Influence of superhorizon scales on cosmological observables generated during inflation
[EN]In the framework known as stochastic inflation, the evolution of cosmological perturbations picks up a noise term. In this article we focus on the fact that in realistic applications of the model, the noise is actually coloured, which leads to memory effects of modes of different scales. We eval...
| Autores: | , , |
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| Formato: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2004 |
| País: | España |
| Recursos: | Universidad de Salamanca (USAL) |
| Repositorio: | GREDOS. Repositorio Institucional de la Universidad de Salamanca |
| OAI Identifier: | oai:gredos.usal.es:10366/169089 |
| Acesso em linha: | http://hdl.handle.net/10366/169089 |
| Access Level: | acceso abierto |
| Palavra-chave: | Fondo Cósmico de Microondas (teoría) Perturbaciones cosmológicas Inflación |
| Resumo: | [EN]In the framework known as stochastic inflation, the evolution of cosmological perturbations picks up a noise term. In this article we focus on the fact that in realistic applications of the model, the noise is actually coloured, which leads to memory effects of modes of different scales. We evaluate the two- and three-point correlation function for the simple toy model of a scalar field with cubic self-interactions in a fixed de Sitter background. We show that in the presence of coloured noise perturbations of observable scale preserve some memory of the super-horizon modes, as scale-dependent imprints in their statistical moments. In particular, we find a blue tilt of the power-spectrum on large scales, and an enhancement of intrinsic non-Gaussianity. |
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