Detection Prospects of Gravitational Waves from SU(2) Axion Inflation

Fuente: arXiv
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Autori principali: Badger, Charles, Duval, Hannah, Fujita, Tomohiro, Kuroyanagi, Sachiko, Romero-Rodríguez, Alba, Sakellariadou, Mairi
Natura: Preprint
Pubblicazione: 2024
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author Badger, Charles
Duval, Hannah
Fujita, Tomohiro
Kuroyanagi, Sachiko
Romero-Rodríguez, Alba
Sakellariadou, Mairi
author_facet Badger, Charles
Duval, Hannah
Fujita, Tomohiro
Kuroyanagi, Sachiko
Romero-Rodríguez, Alba
Sakellariadou, Mairi
contents We study detection prospects of a gravitational-wave background (GWB) sourced by SU(2) gauge fields considering all possible observational constraints. More precisely, we consider bounds set by cosmic microwave background measurements, primordial black hole overproduction, as well as backreaction of the gauge fields on the background evolution. Gravitational-waves data from the first three observing runs of the LIGO-Virgo-KAGRA Collaboration show no evidence for a GWB contribution from axion inflation. However, we are able to place conservative constraints on the parameters of the SU(2) inflation with current data. We investigate conditions on the inflationary potential that would lead to a detectable signal that evades astrophysical and cosmological constraints and discuss detection prospects for third generation networks.
format Preprint
id arxiv_https___arxiv_org_abs_2406_11742
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Detection Prospects of Gravitational Waves from SU(2) Axion Inflation
Badger, Charles
Duval, Hannah
Fujita, Tomohiro
Kuroyanagi, Sachiko
Romero-Rodríguez, Alba
Sakellariadou, Mairi
Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
We study detection prospects of a gravitational-wave background (GWB) sourced by SU(2) gauge fields considering all possible observational constraints. More precisely, we consider bounds set by cosmic microwave background measurements, primordial black hole overproduction, as well as backreaction of the gauge fields on the background evolution. Gravitational-waves data from the first three observing runs of the LIGO-Virgo-KAGRA Collaboration show no evidence for a GWB contribution from axion inflation. However, we are able to place conservative constraints on the parameters of the SU(2) inflation with current data. We investigate conditions on the inflationary potential that would lead to a detectable signal that evades astrophysical and cosmological constraints and discuss detection prospects for third generation networks.
title Detection Prospects of Gravitational Waves from SU(2) Axion Inflation
topic Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2406.11742