Phenomenology of Electroweak Symmetry Breaking from Theory Space
Nima Arkani-Hamed, Andrew G. Cohen, Thomas Gregoire, Jay G. Wacker
TL;DR
The paper develops theory-space (moose) constructions to realize electroweak symmetry breaking without supersymmetry, yielding naturally light Higgs bosons and perturbative TeV-scale new physics. It shows that a large top Yukawa can drive EWSB through calculable radiative corrections while collective symmetry breaking cancels one-loop quadratic divergences, making the Higgs sector natural up to a higher cutoff $\Lambda \sim 4\pi f$ with UV completion near $10$–$100$ TeV. The model predicts at least two light Higgs doublets, extra weak triplet/singlet scalars, and a stable dark-matter candidate from a geometric $\mathbb{Z}_4$ symmetry, plus a rich TeV-scale spectrum of heavy states that cancel divergences and modify collider phenomenology. The explicit $N=2$ torus realization provides concrete spectrum and coupling patterns, illustrating the mechanism and highlighting potential collider and cosmological implications as well as comparisons to supersymmetric approaches.
Abstract
Recently, a new class of realistic models for electroweak symmetry breaking have been constructed, without supersymmetry. These theories have naturally light Higgs bosons and perturbative new physics at the TeV scale. We describe these models in detail, and show that electroweak symmetry breaking can be triggered by a large top quark Yukawa coupling. A rich spectrum of particles is predicted, with a pair of light Higgs doublets accompanied by new light weak triplet and singlet scalars. The lightest of these new scalars is charged under a geometric discrete symmetry and is therefore stable, providing a new candidate for WIMP dark matter. At TeV energies, a plethora of new heavy scalars, gauge bosons and fermions are revealed, with distinctive quantum numbers and decay modes.
