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Non-oscillatory no-scale inflation

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John Ellis, Dimitri V. Nanopoulos, Keith A. Olive, Sarunas Verner

Original languageEnglish
Article number052
JournalJournal of Cosmology and Astroparticle Physics
Issue number3
PublishedMar 2021

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Publisher Copyright: © 2021 IOP Publishing Ltd and Sissa Medialab. Copyright: Copyright 2021 Elsevier B.V., All rights reserved.

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We propose a non-oscillatory no-scale supergravity model of inflation (NO-NO inflation) in which the inflaton does not oscillate at the end of the inflationary era. Instead, the Universe is then dominated by the inflaton kinetic energy density (kination). During the transition from inflation to kination, the Universe preheats instantly through a coupling to Higgs-like fields. These rapidly annihilate and scatter into ultra-relativistic matter particles, which subsequently dominate the energy density, and reheating occurs at a temperature far above that of Big Bang Nucleosynthesis. After the electroweak transition, the inflaton enters a tracking phase as in some models of quintessential inflation. The model predictions for cosmic microwave background observables are consistent with Planck 2018 data, and the density of gravitational waves is below the upper bound from Big Bang Nucleosynthesis. We also find that the density of supersymmetric cold dark matter produced by gravitino decay is consistent with Planck 2018 data over the expected range of supersymmetric particle masses.

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