The curvature perturbation in a box

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dc.creatorLyth, David H.
dc.date2007-07-03
dc.date2008-02-15
dc.date.accessioned2026-07-07T11:17:27Z
dc.date.available2026-07-07T11:17:27Z
dc.descriptionThe 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.
dc.descriptionas published
dc.identifierhttps://arxiv.org/abs/0707.0361
dc.identifierhttp://arxiv.org/abs/0707.0361
dc.identifierJCAP0712:016,2007
dc.identifierdoi:10.1088/1475-7516/2007/12/016
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193013
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleThe curvature perturbation in a box
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