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Challenges in Supersymmetric Cosmology

Abstract : We discuss the possibility that inflation is driven by supersymmetry breaking with the scalar component of the goldstino superfield (sgoldstino) playing the role of the inflaton and charged under a gauged U(1) R-symmetry. Imposing a linear superpotential allows us to satisfy easily the slow-roll conditions, avoiding the so-called η-problem, and leads to an interesting class of small field inflation models, characterised by an inflationary plateau around the maximum of the scalar potential near the origin, where R-symmetry is restored with the inflaton rolling down to a minimum describing the present phase of the Universe. Inflation can be driven by either an For a D-term, while the minimum has a positive tuneable vacuum energy. The models agree with cosmological observations and in the simplest case predict a rather small tensor-to-scalar ratio of primordial perturbations. We propose a generalisation of Fayet-Iliopoulos model as a microscopic model leading to this class of inflation models at low energy.
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Submitted on : Wednesday, April 29, 2020 - 4:20:05 PM
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Ignatios Antoniadis, Auttakit Chatrabhuti. Challenges in Supersymmetric Cosmology. Symmetry, MDPI, 2020, 12 (3), pp.468. ⟨10.3390/sym12030468⟩. ⟨hal-02558488⟩



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