Summary
In the universe dominated by massive neutrino dark matter we calculated the peculiar velocity and compared this with the large-scale bulk motion. The constraints on parameters of the universe, such as the index of density fluctuation spectrum and density contrast of large-scale structure, cosmological density parameter and Hubble parameter, and mass and degeneracy parameter of the dark-matter component, were discussed. The dependence of the window function was also discussed.
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Presented at the Second Italian-Korean Meeting on Relativistic Astrophysics held at the University of Rome and in Limone Piemonte in July 1989.
To speed up publication, proofs were not sent to the author and were supervised by the Scientific Committee.