In previous work the authors have analysed the global properties of an appr
oximate model of radiation damping for charged particles. This work is put
into context and related to the original motivation of understanding approx
imations used in the study of gravitational radiation damping. We examine t
o what extent the results obtained previously depend on the particular mode
l chosen. Comparisons are made with other models for gravitational and elec
tromagnetic fields. The relation of the kinetic model for which theorems we
re proved to certain many-particle models with radiation damping is exhibit
ed.