Abstract
After a complement to previous papers on the gauge invariance of the Boltzmann collisional operator, we compare a recent homogeneous set of data on radio-QSOs, including angular sizes and bending of lobes, with what is expected from either our new cosmological gauge model or several conventional models. It is shown that the new gauge model provides a much better fit to the angular size distribution versus redshift than the Friedman model with q0=1 /2, and similarly to the bending, thanks to crude hypotheses on the mechanisms involved with the formation of jets.
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