Some inflationary models under the light of Planck 2018 results

Fuente: arXiv
Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Pozo, Daniel, Zambrano, Jordan, Villegas, Ismael, Hernández-Jiménez, Rafael, Rojas, Clara
Format: Preprint
Veröffentlicht: 2023
Schlagworte:
Online-Zugang:
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
_version_ 1866917651998048256
author Pozo, Daniel
Zambrano, Jordan
Villegas, Ismael
Hernández-Jiménez, Rafael
Rojas, Clara
author_facet Pozo, Daniel
Zambrano, Jordan
Villegas, Ismael
Hernández-Jiménez, Rafael
Rojas, Clara
contents In this work we study four well-known inflationary scenarios that are reported by the most recent Planck observations: Natural inflation, Hilltop quartic inflation, Starobinsky inflationary model, and Large field power-law potentials $V(ϕ)\sim ϕ^{p}$, considering $p=\sfrac{2}{3}, \sfrac{4}{3}$. The analysis is done using both the slow-roll approximation and the numerical solution to the background and perturbation equations. We show that the numerical solution improved the precision of these models with respect to the contour plot $r$ vs. $n_\sca$, having a lower $r$ in each model compared to the value calculated from the slow-roll approximation.
format Preprint
id arxiv_https___arxiv_org_abs_2311_04683
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Some inflationary models under the light of Planck 2018 results
Pozo, Daniel
Zambrano, Jordan
Villegas, Ismael
Hernández-Jiménez, Rafael
Rojas, Clara
General Relativity and Quantum Cosmology
In this work we study four well-known inflationary scenarios that are reported by the most recent Planck observations: Natural inflation, Hilltop quartic inflation, Starobinsky inflationary model, and Large field power-law potentials $V(ϕ)\sim ϕ^{p}$, considering $p=\sfrac{2}{3}, \sfrac{4}{3}$. The analysis is done using both the slow-roll approximation and the numerical solution to the background and perturbation equations. We show that the numerical solution improved the precision of these models with respect to the contour plot $r$ vs. $n_\sca$, having a lower $r$ in each model compared to the value calculated from the slow-roll approximation.
title Some inflationary models under the light of Planck 2018 results
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2311.04683