Can the neutrino picture be revived? QSO constraints revisited

Details Can the neutrino picture be revived? QSO constraints revisited Can the neutrino picture be revived? QSO constraints revisited

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...267....1b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 267, no. 1, p. 1-10.

Astronomy and Astrophysics

Astrophysics

14

Astronomical Models, Galactic Evolution, Neutrinos, Quasars, Dark Matter, Red Shift

Scientific paper

The constraints are discussed that can be set on the hot dark matter (HDM) picture for the formation of large-scale structure from the existence of QSOs at various redshifts. The model is described by a single parameter on which a firm limit is set independently of the uncertainty in the problem. It is found that conservative limits on the number density of QSOs do not rule out the HDM model for the spherical density threshold.

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