Direct Higgs-gravity interaction and stability of our Universe
arXiv:1905.02975 · doi:10.1103/PhysRevD.99.096029
Abstract
The Higgs effective potential becomes unstable at approximately GeV, and if only standard model interactions are considered, the lifetime of the electroweak vacuum turns out to be much larger than the age of the Universe . It is well known, however, that is extremely sensitive to the presence of unknown new physics: the latter can enormously lower . This poses a serious problem for the stability of our Universe, demanding for a physical mechanism that protects it from a disastrous decay. We have found that there exists a universal stabilizing mechanism that naturally originates from the nonminimal coupling between gravity and the Higgs boson. As this Higgs-gravity interaction necessarily arises from the quantum dynamics of the Higgs field in a gravitational background, this stabilizing mechanism is certainly present. It is not related to any specific model, being rather natural and universal as it comes from fundamental pillars of our physical world: gravity, the Higgs field, the quantum nature of physical laws.
5 pages, 4 figures
References in corpus (11)
- The Standard Model Higgs boson as the inflaton
- Combined Measurement of the Higgs Boson Mass in Collisions at and 8 TeV with the ATLAS and CMS Experiments
- Cosmological implications of the Higgs mass measurement
- The lifetime of the electroweak vacuum and sensitivity to Planck scale physics
- Consistent Use of the Standard Model Effective Potential
- Top mass determination, Higgs inflation, and vacuum stability
- Consistent Use of Effective Potentials
- On the gauge dependence of the Standard Model vacuum instability scale
- Critical behavior of the PT-symmetric quantum field theory
- Impact of New Physics on the EW vacuum stability in a curved spacetime background
- Effective potential and vacuum stability