Kinetic Gauge Friction in Natural Inflation

Fuente: arXiv
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Autori principali: Michelotti, Martino, Quaglia, Rodrigo Gonzalez, Dimastrogiovanni, Ema, Fasiello, Matteo, Roest, Diederik
Natura: Preprint
Pubblicazione: 2024
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author Michelotti, Martino
Quaglia, Rodrigo Gonzalez
Dimastrogiovanni, Ema
Fasiello, Matteo
Roest, Diederik
author_facet Michelotti, Martino
Quaglia, Rodrigo Gonzalez
Dimastrogiovanni, Ema
Fasiello, Matteo
Roest, Diederik
contents We study an extension of the natural inflation model comprising a non-Abelian gauge sector coupled to the axion-inflaton kinetic term. We show how such non-minimal coupling serves as a source of friction for the rolling inflaton granting sixty or more $e$-folds of accelerated expansion for sub-Planckian values of the axion decay constant. The analysis of perturbations reveals a negative sound speed, thus signaling an instability. Implementing a Chern-Simons-type coupling between the inflaton and gauge sectors cures the instability by delivering a positive speed. We perform a numerical study of scalar and tensor perturbations for a fiducial set of parameters finding that the corresponding observables are compatible with current CMB bounds.
format Preprint
id arxiv_https___arxiv_org_abs_2411_19892
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Kinetic Gauge Friction in Natural Inflation
Michelotti, Martino
Quaglia, Rodrigo Gonzalez
Dimastrogiovanni, Ema
Fasiello, Matteo
Roest, Diederik
Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
High Energy Physics - Theory
We study an extension of the natural inflation model comprising a non-Abelian gauge sector coupled to the axion-inflaton kinetic term. We show how such non-minimal coupling serves as a source of friction for the rolling inflaton granting sixty or more $e$-folds of accelerated expansion for sub-Planckian values of the axion decay constant. The analysis of perturbations reveals a negative sound speed, thus signaling an instability. Implementing a Chern-Simons-type coupling between the inflaton and gauge sectors cures the instability by delivering a positive speed. We perform a numerical study of scalar and tensor perturbations for a fiducial set of parameters finding that the corresponding observables are compatible with current CMB bounds.
title Kinetic Gauge Friction in Natural Inflation
topic Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
High Energy Physics - Theory
url https://arxiv.org/abs/2411.19892