2008/06/11 by Adam Falkowski, M. Pérez-Victoria, Manuel Perez-Victoria · 4 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Brane #Cosmology and Gravitation Theories #Electroweak interaction #Gauge boson #Gauge symmetry #Gauge theory #Higgs boson #Higgs field #Mathematical physics #Particle physics #Particle physics theoretical and experimental studies #Physics #Randall–Sundrum model #Scalar field #Symmetry breaking #Technicolor #Theoretical physics #hep-ph
paper · pdf · doi:10.1088/1126-6708/2008/12/107
published as JHEP 0812:107,2008 · 32 pages, a few figures
arxiv created 2008/06/11 · openalex publication_date 2008/12/29 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We extend the 5D gauge-higgs scenario to the soft-wall framework where the IR brane is replaced by a smoothly decaying warp factor. The electroweak symmetry of the Standard Model is embedded in a larger symmetry group whose gauge bosons propagate in the bulk of a warped fifth dimension. This gauge symmetry is partly broken by UV boundary conditions and by a condensate of a bulk scalar field. The Higgs boson lives partly in the 5th component of the gauge field, and partly in the the bulk scalar. The Higgs potential is not UV sensitive if the condensate vanishes fast enough in the UV region. The soft-wall realization opens new possibilities for the spectrum and the couplings of the Kaluza-Klein resonances. We study two particular soft-wall backgrounds: one with resonances whose masses follow the linear Regge trajectory, and another with a continuum above a mass gap. We find that constraints on the Kaluza-Klein scale from electroweak precision tests are less severe than in analogous models with the IR brane. For the linear spectrum the typical constraint on the lightest resonance mass is 2 TeV, while the continuum is allowed to start below 1 TeV.