Sigmoidal Inflation

Fuente: arXiv
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Autori principali: Díaz, E., Meza-Aldama, O.
Natura: Preprint
Pubblicazione: 2019
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author Díaz, E.
Meza-Aldama, O.
author_facet Díaz, E.
Meza-Aldama, O.
contents In this paper we present a new cosmological inflationary model which is constructed using the Ivanov-Salopek-Bond method with a logistic generating function. We derive the inflationary observables as well as the duration and temperature of the subsequent reheating epoch of our model exactly, with no need to recur to the slow roll approximation. The obtained scalar spectral index and tensor-to-scalar ratio of perturbations fall comfortably within the range of the measurements presented by the Planck collaboration. On the other hand, for the reheating era, our model predicts a relatively small number of e-folds and thus high temperatures, still within range of Planck's bounds.
format Preprint
id arxiv_https___arxiv_org_abs_1912_06312
institution arXiv
publishDate 2019
record_format arxiv
spellingShingle Sigmoidal Inflation
Díaz, E.
Meza-Aldama, O.
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
In this paper we present a new cosmological inflationary model which is constructed using the Ivanov-Salopek-Bond method with a logistic generating function. We derive the inflationary observables as well as the duration and temperature of the subsequent reheating epoch of our model exactly, with no need to recur to the slow roll approximation. The obtained scalar spectral index and tensor-to-scalar ratio of perturbations fall comfortably within the range of the measurements presented by the Planck collaboration. On the other hand, for the reheating era, our model predicts a relatively small number of e-folds and thus high temperatures, still within range of Planck's bounds.
title Sigmoidal Inflation
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/1912.06312