Self-Gravitating Three-Field Q-Ball Configurations: Spherical Solutions and Preliminary Dynamical Tests

This paper documents the post-publication self-gravitating extension of the RFL/QGT-C three-field candidate. A spherical boundary-value continuation was computed from G_T m^2=0.001 to 0.06. At the reference point G_T m^2=0.06, the solution gives omega/m=0.83637668, M_ADM=5.96699625, Q=5.09419054, N_min=0.50700610, and max(2G_T M/r)=0.49299390. The metric light-ring criterion is crossed on the computed interval, but N remains positive and no horizon is present in the static solution. A 1% and a 10% spherical perturbation were evolved and remained horizon-free during their short windows. Constraint-solved compressed initial data bracket N_min=0 near c=2.4575. The evidence supports numerical spherical configurations and short-window radial robustness for one parameter set. It does not demonstrate a black hole or singularity resolution, but provides a robust numerical framework for horizonless compact objects.