Four-year COBE normalization of inflationary cosmologies

dc.creatorBunn, Emory F
dc.creatorLiddle, Andrew R
dc.creatorWhite, Martin
dc.date1996-07-05
dc.date1996-08-01
dc.date.accessioned2026-07-07T12:01:03Z
dc.date.available2026-07-07T12:01:03Z
dc.descriptionWe supply fitting formulae enabling the normalization of slow-roll inflation models to the four-year COBE data. We fully include the effect of the gravitational wave modes, including the predicted relation of the amplitude of these modes to that of the density perturbations. We provide the normalization of the matter power spectrum, which can be directly used for large-scale structure studies. The normalization for tilted spectra is a special case. We also provide fitting functions for the inflationary energy scale of COBE-normalized models and discuss the validity of approximating the spectra by power-laws. In an Appendix, we extend our analysis to include models with a cosmological constant, both with and without gravitational waves.
dc.description5 pages LaTeX file, using RevTeX. A correction is made to the final fitting function, Eq.A5. This correction only affects models which have BOTH gravitational waves and a cosmological constant
dc.identifierhttps://arxiv.org/abs/astro-ph/9607038
dc.identifierhttp://arxiv.org/abs/astro-ph/9607038
dc.identifierPhys.Rev.D54:5917-5921,1996
dc.identifierdoi:10.1103/PhysRevD.54.R5917
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/206981
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleFour-year COBE normalization of inflationary cosmologies
dc.typetext

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