Early Objects in the Cosmic String Theory with Hot Dark Matter

Abstract

We study the accretion of hot dark matter onto moving cosmic string loops, using an adaptation of the Zeldovich approximation to HDM. We show that a large number of nonlinear objects of mass greater than $10^{12}M_\odot$, which could be the hosts of high redshift quasars, are formed by a redshift of $z=4$.

9 pages, includes 1 figure, uses Latex, psfig macro. To appear in Proceedings of the Workshop on `Cosmology at High and Low Redshifts', Hangzhou, China, October 1996