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.
Authors
- Rudnei O. Ramos (ORCID: https://orcid.org/0000-0001-8781-4928)
- Vahid Kamali (ORCID: https://orcid.org/0000-0003-2158-9742)
Institutions
- Bu-Ali Sina University (IR)
- Universidade do Estado do Rio de Janeiro (BR)
- Institute for Research in Fundamental Sciences (IR)
- McGill University (CA)
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