Starobinsky-like inflation and soft-SUSY breaking
arXiv:1903.08448 · doi:10.1007/JHEP05(2019)211
Abstract
We study a version of Starobinsky-like inflation in no-scale supergravity (SUGRA) where a Polonyi term in the hidden sector breaks supersymmetry (SUSY) after inflation, providing a link between the gravitino mass and inflation. We extend the theory to the visible sector and calculate the soft-SUSY breaking parameters depending on the modular weights in the superpotential and choice of Kähler potential. We are led to either no-scale SUGRA or pure gravity mediated SUSY breaking patterns, but with inflationary constraints on the Polonyi term setting a strict upper bound on the gravitino mass TeV. Since gaugino masses are significantly lighter than , this suggests that SUSY may be discovered at the LHC or FCC.
References in corpus (19)
- Inflationary Cosmology
- Superconformal Symmetry, NMSSM, and Inflation
- New models of chaotic inflation in supergravity
- General inflaton potentials in supergravity
- Possible Signals of Wino LSP at the Large Hadron Collider
- Solving the -Problem in Hybrid Inflation with Heisenberg Symmetry and Stabilized Modulus
- Resurrecting No-Scale Supergravity Phenomenology
- Chaotic Inflation in Supergravity with Heisenberg Symmetry
- SUGRA chaotic inflation and moduli stabilisation
- Supersymmetric Moduli Stabilization and High-Scale Inflation
- SU(5) Grand Unification in Pure Gravity Mediation
- Sneutrino Inflation with -attractors
- Universality in Pure Gravity Mediation with Vector Multiplets
- Towards Matter Inflation in Heterotic String Theory
- Light Higgsinos in Pure Gravity Mediation
- Sneutrino Chaotic Inflation and Landscape
- Leptogenesis after Chaotic Sneutrino Inflation and the Supersymmetry Breaking Scale
- Polynomial Chaotic Inflation in Supergravity Revisited
- Chaotic Inflation from Nonlinear Sigma Models in Supergravity