Classicality of the primordial perturbations

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dc.creatorLyth, David H.
dc.creatorSeery, David
dc.date2006-07-28
dc.date2008-04-21
dc.date.accessioned2026-07-07T11:42:34Z
dc.date.available2026-07-07T11:42:34Z
dc.descriptionWe show that during inflation, a quantum fluctuation becomes classical at all orders if it becomes classical at first order. Implications are discussed.
dc.description4 pages, uses RevTeX4 LaTeX document class. v2: More details of the classicality argument, and an improved discussion of its implications. v3: matches version published in PLB
dc.identifierhttps://arxiv.org/abs/astro-ph/0607647
dc.identifierhttp://arxiv.org/abs/astro-ph/0607647
dc.identifierPhys.Lett.B662:309-313,2008
dc.identifierdoi:10.1016/j.physletb.2008.03.010
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200930
dc.subjectAstrophysics
dc.titleClassicality of the primordial perturbations
dc.typetext

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