
TL;DR
This paper proposes a novel inflationary scenario where R symmetry remains unbroken during inflation and is only broken afterwards, linking SUSY breaking, inflation, and dark matter in a high-scale SUSY framework.
Contribution
It introduces a model where late-time R symmetry breaking drives inflation and connects SUSY breaking with cosmological evolution, avoiding supergravity corrections.
Findings
Inflation driven by SUSY-breaking vacuum energy
Reheating via gravitino decay compatible with leptogenesis
Dark matter as thermally produced TeV winos
Abstract
Spontaneously broken supersymmetry (SUSY) and a vanishingly small cosmological constant imply that R symmetry must be spontaneously broken at low energies. Based on this observation, we suppose that, in the sector responsible for low-energy R symmetry breaking, a discrete R symmetry remains preserved at high energies and only becomes dynamically broken at relatively late times in the cosmological evolution, i.e., after the dynamical breaking of SUSY. Prior to R symmetry breaking, the Universe is then bound to be in a quasi-de Sitter phase---which offers a dynamical explanation for the occurrence of cosmic inflation. This scenario yields a new perspective on the interplay between SUSY breaking and inflation, which neatly fits into the paradigm of high-scale SUSY: inflation is driven by the SUSY-breaking vacuum energy density, while the chiral field responsible for SUSY breaking, the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
