Properties of an Ar/C2H2 plasma afterglow with dust particles are investigated at different assumptions concerning negative ion formation. First, numerical calculations are carried out assuming that C2nH2− negative ions, where n is a natural number, are the dominant anions in the plasma afterglow (the case (i)). Second, the studies are conducted assuming that C2nH− anions are only the negative ions, which are present in the afterglow plasma (the case (ii)). It is shown that the total density of negative ions n_ in the case (ii) is smaller than n_ in the case (i). Due to smaller n_, the positive ion densities are smaller and the absolute values of the mean dust charge and its variances are larger in the case (ii) than the corresponding values calculated using the approach (i). We also calculated the dust charge distribution functions (DCDFs) for late afterglow times. It is found that the DCDFs obtained in the case (ii) are shifted to the region of larger negative charges comparing with the dust charge distributions obtained in the case (i). The differences are mainly due to the loss of C2nH − anions in collisions with H atoms in the case (ii). In the case when the loss of negative ions in collisions with H atoms is not taken into account in the models, the both approaches give nearly the same time dependences for positive and negative ion densities, electron density, mean dust charge and its variance.
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