Standard Model vacuum decay in a de Sitter Background
arXiv:1707.09175 · doi:10.1103/PhysRevD.97.025012
Abstract
We present a calculation of thick-wall Coleman-de-Luccia (CdL) bounces in the Standard Model effective potential in a de Sitter background. The calculation is performed including the effect of the bounce back-reaction on the metric, which we compare with the case of a fixed de-Sitter background, and with similar full-backreaction calculation in a model polynomial potential. The results show that the Standard Model potential exhibits non-trivial behavior: rather than a single CdL solution, there are multiple (non-oscillating) bounce solutions which may contribute to the decay rate. All the extra solutions found have higher actions than the largest amplitude solution, and thus would not contribute significantly to the decay rate, but their existence demonstrates that CdL solutions in the Standard Model potential are not unique, and the existence of additional, lower action, solutions cannot be ruled out. This suggests that a better understanding of the appearance and disappearance of CdL solutions in de Sitter space is needed to fully understand the vacuum instability issue in the Standard Model.
20 pages, 11 figures
References in corpus (19)
- Observation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC
- Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC
- Big-Bang Nucleosynthesis
- Cosmological implications of the Higgs mass measurement
- Spacetime curvature and the Higgs stability during inflation
- Gravitational corrections to Standard Model vacuum decay
- Thermal derivation of the Coleman-De Luccia tunneling prescription
- Top mass determination, Higgs inflation, and vacuum stability
- Electroweak Vacuum Stability in light of BICEP2
- On gravitational and thermal corrections to vacuum decay
- (Higgs) vacuum decay during inflation
- Gauge-Independent Scales Related to the Standard Model Vacuum Instability
- Probabilities in the landscape: The decay of nearly flat space
- Transitions Between de Sitter Minima
- Regulating Eternal Inflation II: The Great Divide
- The number of negative modes of the oscillating bounces
- Bounces with O(3) x O(2) symmetry
- The impact of non-minimally coupled gravity on vacuum stability
- Do metric fluctuations affect the Higgs dynamics during inflation?