Critical Higgs inflation in a Viable Motivated Model

Abstract

An extension of the Standard Model with three right-handed neutrinos and a simple invisible axion model can account for all experimentally confirmed signals of new physics (neutrino oscillations, dark matter and baryon asymmetry) in addition to solving the strong CP problem, stabilizing the electroweak vacuum and satisfying all current observational bounds. We show that this model can also implement critical Higgs inflation, which corresponds to the frontier between stability and metastability of the electroweak vacuum. This leads to a value of the non-minimal coupling between the Higgs and the Ricci scalar that is much lower than the one usually quoted in Higgs inflation away from criticality. Then, an advantage is that the scale of perturbative unitarity breaking on flat spacetime can be very close to the Planck mass, where anyhow new physics is required. The higher dimensional operators are under control in this inflationary setup. The dependence of the cutoff on the Higgs background is also taken into account as appropriate when the Higgs is identified with the inflaton. Furthermore, critical Higgs inflation enjoys a robust inflationary attractor that makes it an appealing setup for the early universe. In the proposed model, unlike in the Standard Model, critical Higgs inflation can be realized without any tension with the observed quantities, such as the top mass and the strong coupling.

13 pages, 6 figures; v2: explanations and references added; v3: title changed and more explanations added (version accepted by PRD)

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• All-in-one Relaxion, a unified solution to five BSM puzzles
• Primordial Black Holes as Dark Matter through Higgs Criticality
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• Several Problems in Particle Physics and Cosmology Solved in One SMASH
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• Warm Inflation, Neutrinos and Dark matter: a minimal extension of the Standard Model
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• Axion-Sterile-Neutrino Dark Matter
• (Multi-field) Natural Inflation and Gravitational Waves
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• Hearing Higgs with Gravitational Wave Detectors
• Inflationary scenarios beyond the Standard Model