ar X iv : h ep - p h / 96 08 37 1 v 1 1 9 A ug 1 99 6 LBNL - 39251 Strong WW Scattering

Chiral lagrangians provide a model independent description of the strongly interacting symmetry breaking sector. In this work it is first reviewed the LHC sensitivity to the chiral parameters (in the hardest case of non-resonant low-energy WW scattering). Later it is shown how to reproduce or predict the resonance spectrum by means of dispersion theory and the inverse amplitude method. We present a parameter space scan that covers many different strong WW scattering scenarios. Talk presented at the: 1996 DPF/DPB Summer Study on New Directions for High-Energy Physics. (Snowmass 96). This work was supported by the Director, Office of Energy Research, Office of High Energy and Nuclear Physics, Division of High Energy Physics of the U.S. Department of Energy under Contract DE-AC03-76SF00098. Complutense del Amo fellow. On leave of absence from Departamento de F́ısica Teórica. Univ. Complutense. 28040 Madrid, Spain.