English

Higgsless Electroweak Symmetry Breaking from Theory Space

High Energy Physics - Phenomenology 2009-11-10 v2

Abstract

We investigate unitarity of W+WW^+W^- scattering in the context of theory space models of the form U(1)×[SU(2)]N×SU(2)N+1U(1)\times {[SU(2)]}^N\times SU(2)_{N+1}, which are broken down to U(1)EMU(1)_{EM} by non-linear Σ\Sigma fields, without the presence of a physical Higgs Boson. By allowing the couplings of the U(1) and the final SU(2)N+1SU(2)_{N+1} to vary, we can fit the WW and ZZ masses, and we find that the coefficient of the term in the amplitude that grows as E2/mW2E^2/m_W^2 at high energies is suppressed by a factor of (N+1)2(N+1)^{-2}. In the N+1N+1\to\infty limit the model becomes a 5-dimensional SU(2) gauge theory defined on an interval, where boundary terms at the two ends of the interval break the SU(2) down to U(1)EMU(1)_{EM}. These boundary terms also modify the Kaluza-Klein (KK) mass spectrum, so that the lightest KK states can be identified as the WW and ZZ bosons. The TT parameter, which measures custodial symmetry breaking, is naturally small in these models. Depending on how matter fields are included, the strongest experimental constraints come from precision electroweak limits on the SS parameter.

Keywords

Cite

@article{arxiv.hep-ph/0312324,
  title  = {Higgsless Electroweak Symmetry Breaking from Theory Space},
  author = {Roshan Foadi and Shrihari Gopalakrishna and Carl Schmidt},
  journal= {arXiv preprint arXiv:hep-ph/0312324},
  year   = {2009}
}

Comments

21 pages, 8 figures, JHEP format (published version, some minor clarifying sentences added)

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