Astronomy and Astrophysics – Astrophysics
Scientific paper
1996-01-28
Phys.Rev.D53:3011-3016,1996
Astronomy and Astrophysics
Astrophysics
18 pages, 5 figures, to appear in Phys. Rev. D
Scientific paper
10.1103/PhysRevD.53.3011
We present a re-analysis of the cosmic confusion hypothesis, elucidating the degree to which ``confusion'' can be expected to hold in a class of flat, adiabatic models. This allows us to devise a simple and accurate fitting function for the height of the first peak in the radiation power spectrum in a wide range of inflationary inspired models. The range preferred by current data is given, together with a discussion of the impact of measurements of the peak height on constraining models of structure formation.
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