Constraints on Massive Neutrinos as Hot Dark Matter

Details Constraints on Massive Neutrinos as Hot Dark Matter Constraints on Massive Neutrinos as Hot Dark Matter

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nuphs..51..254m&link_type=abstract

Nuclear Physics B Proceedings Supplements, v. 51, p. 254-258.

Physics

Nuclear Physics

1

Scientific paper

This article highlights three astronomical observations that can constrain the masses of neutrinos as hot dark matter: high-redshift damped Lyα systems, the cosmic microwave background anisotropy, and gravitational lenses. Theoretical predictions and current constraints are summarized. More data are expected in the near future from all three types of observations.

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