Formation of High Redshift Objects in a Cosmic String Theory with Hot Dark Matter
arXiv:astro-ph/9510141 · doi:10.1093/mnras/280.3.797
Abstract
Using a modification of the Zel'dovich approximation adapted to hot dark matter, the accretion of such matter onto moving cosmic string loops is studied. It is shown that a large number of $10^{12}M_\odot$ nonlinear objects will be produced by a redshift of $z=4$. These objects could be the hosts of high redshift quasars.
21 pages, 1 figure, uses phyzzx and epsf macros