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[en] If one flavour of neutrino and antineutrino of mass m/sub upsilon/ is responsible for the non-luminous matter in the outer parts of galaxies, one can obtain firm lower limits on the value of m/sub upsilon/ from the observed distribution of dark matter. Note that the method described here does not depend on the actual coarse-grained phase-space distribution of neutrinos in galaxies (except for assuming isotropy). Another approach to the problem with the same advantage is presented
Source
Kolb, E.W.; Turner, M.S.; Lindley, D.; Olive, K.; Seckel, D; p. 510-511; ISBN 0-226-45032-5; 
; 1986; p. 510-511; University of Chicago Press; Chicago, IL (USA)
; 1986; p. 510-511; University of Chicago Press; Chicago, IL (USA)