English

The Scale Factor Potential Approach to Inflation

General Relativity and Quantum Cosmology 2020-06-02 v2 Cosmology and Nongalactic Astrophysics High Energy Physics - Theory

Abstract

We propose a new approach to investigate inflation in a model-independent way, and in particular to elaborate the involved observables, through the introduction of the "scale factor potential". Through its use one can immediately determine the inflation end, which corresponds to its first (and global) minimum. Additionally, we express the inflationary observables in terms of its logarithm, using as independent variable the e-folding number. As an example, we construct a new class of scalar potentials that can lead to the desired spectral index and tensor-to-scalar ratio, namely ns0.965n_s \approx 0.965 and r104r \sim 10^{-4} for 60 ee-folds, in agreement with observations.

Keywords

Cite

@article{arxiv.1909.01982,
  title  = {The Scale Factor Potential Approach to Inflation},
  author = {David Benisty and Eduardo I. Guendelman and Emmanuel N. Saridakis},
  journal= {arXiv preprint arXiv:1909.01982},
  year   = {2020}
}

Comments

Accepted for Publishing in EPJC

R2 v1 2026-06-23T11:05:43.685Z