We study the black hole evaporation and Hawking radiation for a noncommutative charged Vaidya black hole. For this purpose, we determine a spherically symmetric charged Vaidya model and then formulate a noncommutative Reissner-Nordstr?m-like solution of this model, which leads to an exact (t - r)-depen-dent metric. The behavior of the temporal component of this metric and the corresponding Hawking tem-perature are investigated. The results are shown in the form of graphs. Further, we examine the tunneling pro-cess of charged massive particles through the quantum horizon. We find that the tunneling amplitude is mod-ified due to noncommutativity. Also, it turns out that the black hole evaporates completely in the limits of large time and horizon radius. The effect of charge is to reduce the temperature from a maximum value to zero. We note that the final stage of black hole evaporation is a naked singularity.
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