期刊
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
卷 -, 期 12, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2007/12/016
关键词
cosmological perturbation theory; inflation; physics of the early universe
The stochastic properties of cosmological perturbations are best defined through the Fourier expansion in afinite box. I discuss the reasons for that with reference to the curvature perturbation, and explore some issues arising from it.
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