Majorana Neutrino Masses Can Save One Family Technicolour

Abstract

We make non perturbative estimates of the electroweak radiative correction parameter $S$ in dynamical symmetry breaking models with Majorana neutrino masses. The Majorana masses are treated as perturbations to a Non Local Chiral Model of the strong interactions. We argue that parameter ranges exist that would allow realistic values of $S$ and $T$ in one family Technicolour models.

Comments: 15 pages plus appended diagrams (ps), Latex, SHEP 92/93--23