Detection prospects of gravitational waves from SU(2) axion inflation

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. Published by the American Physical Society 2024

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2024-10-24
DOI
https://doi.org/10.1103/physrevd.110.084063
Citations
9
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
2.98

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article

Detection prospects of gravitational waves from SU(2) axion inflation

Mairi Sakellariadou, Sachiko Kuroyanagi, C. Badger, A. Romero et al.
9 citations
Physical review. D/Physical review. D.
Cosmology and Gravitation Theories
2.98
article

Detection prospects of gravitational waves from SU(2) axion inflation

Mairi Sakellariadou, Sachiko Kuroyanagi, C. Badger, A. Romero, Tomohiro Fujita, H. Duval
article en
9 citations

Abstract

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. Published by the American Physical Society 2024

Physical review. D/Physical review. D.Vol. 110(8)
Vrije Universiteit Brussel (BE), Consejo Superior de Investigaciones Científicas (ES), Waseda University (JP), King's College London (GB), Nagoya University (JP), The University of Tokyo (JP)
National Science Foundation, Comunidad de Madrid, Ministry of Education, Culture, Sports, Science and Technology, Academia Sinica, Fonds Wetenschappelijk Onderzoek, National Research Foundation of Korea, Vrije Universiteit Brussel, Centre National de la Recherche Scientifique, Ministerio de Ciencia e Innovación, MPS España, Vlaamse Interuniversitaire Raad, Ministry of Science and ICT, South Korea, Science and Technology Facilities Council, Australian Research Council, Japan Society for the Promotion of Science, Instituto Nazionale di Fisica Nucleare, Agencia Estatal de Investigación
Decent work and economic growth
Openalex Percentile: Top 9%
Cosmology and Gravitation Theories
2.98
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