The new discussion of a neutrino mass and issues in the formation of large-scale structure

Details The new discussion of a neutrino mass and issues in the formation of large-scale structure The new discussion of a neutrino mass and issues in the formation of large-scale structure

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..222..521m&link_type=abstract

In: After the first three minutes; Proceedings of the 1st Astrophysics Workshop, Univ. of Maryland, College Park, Oct. 15-17, 19

Astronomy and Astrophysics

Astrophysics

Cosmology, Dark Matter, Leptons, Neutrinos, Universe, Astronomical Models, Galactic Evolution, Quasars, Topology

Scientific paper

It is argued that the discrepancy between the large-scale structure predicted by cosmological models with neutrino mass (hot dark matter) do not differ drastically from the observed structure. Evidence from the correlation amplitude, nonlinearity and the onset of galaxy formation, large-scale streaming velocities, and the topology of large-scale structure is considered. Hot dark matter models seem to be as accurate predictors of the large-scale structure as are cold dark matter models.

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