Vanilla Inflation Predicts Negative Running

Fuente: arXiv
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Autores principales: Martin, Jerome, Ringeval, Christophe, Vennin, Vincent
Formato: Preprint
Publicado: 2024
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author Martin, Jerome
Ringeval, Christophe
Vennin, Vincent
author_facet Martin, Jerome
Ringeval, Christophe
Vennin, Vincent
contents We show that the simplest, and currently favoured, theoretical realizations of cosmic inflation yield a sharp prediction for the running of the spectral index $α_\mathrm{S}$. Using latest cosmological data, we compute its marginalized posterior probability distribution over the space of nearly 300 models of single-field slow-roll inflation. The most probable value is $α_\mathrm{S}=-6.3 \times 10^{-4}$, lying within the $98\%$ credible interval $-1.8 \times 10^{-3}< α_\mathrm{S}< -9.1 \times 10^{-5}$. Within the landscape of all the proposed slow-roll inflationary models, positive values for the running are therefore disfavoured at more than three-sigma.
format Preprint
id arxiv_https___arxiv_org_abs_2404_15089
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Vanilla Inflation Predicts Negative Running
Martin, Jerome
Ringeval, Christophe
Vennin, Vincent
Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
High Energy Physics - Theory
We show that the simplest, and currently favoured, theoretical realizations of cosmic inflation yield a sharp prediction for the running of the spectral index $α_\mathrm{S}$. Using latest cosmological data, we compute its marginalized posterior probability distribution over the space of nearly 300 models of single-field slow-roll inflation. The most probable value is $α_\mathrm{S}=-6.3 \times 10^{-4}$, lying within the $98\%$ credible interval $-1.8 \times 10^{-3}< α_\mathrm{S}< -9.1 \times 10^{-5}$. Within the landscape of all the proposed slow-roll inflationary models, positive values for the running are therefore disfavoured at more than three-sigma.
title Vanilla Inflation Predicts Negative Running
topic Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
High Energy Physics - Theory
url https://arxiv.org/abs/2404.15089