Super-horizon Perturbations and CMBA

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dc.creatorZeng, Ding-fang
dc.creatorGao, Yi-hong
dc.date2005-03-21
dc.date.accessioned2026-07-07T04:18:11Z
dc.date.available2026-07-07T04:18:11Z
dc.descriptionWe provided a gedanken experiment and argued that since observers inside a given Hubble volume could not detect the super horizon perturbation modes as real perturbations, these modes could only affect the average value of the cosmic microwave background (CMB), but not its anisotropy properties (CMBA) in that Hubble volume.
dc.description1 pages, 1 figures
dc.identifierhttps://arxiv.org/abs/hep-th/0503154
dc.identifierhttp://arxiv.org/abs/hep-th/0503154
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/53074
dc.subjectHigh Energy Physics - Theory
dc.titleSuper-horizon Perturbations and CMBA
dc.typetext

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