On the Stark broadening of O I spectral lines: comparison with experiments

Stark broadening parameters, line widths, and shifts have been calculated for spectral lines within the neutral oxygen spectrum for experimental conditions of published experiments to compare experiments with results of the semiclassical perturbation method.The obtained data are of particular interest in astrophysics, for instance, for the investigation of stellar spectra but also for laboratory plasma diagnostics and plasma spectra containing lines of neutral oxygen.