Novel Effects in Electroweak Breaking from a Hidden Sector
By J. Espinosa, M. Quirós. 2007
185 citations recorded by the source corpus.
The Higgs boson offers a unique window to hidden sector fields S{sub i}, singlets under the standard model gauge group, via the renormalizable interactions |H|{sup 2}S{sub i}{sup 2}. We prove that such interactions can provide new patterns for electroweak breaking, including radiative breaking by dimensional transmutation consistent with CERN LEP bounds, and trigger the strong enough first-order phase transition required by electroweak baryogenesis.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/1db45ee0dd1045eae4c5e2e1833df214521206ba
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Citations in the corpus
- Building and testing models with extended Higgs sectors (2017, background): “[474, 475, 476, 477, 478, 479, 480, 481, 359] for recent in-depth studies which combine the requirement of the strong EWPT with the collider results.”
- Gravitational wave production by collisions: more bubbles (2008, background): “This result is especially interesting in the light of recent investigations [7, 8] that indicate that in the case of a first-order electroweak phase transition (obtained by a singlet sector [14, 15] or higher dimensional operators [16, 17, 18]) the peak frequency of the produced radiation is below t”
- Effective Action, Conformal Anomaly and the Issue of Quadratic Divergences (2007, methodology): “A similar model with extra scalar fields, but without right-chiral neutrinos is also considered in [ 8 ].”
- Testing electroweak baryogenesis with future colliders (2014, background): “This scenario of adding a singlet with a Z2 symmetry to the SM has been well-studied in a variety of different contexts [50–56].”
- Some cosmological implications of hidden sectors (2008, methodology): “In this way a mass scale is introduced via dimensional transmutation [2, 3].”
- Cosmological backgrounds of gravitational waves and eLISA/NGO: phase transitions, cosmic strings and other sources (2012, methodology): “(16), is due to the total κ = κφ + κv, since both the gradient energy of the Higgs field and the kinetic energy of the bulk fluid motions lead to anisotropic stresses when the bubbles collide.”