Galaxy Formation -- a Condensation Process just after Recombination
Abstract
A scenario of galaxy formation is put forward which is a process of sudden condensation just after recombination. It is essentially based on the fact that the cosmic matter gas after recombination is a general relativistic Boltzmann gas which runs within a few years into a state very close to collision--dominated equilibrium. The mass spectrum of axially symmetric condensation "drops" extends from the lower limit M about solar masses to the upper limit M about solar masses. The lower limit masses are spheres whereas the upper limit masses are extremely thin pancakes. These pancakes contract within a time of about to fastly rotating spiral galaxies with ordinary proportions. In this final state they have a redshift z about 3. At an earlier time during their contraction they are higly active and are observed with a redshift z about 5.
Cite
@article{arxiv.gr-qc/9802051,
title = {Galaxy Formation -- a Condensation Process just after Recombination},
author = {Gerhard Lessner},
journal= {arXiv preprint arXiv:gr-qc/9802051},
year = {2010}
}
Comments
26 pages, 2 figures; to be published in Nuovo Cimento B, Vol.113