Stability and UV completion of the Standard Model
arXiv:1507.08812
Abstract
The knowledge of the stability condition of the electroweak (EW) vacuum is of the greatest importance for our understanding of beyond Standard Model (BSM) physics. It is widely believed that new physics that lives at very high energy scales should have no impact on the stability analysis. This expectation has been recently challenged, but the results were controversial as new physics was given in terms of non-renormalizable higher order operators. Here we consider for the first time a renormalizable (toy) UV completion of the SM, and definitely show that such a decoupling does not take place. This result has important phenomenological consequences, providing a very useful test for BSM theories. In particular, it shows that speculations based on the so called "criticality" do not appear to be well founded.
Cited by in corpus (8)
- Dark matter and neutrino masses from a scale-invariant multi-Higgs portal
- UV (in)sensitivity of Higgs inflation
- Stability of the electroweak ground state in the Standard Model and its extensions
- SpecBit, DecayBit and PrecisionBit: GAMBIT modules for computing mass spectra, particle decay rates and precision observables
- Constraining the effective action by a method of external sources
- Stationary configurations of the Standard Model Higgs potential: electroweak stability and rising inflection point
- Conformal Standard Model with an extended scalar sector
- Running Non-Minimal Inflation with Stabilized Inflaton Potential