ON THE NEUTRINO MASS AND THE HIDDEPI MASS IN CELESTIAL BODIES

We continually use the phenomenological of the galaxy with two constituents (v+B) as in a previous paper ^1] and uniformly handle S galaxy, E galaxy, etc. through the normalization method. At the same time, we extend this model from degenerate condition to isoentropic condition and from low temperature to high temperature. Thus, on a much more perfect foundation it is indirectly verified that the massive neutrino can account for the missing mass hidden in different celestial scales between galaxy and galactic cluster, but it can not rule out the possibiilty that there are some new massive fermions which are lighter than neutrino. Besides, in this paper we handle 21 samples of Sc galaxy yet, and obtain the average upper limit (15 eV.) of m_v. Because the spherically symmetric model is insufficient for calculation of m_v, we will progres sively research the non-spherically symmetric model, in another paper.