We use an improvement of a three-dimensional model [Phys. Rev. A 27, 2321 (1983)], taking space charge into account for ions confined in a quadrupole rf trap. This model allows us to calculate the spatial and energy probability densities of strongly confined ions in the presence of a light buffer gas and shows the evolution of these properties as the total number n of ions increases. The ions are Ce⁺ in the presence of dilute helium. For the chosen working point, the distributions remain Gaussian when n does not exceed (2-3) ×{} 10⁵ ions at room temperature. The influence of the temperature on the importance of space-charge phenomenon is also studied.
No takes yet. Share an insight, caveat, or question.
Vedel et al. (1984) studied this question.
Synapse has enriched one closely related paper. Consider it for comparative context: