The curvature perturbation in a box
By D. Lyth. 2007
143 citations recorded by the source corpus.
The stochastic properties of cosmological perturbations are best defined through the Fourier expansion in a finite box. I discuss the reasons for that with reference to the curvature perturbation, and explore some issues arising from it.
Subfields: Astronomy and Astrophysics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/3cf7666f2522f8aa3500cbff3f0191838e7519bf
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In Astronomy and Astrophysics
In Statistical and Nonlinear Physics
Citations in the corpus
- Semiclassical relations and IR effects in de Sitter and slow-roll space-times (2010, result): “This interpretation also resembles some of the ideas in [38, 39].”