Shaft Inflation and the Planck satellite observations

TL;DR

This paper introduces a new family of inflation models with scalar potentials that transition from monomial near the origin to a plateau at large field values, aligning well with observations and allowing for potentially observable tensor modes.

Contribution

The paper presents a novel inflation model family derived from supersymmetry with a potential interpolating between monomial and plateau forms, matching observational data without fine-tuning.

Findings

Models agree with latest cosmological observations.

Potential for observable tensor modes in future experiments.

No fine-tuning required for compatibility with data.

Abstract

A new family of inflation models is introduced and studied. The models are characterised by a scalar potential which, far from the origin, approaches an inflationary plateau in a power-law manner, while near the origin becomes monomial, as in chaotic inflation. The models are obtained in the context of global supersymmetry starting with a superpotential, which interpolates from a generalised monomial to an O'Raifearteagh form for small to large values of the inflaton field respectively. It is demonstrated that the observables obtained, such as the scalar spectral index, its running and the tensor to scalar ratio, are in excellent agreement with the latest observations, without any fine-tuning. Moreover, by widening mildly the shaft in field space, it is shown that sizable tensors can be generated, which may well be observable in the near future.