Constraints on the tensor mode from large scale structure observations

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dc.creatorNovosyadlyj, B.
dc.creatorDurrer, R.
dc.creatorApunevych, S.
dc.date2000-11-07
dc.date.accessioned2026-07-07T01:56:27Z
dc.date.available2026-07-07T01:56:27Z
dc.descriptionObservational data on the large scale structure (LSS) of the Universe are used to establish an upper limit for the amplitude of the tensor mode marginalized over all other cosmological parameters within the class of adiabatic inflationary models. It is shown that the upper 1$σ$ limit for the contribution of a tensor mode to the COBE DMR data is T/S$<1$.
dc.description3 pages, to appear in the proceedings of the IAU Symposium 201, Manchester, 7-11 August 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0011149
dc.identifierhttp://arxiv.org/abs/astro-ph/0011149
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2006
dc.subjectAstrophysics
dc.titleConstraints on the tensor mode from large scale structure observations
dc.typetext

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