A spatially homogeneous and anisotropic locally-rotationally-symmetric Bianchi type-I spacetime model with strange quark matter (SQM) and a variable cosmological term $\Lambda \left(t\right)$ is studied in $f(R,T)$ theory. The exact solutions are obtained for a particular form of $f(R,T)=R+2\lambda T$ under the law of variable deceleration parameter proposed by Banerjee et al (2005). The model presents a cosmological scenario of transition from early deceleration to late time acceleration. In the absence of $f(R,T)$ gravity and SQM, $\Lambda \left(t\right)$ accelerates the universe. In a specific case when $\Lambda \left(t\right)$ vanishes at late times, the SQM accelerates the universe, even in the absence of $f(R,T)$ gravity. The model shows the possibility that SQM could be an alternative to dark energy. The physical viability of the model costs the observational inconsistency.

具有奇异夸克物质 (SQM) 和可变宇宙学项的空间均匀和各向异性局部旋转对称 Bianchi I 型时空模型 $\Lambda \left(吨\right)$ 在学习 $F(\mathrm{电阻},吨)$理论。得到特定形式的精确解$F(\mathrm{电阻},吨)=\mathrm{电阻}+2\lambda 吨$根据 Banerjee 等人 (2005) 提出的可变减速参数定律。该模型呈现了从早期减速到晚期加速过渡的宇宙学情景。在缺少...之下$F(\mathrm{电阻},吨)$ 重力和 SQM， $\Lambda \left(吨\right)$加速宇宙。在特定情况下，当$\Lambda \left(吨\right)$ 在后期消失，SQM 加速宇宙，即使在没有 $F(\mathrm{电阻},吨)$重力。该模型显示了 SQM 可以替代暗能量的可能性。模型的物理可行性会导致观测不一致。