Efeitos Não-Lineares: uma nova janela para o Universo primordial

Auteur/ices

DOI :

https://doi.org/10.47456/Cad.Astro.v7nEspecial.53347

Mots-clés :

Inflação, Formalismo Estocástico, Buracos Negros Primordiais, Colapso Estocástico.

Résumé

A compreensão do universo primordial é fundamental para conectar física de altas energias, cosmologia observacional e formação das estruturas cósmicas. Neste trabalho, discuto o formalismo estocástico aplicado à inflação e a cenários alternativos de colapso, destacando sua capacidade de acessar efeitos não-lineares na distribuição primordial de densidade. Apresento aplicações na produção de buracos negros primordiais (PBHs), incluindo o cenário do curvaton fortemente não-gaussiano, e discuto a estabilidade quântica de modelos colapsantes. Aponto ainda limitações conceituais do formalismo e perspectivas de investigação neste tópicos.

Biographie de l'auteur

  • Tays Miranda, École Normale Supérieure - PSL

    Tays Miranda (tays.miranda@phys.ens.fr) é pesquisadora de pós-doutorado (Junior Research Chair) em Paris. Sua pesquisa concentra-se na cosmologia do universo primordial, com ênfase em efeitos estocásticos.

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Publiée

2026-07-30

Comment citer

[1]
T. Miranda, « Efeitos Não-Lineares: uma nova janela para o Universo primordial », Cad. Astro., vol. 7, nᵒ Especial, p. 61–71, juill. 2026, doi: 10.47456/Cad.Astro.v7nEspecial.53347.