Gravitational corrections to electroweak vacuum decay: metric vs. Palatini
arXiv:2212.03052 · doi:10.1016/j.physletb.2023.137885
Abstract
We consider the standard Einstein-Hilbert-Higgs action where the Higgs field couples nonminimally with gravity via the term , and investigate the stability of the electroweak vacuum in the presence of gravitational corrections in both the metric and Palatini formulations of gravity. In order to identify the differences between the two formalisms analytically, we follow a perturbative approach in which the gravitational corrections are taken into consideration via a leading order expansion in the gravitational coupling constant. Our analysis shows that in the Palatini formalism, the well-known effect of gravity suppressing the vacuum decay probability, becomes milder in comparison with the metric case for any value of the nonminimal coupling . Furthermore, we have found that in the Palatini formalism, the positivity of the gravitational corrections, which is a necessary requirement for the unitarity of the theory, entails the lower bound .
typos corrected
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Cited by in corpus (10)
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- Gravity-improved metastability bounds for the Type-I Seesaw Mechanism
- Beyond (and back to) Palatini quadratic gravity and inflation
- General Einstein-Cartan quadratic gravity with derivative couplings
- Natural inflation in Palatini
- Cosmic inflation in metric-affine gravity
- Inflationary assessment of Einstein-Cartan models