Reproducing Cosmic Microwave Background anisotropies with mixed isocurvature perturbations

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  • 2 April 2001
Abstract
Recently high quality data of the cosmic microwave background anisotropies have been published. In this work we show that this data can be very well fitted with fixed standard cosmological parameters if we enlarge somewhat the allowed space of initial conditions. We find also that initial conditions where the adiabatic mode dominates are favored.

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