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arXiv:1502.01334·v3·Cosmology and Nongalactic Astrophysics

Dynamically Induced Planck Scale and Inflation

Kristjan Kannike🇪🇪 · Gert Hütsi🇪🇪 · Liberato Pizza🇮🇹 · Antonio Racioppi🇪🇪 · Martti Raidal🇪🇪 · Alberto Salvio🇪🇸 · Alessandro Strumia🇮🇹

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Abstract

Theories where the Planck scale is dynamically generated from dimensionless interactions provide predictive inflationary potentials and super-Planckian field variations. We first study the minimal single-field realisation in the low-energy effective field theory limit, finding the predictions for the spectral index and for the tensor-to-scalar ratio, which can be reduced down to in presence of large couplings. Next we consider agravity as a dimensionless quantum gravity theory finding a multi-field inflation that converges towards an attractor trajectory that predicts and , interpolating between the quadratic and Starobinsky inflation. These theories relate the smallness of the weak scale to the smallness of inflationary perturbations: both arise naturally because of small couplings, implying a reheating temperature of GeV. A measurement of by Keck/Bicep3 would give us information on quantum gravity in the dimensionless scenario.

Comments: 29 pages, 5 figures. v3: final published version

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