  In this work, I present for the first time the analysis concerning the growth
of matter fluctuations in the framework of $f(R,T)$ modified gravity where I
presume $f(R,T) = R + \lambda T$, where $R$ denote the Ricci scalar, $T$ the
trace of the energy-momentum tensor and $\lambda$ a constant. I first solve the
Friedman equations assuming a dust universe ($\omega =0$) for the Hubble
parameter $H(z)$ and then employ it in the equation of matter density
fluctuations $\delta(z)$ to solve for $\delta(z)$ and the growth rate $f(z)$.
Next, I proceed to show the behavior of $f(z)$ and $\delta(z)$ with redshift
for some values of $\lambda$ with observational constraints. Finally, following
the prescription of \cite{growft41}, I present an analytical expression for the
growth index $\gamma$ which is redshift dependent and the expression reduces to
$3/5$ for $\lambda=0$, which is the growth index for a dust universe.
