Mixed Cold-Hot Dark Matter Model with several Massive Neutrino Types
Dmitri Pogosyan, Alexei Starobinsky
Abstract
Mixed cold-hot dark matter cosmological models (CHDM) with Ωtot=1, approximately flat initial spectrum of adiabatic perturbations and 1, 2 or 3 types of massive neutrinos are compared and tested using recent observational data. The models with 2 or 3 neutrino types of equal mass permit as the best fit larger values of both the Hubble constant (H0 60 for 2 types, H0 65 for 3 types) and the total Ων (up to 0.3 for 3 types) than the model with 1 massive type. Also, they have less problems with abundances of early compact objects including Ly-α clouds.
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