Light inflaton model in a metastable Universe

Abstract

We minimally extend the SM with a Z${}_2$ symmetric potential containing a single scalar field, serving as our inflaton with a quartic self-coupling. In the model we have symmetry breaking in both sectors, and with the addition of an inflaton-Higgs portal, the Universe is able to efficiently reheat via 2-2 inflaton-Higgs scattering. Assuming that the Universe with a positive cosmological constant should be metastable, only one particular symmetry breaking pattern in the vacuum is possible, without the need to finely-tune the Higgs' quartic self-coupling. Inflaton with masses in the range $O(10^{-3})\le m_{\chi }\le m_h$ and mixing angles that span ${\theta }_m^2=O(10^{-11}-10^{-2})$ evade all current cosmological, experimental and stability constraints required for a metastable EW vacuum. Upgraded particle physics experiments may be able to probe the parameter space with ${\theta }_m^2\ge O(10^{-4})$, where we would observe trilinear Higgs couplings suppressed by up to $2\%$ compared to the SM value. However to access the parameter space of very weakly-coupled inflaton, we rely on the proposals to build experiments that target the hidden sector.

22 pages, 2 figures Version accepted in PRD, improved plots

References in corpus (4)

• Cosmological implications of the Higgs mass measurement
• Discovering New Light States at Neutrino Experiments
• On gravitational and thermal corrections to vacuum decay
• Inflaton mass in the nuMSM inflation