magnetized strange quark matter distributions for Bianchi I and V universes in reconstructed f (R, T) = α1R+α2f3(T) gravity (here α1 and α2 are constants; f3(T) is an arbitrary function of T). To get solutions of the field equations we have used a deceleration parameter and the equation of state for strange quark matter. The new represented f(R,T) model includes two models of Harko et al. and transforms to general relativity. When t → ∞, we get the dark energy model (p = −ρ) in reconstructed f (R, T) = α1R + α2f3(T) gravity. However, we obtain zero magnetic field in all f(R, T) gravitation models.eninfo:eu-repo/semantics/openAccessf(R,T) gravityBianchi I universeBianchi V universemagnetized strange quarkdeceleration parameterArticle41546947610.3906/fiz-1706-4N/AWOS:0004151095000102-s2.0-85035140562Q2