Correlated mixtures of adiabatic and isocurvature cosmological perturbations
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The Cosmic Microwave Background (CMB) anisotropies measurements can provide many clues about the Universe. Although the common belief is that they will allow a very precise measurement of the cosmological parameters (that is, the current state of the Universe), they will alternatively give interesting informations about the state of the initial perturbations (that is, the state of the Universe at the end of inflation). In this paper, we study the observational consequences on the CMB anisotropies of some wide set of inital conditions, with a correlated mixture of adiabatic and isocurvature perturbations.
4 pages, 3 figures, to appear in the proceedings of the XXXVth Rencontres de Moriond "Energy densities in the Universe"
4 pages, 3 figures, to appear in the proceedings of the XXXVth Rencontres de Moriond "Energy densities in the Universe"