  This paper is devoted to study charged fermion particles tunneling through
the horizon of Kerr-Newman-AdS black hole surrounded by quintessence by using
Hamilton-Jacobi ansatz. In our analysis, we investigate Hawking temperature as
well as quantum corrected Hawking temperature on account of generalized
uncertainty principle. Moreover, we discuss the effects of correction parameter
$\beta$ on the corrected Hawking temperature $T_{e-H}$, graphically. We
conclude that the temperature $T_{e-H}$ vanishes when $\beta=100$, whereas for
$\beta<100$ and $\beta>100$, the temperature turns out to be positive and
negative, respectively. We observe that the graphs of $T_{e-H}$ w.r.t.
quintessence parameter $\alpha$ exhibit behavior only for the particular
ranges, i.e., $0<\alpha<1/6$, charge $0<Q\leq1$ and rotation parameter
$0<a\leq1$. For smaller and larger values of negative $\Lambda$, as horizon
increases, the temperature decreases and increases, respectively.
