Early Objects in the Cosmic String Theory with Hot Dark Matter
R. Moessner, R. Brandenberger
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 1012M, which could be the hosts of high redshift quasars, are formed by a redshift of z=4.
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