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Initial power spectrum shape

2004/12/01 by M. Douspis, Marian Douspis, Douspis, Marian
Earth and Planetary Sciences · Physics and Astronomy · #Astronomy and Astrophysical Research #Cosmology and Gravitation Theories #Geophysics and Gravity Measurements #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0412022

4 pages, Proceedings SF2A 2004 conference, Paris, eds.: F. Combes, D. Barret, T. Contini, F. Meynadier and L. Pagani

arxiv created 2004/12/01 · arxiv updated 2009/12/01

Abstract

Mainly used to set constraints on cosmological parameters, CMB anisotropies can give information on primordial universe. Unfortunately, initial conditions and late time cosmology are degenerated. I focus on the effect of the shape of the initial power spectrum of fluctuations on the cosmological parameter estimation from CMB temperature anisotropies. Strong constraints obtained using a priori knowledge of the initial spectrum disappear when the latter is let free.

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