Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-07-03
JCAP0712:016,2007
Astronomy and Astrophysics
Astrophysics
as published
Scientific paper
10.1088/1475-7516/2007/12/016
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 the curvature perturbation, and explore some issues arising from
it.
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