Deformations of Starobinsky Inflation in No-Scale SU(5) and SO(10) GUTs

TL;DR

This paper explores how deformations of Starobinsky inflation within no-scale SU(5) and SO(10) GUT frameworks can better fit recent CMB data, addressing constraints from particle physics and cosmology.

Contribution

It introduces deformations of Starobinsky inflation in no-scale GUT models, showing their potential to reconcile inflation predictions with recent observational data.

Findings

SU(5) with CMSSM-like SUSY breaking struggles to meet all constraints.

Pure gravity-mediated SUSY breaking in SU(5) fits constraints more easily.

Deformations reduce dependence on initial conditions for inflation.

Abstract

The original Starobinsky $R + R^2$ model of inflation is consistent with Planck and other measurements of the CMB, but recent results from the ACT and SPT Collaborations hint that the tilt of scalar perturbations may be in tension with the prediction of the Starobinsky model. No-scale models of inflation can reproduce the predictions of the Starobinsky model, but also provide a framework for incorporating deformations that could accommodate more easily the ACT and SPT data. We discuss this possibility in the contexts of SU(5) GUTs, taking into account the constraints on these models imposed by the longevity of the proton, the cold dark matter density and the measured value of the Higgs boson. We find that SU(5) with a CMSSM-like pattern of soft supersymmetry breaking has difficulty in accommodating all the constraints, whereas SU(5) with pure gravity-mediated supersymmetry breaking can accommodate them easily. We also consider two SO(10) symmetry-breaking patterns that can accommodate the ACT and SPT data. In both the SU(5) and SO(10) models, the deformations avoid issues associated with large initial field values in the Starobinsky model: in particular, the total number of e-folds is largely independent of the initial conditions.