  The aim of this paper is to study the black hole evaporation and Hawking
radiation for a noncommutative charged Vaidya black hole. For this purpose, we
determine spherically symmetric charged Vaidya model and then formulate a
noncommutative Reissner-Nordstr$\ddot{o}$m-like solution of this model which
leads to an exact $(t-r)$ dependent metric. The behavior of temporal component
of this metric and the corresponding Hawking temperature is investigated. The
results are shown in the form of graphs. Further, we examine the tunneling
process of the charged massive particles through the quantum horizon. It is
found that the tunneling amplitude is modified due to noncommutativity. Also,
it turns out that black hole evaporates completely in the limits of large time
and horizon radius. The effect of charge is to reduce the temperature from
maximum value to zero. It is mentioned here that the final stage of black hole
evaporation turns out to be a naked singularity.
