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Perturbatively including inhomogeneities in axion inflation
Axion inflation, i.e. an axion-like inflaton coupled to an Abelian gauge field through a Chern-Simons interaction, comes with a rich and testable phenomenology. This is particularly true in the strong backreaction regime, where the gauge field production heavily impacts the axion dynamics. Lattice s...
Autores principales: | , , |
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Lenguaje: | eng |
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2023
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Acceso en línea: | http://cds.cern.ch/record/2875964 |
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author | Domcke, Valerie Ema, Yohei Sandner, Stefan |
author_facet | Domcke, Valerie Ema, Yohei Sandner, Stefan |
author_sort | Domcke, Valerie |
collection | CERN |
description | Axion inflation, i.e. an axion-like inflaton coupled to an Abelian gauge field through a Chern-Simons interaction, comes with a rich and testable phenomenology. This is particularly true in the strong backreaction regime, where the gauge field production heavily impacts the axion dynamics. Lattice simulations have recently demonstrated the importance of accounting for inhomogeneities of the axion field in this regime. We propose a perturbative scheme to account for these inhomogeneities while maintaining high computational efficiency. Our goal is to accurately capture deviations from the homogeneous axion field approximation within the perturbative regime as well as self-consistently determine the onset of the non-perturbative regime. |
id | cern-2875964 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2023 |
record_format | invenio |
spelling | cern-28759642023-10-24T02:44:21Zhttp://cds.cern.ch/record/2875964engDomcke, ValerieEma, YoheiSandner, StefanPerturbatively including inhomogeneities in axion inflationhep-phParticle Physics - Phenomenologyastro-ph.COAstrophysics and AstronomyAxion inflation, i.e. an axion-like inflaton coupled to an Abelian gauge field through a Chern-Simons interaction, comes with a rich and testable phenomenology. This is particularly true in the strong backreaction regime, where the gauge field production heavily impacts the axion dynamics. Lattice simulations have recently demonstrated the importance of accounting for inhomogeneities of the axion field in this regime. We propose a perturbative scheme to account for these inhomogeneities while maintaining high computational efficiency. Our goal is to accurately capture deviations from the homogeneous axion field approximation within the perturbative regime as well as self-consistently determine the onset of the non-perturbative regime.arXiv:2310.09186IFIC/23-45FTUV-23-1005.0503UMN-TH-4226/23FTPI-MINN-23-18CERN-TH-2023-186oai:cds.cern.ch:28759642023-10-13 |
spellingShingle | hep-ph Particle Physics - Phenomenology astro-ph.CO Astrophysics and Astronomy Domcke, Valerie Ema, Yohei Sandner, Stefan Perturbatively including inhomogeneities in axion inflation |
title | Perturbatively including inhomogeneities in axion inflation |
title_full | Perturbatively including inhomogeneities in axion inflation |
title_fullStr | Perturbatively including inhomogeneities in axion inflation |
title_full_unstemmed | Perturbatively including inhomogeneities in axion inflation |
title_short | Perturbatively including inhomogeneities in axion inflation |
title_sort | perturbatively including inhomogeneities in axion inflation |
topic | hep-ph Particle Physics - Phenomenology astro-ph.CO Astrophysics and Astronomy |
url | http://cds.cern.ch/record/2875964 |
work_keys_str_mv | AT domckevalerie perturbativelyincludinginhomogeneitiesinaxioninflation AT emayohei perturbativelyincludinginhomogeneitiesinaxioninflation AT sandnerstefan perturbativelyincludinginhomogeneitiesinaxioninflation |