Seminars and Journal Clubs

Stability of the Electroweak Scale and Inflation

by Alberto Salvio (UAM)

Europe/Brussels
E/3rd floor-E.361 - Meeting room (E.361) (Marc de Hemptinne (chemin du Cyclotron, 2, Louvain-la-Neuve))

E/3rd floor-E.361 - Meeting room (E.361)

Marc de Hemptinne (chemin du Cyclotron, 2, Louvain-la-Neuve)

15
Description
The LHC has fixed the last Standard Model (SM) parameter, the mass of the Brout-Englert-Higgs boson, h. Now, we can study the predictions of the SM (appropriately extended to account for neutrino oscillations and dark matter) in a vast energy range, up to the Planck scale. Although the SM does not provide a dynamical explanation of electroweak symmetry breaking (EWSB), this analysis is important for at least two reasons. It gives us information about very high energies, which we cannot even dream to reach at particle colliders, and, even more importantly, it can also tell us whether the SM has other problems, besides those that are universally accepted as SM problems. We will discuss the currently most precise determination of the bound on the h mass that ensures our vacuum is stable up to Planck energies. We will find that we are very close to the border between stability and metastability, with a pronounced preference for the metastable scenario. This fact puts bounds on the possibility to trigger inflation through h and so points towards a beyond the SM explanation of inflation. Such an explanation as well as a dynamical origin of EWSB can be achieved, remarkably, in theories of all interactions (including gravity) where fundamental scales are absent: agravity.