Clustering of the Relic Neutrinos and the Velocity Dispersion in a Cluster of Galaxies

Details Clustering of the Relic Neutrinos and the Velocity Dispersion in a Cluster of Galaxies Clustering of the Relic Neutrinos and the Velocity Dispersion in a Cluster of Galaxies

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pthph..65..374s&link_type=abstract

Progress of Theoretical Physics, Vol. 65, No. 1, pp. 374-377

Physics

8

Scientific paper

Clustering of the cosmological relic neutrinos into a cluster of
galaxies is investigated. In order to explain the missing mass in
typical clusters of galaxies such as Virgo and Coma, the neutrino mass
must be larger than ˜20 eV.

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