Thermal effects on warm chromoinflation

Abstract We explore a model of a pseudo-Nambu-Goldstone boson inflaton field coupled to a non-Abelian SU(2) gauge field. This model naturally leads to a warm inflation scenario, where the inflationary dynamics is dominated by thermal dissipation. In this work, we consider a scenario where the inflaton, an axion-like field, is coupled to the SU(2) gauge field, similar to chromoinflation models. Both the inflaton and the gauge field with a non-vanishing vacuum expectation value are coupled to a thermal radiation bath. We demonstrate that the presence of the thermal bath during warm chromoinflation induces a thermal plasma mass for the background gauge field. This thermal mass can significantly disrupt the dynamics of the background gauge field, thereby driving it to its trivial null solution.

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Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2025-01-01
DOI
https://doi.org/10.1088/1475-7516/2025/01/048
Citations
2
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
2.31
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article

Thermal effects on warm chromoinflation

Rudnei O. Ramos, Vahid Kamali
2 citations
Journal of Cosmology and Astroparticle Physics
Cosmology and Gravitation Theories
2.31
article

Thermal effects on warm chromoinflation

Rudnei O. Ramos, Vahid Kamali
article en
2 citations

Abstract

Abstract We explore a model of a pseudo-Nambu-Goldstone boson inflaton field coupled to a non-Abelian SU(2) gauge field. This model naturally leads to a warm inflation scenario, where the inflationary dynamics is dominated by thermal dissipation. In this work, we consider a scenario where the inflaton, an axion-like field, is coupled to the SU(2) gauge field, similar to chromoinflation models. Both the inflaton and the gauge field with a non-vanishing vacuum expectation value are coupled to a thermal radiation bath. We demonstrate that the presence of the thermal bath during warm chromoinflation induces a thermal plasma mass for the background gauge field. This thermal mass can significantly disrupt the dynamics of the background gauge field, thereby driving it to its trivial null solution.

Journal of Cosmology and Astroparticle PhysicsVol. 2025(01)
Bu-Ali Sina University (IR), Universidade do Estado do Rio de Janeiro (BR), Institute for Research in Fundamental Sciences (IR), McGill University (CA)
Openalex Percentile: Top 14%
Cosmology and Gravitation Theories
2.31
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