| Texto completo | |
| Autor(es): |
de Souza, Rayff
;
Rodrigues, Jamerson G.
;
Siqueira, Clarissa
;
dos Santos, Felipe B. M.
;
Alcaniz, Jailson
Número total de Autores: 5
|
| Tipo de documento: | Artigo Científico |
| Fonte: | Journal of High Energy Physics; v. N/A, n. 4, p. 21-pg., 2025-04-16. |
| Resumo | |
A compelling way to address the inflationary period is via the warm inflation scenario, where the interaction of the inflaton field with other degrees of freedom affects its dynamics in such a way that slow-roll inflation is maintained by dissipative effects in a thermal bath. In this context, if a dark matter particle is coupled to the bath due to non-renormalizable interactions, the observed dark matter abundance may be produced during warm inflation via ultra-violet freeze-in. In this work, we propose applying this scenario in the framework of a U(1)B-L gauge extension of the Standard Model of Particle Physics, where we also employ the seesaw mechanism for generating neutrino masses. (AU) | |
| Processo FAPESP: | 21/01089-1 - Cherenkov Telescope Array: construção e primeiras descobertas |
| Beneficiário: | Luiz Vitor de Souza Filho |
| Modalidade de apoio: | Auxílio à Pesquisa - Projetos Especiais |