Dr
Веселин Георгиев
(ИСФИ и Ронин Институт)
01/11/2019, 17:00
The growth of the density fluctuations is an important cosmological test. In the standard EdS model the growth of the density perturbations evolves with redshift $z$ like $(\frac{1}{1+z})^s$ with $s=1$. Without the introduction of dark matter, this is not fast enough to form galaxies and to account for the observed present-day inhomogeneities. This view is challenged in the present paper [1]...
