Nagpal, RitikaSingh, J. K.Aygun, S.2025-01-272025-01-2720180004-640X1572-946Xhttps://doi.org/10.1007/s10509-018-3335-9https://hdl.handle.net/20.500.12428/21693In this paper, we have studied the magnetized quark matter (QM) and strange quark matter (SQM) distributions in the presence of f (R, T) gravity in the background of Friedmann-Lemaitre-Robertson-Walker (FLRW) metric. To get exact solutions of modified field equations we have used f (R, T) = R + 2f (T) model given by Harko et al. with two different parametrization of geometrical parameters i.e. the parametrization of the deceleration parameter q, and the scale factor a in hybrid expansion form. Also, we have obtained Einstein Static Universe (ESU) solutions for QM and SQM distributions in f (R, T) gravity and General Relativity (GR). All models in f (R, T) gravity and GR for FRW and ESU Universes with QM also SQM distributions, we get zero magnetic field. These results agree with the solutions of Aktas and Aygun in f (R, T) gravity. However, we have also discussed the physical consequences of our obtained models.eninfo:eu-repo/semantics/closedAccessf (R, T) theoryMagnetized quark and strange quark matterFLRW universeDeceleration parameterStatic Einstein universeArticle363610.1007/s10509-018-3335-9Q3WOS:0004319450000012-s2.0-85046664904Q2