Natural Relaxation
arXiv:1510.00710 · doi:10.1142/S0217732316502151
Abstract
Motivated by natural inflation, we propose a relaxation mechanism consistent with inflationary cosmology that explains the hierarchy between the electroweak scale and Planck scale. This scenario is based on a selection mechanism that identifies the low scale dynamics as the one that is screened from UV physics. The scenario also predicts the near-criticality and metastability of the standard model vacuum state, explaining the Higgs boson mass observed at the LHC. Once Majorana right-handed neutrinos are introduced to provide a viable reheating channel, our framework yields a corresponding mass scale that allows for the seesaw mechanism as well as for standard thermal leptogenesis. We argue that considering singlet scalar dark matter extensions of the proposed scenario could solve the vacuum stability problem and discuss how the cosmological constant problem is possibly addressed.
Added a discussion on selection principle and expanded references
References in corpus (4)
Cited by in corpus (17)
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- Constraints on Relaxion Windows
- Dynamics of the cosmological relaxation after reheating
- Higgs relaxation after inflation
- Low-Scale D-term Inflation and the Relaxion
- Cosmological Relaxation through the Dark Axion Portal
- Relaxion Dark Matter
- Constraints on the relaxion mechanism with strongly interacting vector-fermions
- Relaxion window
- Towards the fate of the oscillating false vacuum
- Fast-Rolling Relaxion
- A warped relaxion
- Cosmological Relaxation from Dark Fermion Production
- Light Higgs Boson from a Pole Attractor
- Dynamical relaxation in 2HDM models
- Gravitational tests of electroweak relaxation
- Mixing Particle Production for Relaxion Mechanism