Massive neutrinos and the problem of the dark matter in spiral galaxies

Abstract

Using data on rotation curves of 134 spiral galaxies we have calculated the possible value of the tau neutrino mass. We have shown that this mass could explain the nature of the dark matter in spiral galaxies.

7 pages, plain TeX, submitted to the Proceedings of the XI National Conference of Yugoslav Astronomers, to be held in Belgrade, October 9th to 12th, 1996