Dynamics of an Anisotropic Universe in f(R,T) Theory

Dynamics of an anisotropic universe is studied in $f(R,T)$ gravity using a rescaled functional $f(R,T)$.
Three models have been constructed assuming a power law expansion of the universe. Physical features of
the models are discussed. The model parameters are constrained from a dimensional analysis. It is found
from the work that, the $BVI_h$ model in the modified gravity can favour quintessence and phantom phase.