TITLE:
Galaxy Evolution by the Incompatibility between Dark Matter and Baryonic Matter
AUTHORS:
Ding-Yu Chung
KEYWORDS:
Galaxy Evolution, CDM, Dark Matter, MOND, Baryonic Matter, Incompatible Dark Matter, ICDM
JOURNAL NAME:
International Journal of Astronomy and Astrophysics,
Vol.4 No.2,
June
4,
2014
ABSTRACT: The paper derives the
galaxy evolution by the non-interacting (incompatibility) between dark matter
and baryonic matter in terms of the short-range separation between dark matter
and baryonic matter, so dark matter cannot contact baryonic matter. In the
conventional CDM (cold dark matter) model, dark matter and baryonic matter are
interactive (compatible), so dark matter can contact baryonic matter. However,
the conventional CDM model fails to account for the failure to detect dark
matter by the contact (interaction) between dark matter and baryonic matter,
the shortage of small galaxies, the abundance of spiral galaxies, the old age
of large galaxies, and the formation of thin spiral galaxies. The
non-interacting (incompatible cold dark matter) model can account for these
observed phenomena. The five periods of baryonic structure development in the
order of increasing non-interacting (incompatibility) are the free baryonic
matter, the baryonic droplet, the galaxy, the cluster, and the supercluster
periods.