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arXiv:1608.05414·v2·High Energy Physics — Phenomenology

Unifying inflation with the axion, dark matter, baryogenesis and the seesaw mechanism

Guillermo Ballesteros🇫🇷 · Javier Redondo🇪🇸 · Andreas Ringwald🇩🇪 · Carlos Tamarit🇬🇧

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Abstract

A minimal extension of the Standard Model (SM) with a single new mass scale and providing a complete and consistent picture of particle physics and cosmology up to the Planck scale is presented. We add to the SM three right-handed SM-singlet neutrinos, a new vector-like color triplet fermion and a complex SM singlet scalar that stabilises the Higgs potential and whose vacuum expectation value at GeV breaks lepton number and a Peccei-Quinn symmetry simultaneously. Primordial inflation is produced by a combination of (non-minimally coupled to the scalar curvature) and the SM Higgs. Baryogenesis proceeds via thermal leptogenesis. At low energies, the model reduces to the SM, augmented by seesaw-generated neutrino masses, plus the axion, which solves the strong CP problem and accounts for the dark matter in the Universe. The model predicts a minimum value of the tensor-to-scalar ratio , running of the scalar spectral index , the axion mass and cosmic axion background radiation corresponding to an increase of the effective number of relativistic neutrinos of . It can be probed decisively by the next generation of cosmic microwave background and axion dark matter experiments.

Comments: 7 pages, 2 figures

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